bib.bib

%% This BibTeX bibliography file was created using BibDesk.
%% http://bibdesk.sourceforge.net/

%% Created for Adam Beardsley at 2016-08-04 15:49:25 -0700 


%% Saved with string encoding Unicode (UTF-8) 



@article{Thyagarajan:2016,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2016ApJ...825....9T},
	Archiveprefix = {arXiv},
	Author = {{Thyagarajan}, N. and {Parsons}, A.~R. and {DeBoer}, D.~R. and {Bowman}, J.~D. and {Ewall-Wice}, A.~M. and {Neben}, A.~R. and {Patra}, N.},
	Date-Added = {2016-08-04 21:37:03 +0000},
	Date-Modified = {2016-08-04 21:37:03 +0000},
	Doi = {10.3847/0004-637X/825/1/9},
	Eid = {9},
	Eprint = {1603.08958},
	Journal = {\apj},
	Keywords = {cosmology: observations, dark ages, reionization, first stars, instrumentation: interferometers, large-scale structure of universe, radio continuum: galaxies, techniques: interferometric},
	Month = jul,
	Pages = {9},
	Title = {{Effects of Antenna Beam Chromaticity on Redshifted 21 cm Power Spectrum and Implications for Hydrogen Epoch of Reionization Array}},
	Volume = 825,
	Year = 2016,
	Bdsk-Url-1 = {http://dx.doi.org/10.3847/0004-637X/825/1/9}}

@article{Jacobs:2016,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2016ApJ...825..114J},
	Archiveprefix = {arXiv},
	Author = {{Jacobs}, D.~C. and {Hazelton}, B.~J. and {Trott}, C.~M. and {Dillon}, J.~S. and {Pindor}, B. and {Sullivan}, I.~S. and {Pober}, J.~C. and {Barry}, N. and {Beardsley}, A.~P. and {Bernardi}, G. and {Bowman}, J.~D. and {Briggs}, F. and {Cappallo}, R.~J. and {Carroll}, P. and {Corey}, B.~E. and {de Oliveira-Costa}, A. and {Emrich}, D. and {Ewall-Wice}, A. and {Feng}, L. and {Gaensler}, B.~M. and {Goeke}, R. and {Greenhill}, L.~J. and {Hewitt}, J.~N. and {Hurley-Walker}, N. and {Johnston-Hollitt}, M. and {Kaplan}, D.~L. and {Kasper}, J.~C. and {Kim}, H. and {Kratzenberg}, E. and {Lenc}, E. and {Line}, J. and {Loeb}, A. and {Lonsdale}, C.~J. and {Lynch}, M.~J. and {McKinley}, B. and {McWhirter}, S.~R. and {Mitchell}, D.~A. and {Morales}, M.~F. and {Morgan}, E. and {Neben}, A.~R. and {Thyagarajan}, N. and {Oberoi}, D. and {Offringa}, A.~R. and {Ord}, S.~M. and {Paul}, S. and {Prabu}, T. and {Procopio}, P. and {Riding}, J. and {Rogers}, A.~E.~E. and {Roshi}, A. and {Udaya Shankar}, N. and {Sethi}, S.~K. and {Srivani}, K.~S. and {Subrahmanyan}, R. and {Tegmark}, M. and {Tingay}, S.~J. and {Waterson}, M. and {Wayth}, R.~B. and {Webster}, R.~L. and {Whitney}, A.~R. and {Williams}, A. and {Williams}, C.~L. and {Wu}, C. and {Wyithe}, J.~S.~B.},
	Date-Added = {2016-08-04 21:31:10 +0000},
	Date-Modified = {2016-08-04 21:31:10 +0000},
	Doi = {10.3847/0004-637X/825/2/114},
	Eid = {114},
	Eprint = {1605.06978},
	Journal = {\apj},
	Keywords = {dark ages, reionization, first stars, methods: data analysis, techniques: interferometric},
	Month = jul,
	Pages = {114},
	Primaryclass = {astro-ph.IM},
	Title = {{The Murchison Widefield Array 21 cm Power Spectrum Analysis Methodology}},
	Volume = 825,
	Year = 2016,
	Bdsk-Url-1 = {http://dx.doi.org/10.3847/0004-637X/825/2/114}}

@article{Barry:2016,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2016MNRAS.461.3135B},
	Archiveprefix = {arXiv},
	Author = {{Barry}, N. and {Hazelton}, B. and {Sullivan}, I. and {Morales}, M.~F. and {Pober}, J.~C.},
	Date-Added = {2016-08-04 21:22:57 +0000},
	Date-Modified = {2016-08-04 21:23:03 +0000},
	Doi = {10.1093/mnras/stw1380},
	Eprint = {1603.00607},
	Journal = {\mnras},
	Month = sep,
	Pages = {3135-3144},
	Primaryclass = {astro-ph.IM},
	Title = {{Calibration requirements for detecting the 21 cm epoch of reionization power spectrum and implications for the SKA}},
	Volume = 461,
	Year = 2016,
	Bdsk-Url-1 = {http://dx.doi.org/10.1093/mnras/stw1380}}

@article{Lenc:2016,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2016arXiv160705779L},
	Archiveprefix = {arXiv},
	Author = {{Lenc}, E. and {Gaensler}, B.~M. and {Sun}, X.~H. and {Sadler}, E.~M. and {Willis}, A.~G. and {Barry}, N. and {Beardsley}, A.~P. and {Bell}, M.~E. and {Bernardi}, G. and {Bowman}, J.~D. and {Briggs}, F. and {Callingham}, J.~R. and {Cappallo}, R.~J. and {Carroll}, P. and {Corey}, B.~E. and {de Oliveira-Costa}, A. and {Deshpande}, A.~A. and {Dillon}, J.~S. and {Dwarkanath}, K.~S. and {Emrich}, D. and {Ewall-Wice}, A. and {Feng}, L. and {For}, B.-Q. and {Goeke}, R. and {Greenhill}, L.~J. and {Hancock}, P. and {Hazelton}, B.~J. and {Hewitt}, J.~N. and {Hindson}, L. and {Hurley-Walker}, N. and {Johnston-Hollitt}, M. and {Jacobs}, D.~C. and {Kapinska}, A.~D. and {Kaplan}, D.~L. and {Kasper}, J.~C. and {Kim}, H.-S. and {Kratzenberg}, E. and {Line}, J. and {Loeb}, A. and {Lonsdale}, C.~J. and {Lynch}, M.~J. and {McKinley}, B. and {McWhirter}, S.~R. and {Mitchell}, D.~A. and {Morales}, M.~F. and {Morgan}, E. and {Morgan}, J. and {Murphy}, T. and {Neben}, A.~R. and {Oberoi}, D. and {Offringa}, A.~R. and {Ord}, S.~M. and {Paul}, S. and {Pindor}, B. and {Pober}, J.~C. and {Prabu}, T. and {Procopio}, P. and {Riding}, J. and {Rogers}, A.~E.~E. and {Roshi}, A. and {Udaya Shankar}, N. and {Sethi}, S.~K. and {Srivani}, K.~S. and {Staveley-Smith}, L. and {Subrahmanyan}, R. and {Sullivan}, I.~S. and {Tegmark}, M. and {Thyagarajan}, N. and {Tingay}, S.~J. and {Trott}, C. and {Waterson}, M. and {Wayth}, R.~B. and {Webster}, R.~L. and {Whitney}, A.~R. and {Williams}, A. and {Williams}, C.~L. and {Wu}, C. and {Wyithe}, J.~S.~B. and {Zheng}, Q.},
	Date-Added = {2016-08-04 21:18:32 +0000},
	Date-Modified = {2016-08-04 22:47:58 +0000},
	Eprint = {1607.05779},
	Journal = {{ArXiv e-prints, arXiv:1607.05779}},
	Keywords = {Astrophysics - Astrophysics of Galaxies, Astrophysics - Instrumentation and Methods for Astrophysics},
	Month = jul,
	Title = {{Low frequency observations of linearly polarized structures in the interstellar medium near the south Galactic pole}},
	Year = 2016}

@article{DeBreuck:2000,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2000A%26AS..143..303D},
	Author = {{De Breuck}, C. and {van Breugel}, W. and {R{\"o}ttgering}, H.~J.~A. and {Miley}, G.},
	Date-Added = {2016-08-04 15:05:53 +0000},
	Date-Modified = {2016-08-04 15:06:02 +0000},
	Doi = {10.1051/aas:2000181},
	Eprint = {astro-ph/0002297},
	Journal = {\aaps},
	Keywords = {SURVEYS, GALAXIES: ACTIVE, RADIO CONTINUUM: GALAXIES},
	Month = apr,
	Pages = {303-333},
	Title = {{A sample of 669 ultra steep spectrum radio sources to find high redshift radio galaxies}},
	Volume = 143,
	Year = 2000,
	Bdsk-Url-1 = {http://dx.doi.org/10.1051/aas:2000181}}

@article{Hunstead:1991,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/1991AuJPh..44..743H},
	Author = {{Hunstead}, R.~W.},
	Date-Added = {2016-08-04 15:05:07 +0000},
	Date-Modified = {2016-08-04 15:05:07 +0000},
	Journal = {Australian Journal of Physics},
	Pages = {743},
	Title = {{Position and Flux Density Calibration at Molonglo}},
	Volume = 44,
	Year = 1991}

@article{Oort:1988,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/1988A%26AS...73..103O},
	Author = {{Oort}, M.~J.~A. and {Steemers}, W.~J.~G. and {Windhorst}, R.~A.},
	Date-Added = {2016-08-04 15:04:18 +0000},
	Date-Modified = {2016-08-04 15:04:23 +0000},
	Journal = {\aaps},
	Keywords = {Astronomical Catalogs, Cosmology, Radio Sources (Astronomy), Astronomical Maps, Centimeter Waves, Data Sampling, Radio Galaxies},
	Month = apr,
	Pages = {103-123},
	Title = {{A deep 92 CM survey of the Lynx area}},
	Volume = 73,
	Year = 1988}

@article{Greig:2016,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2016MNRAS.455.4295G},
	Archiveprefix = {arXiv},
	Author = {{Greig}, B. and {Mesinger}, A. and {Pober}, J.~C.},
	Date-Added = {2016-08-01 14:56:59 +0000},
	Date-Modified = {2016-08-01 14:56:59 +0000},
	Doi = {10.1093/mnras/stv2618},
	Eprint = {1509.02158},
	Journal = {\mnras},
	Keywords = {galaxies: high-redshift, intergalactic medium, cosmology: theory, dark ages, reionization, first stars, diffuse radiation, early Universe},
	Month = feb,
	Pages = {4295-4300},
	Title = {{Constraints on the temperature of the intergalactic medium at z = 8.4 with 21-cm observations}},
	Volume = 455,
	Year = 2016,
	Bdsk-Url-1 = {http://dx.doi.org/10.1093/mnras/stv2618}}

@article{Carroll:2016,
	Abstract = {Detection of the Epoch of Reionization HI signal requires a precise understanding of the intervening galaxies and AGN, both for instrumental calibration and foreground removal. We present a catalogue of 7394 extragalactic sources at 182 MHz detected in the RA=0 field of the Murchison Widefield Array Epoch of Reionization observation programme. Motivated by unprecedented requirements for precision and reliability we develop new methods for source finding and selection. We apply machine learning methods to self-consistently classify the relative reliability of 9490 source candidates. A subset of 7466 are selected based on reliability class and signal-to-noise ratio criteria. These are statistically cross-matched to four other radio surveys using both position and flux density information. We find 7369 sources to have confident matches, including 90 partially resolved sources that split into a total of 192 sub-components. An additional 25 unmatched sources are included as new radio detections. The catalogue sources have a median spectral index of −0.85. Spectral flattening is seen toward lower frequencies with a median of −0.71 predicted at 182 MHz. The astrometric error is 7'' compared to a 2.3' beam FWHM. The resulting catalogue covers ∼1400 deg2 and is complete to approximately 80 mJy within half beam power. This provides the most reliable discrete source sky model available to date in the MWA EoR0 field for precision foreground subtraction.},
	Author = {Carroll, P. A. and Line, J. and Morales, M. F. and Barry, N. and Beardsley, A. P. and Hazelton, B. J. and Jacobs, D. C. and Pober, J. C. and Sullivan, I. S. and Webster, R. L. and Bernardi, G. and Bowman, J. D. and Briggs, F. and Cappallo, R. J. and Corey, B. E. and de Oliveira-Costa, A. and Dillon, J. S. and Emrich, D. and Ewall-Wice, A. and Feng, L. and Gaensler, B. M. and Goeke, R. and Greenhill, L. J. and Hewitt, J. N. and Hurley-Walker, N. and Johnston-Hollitt, M. and Kaplan, D. L. and Kasper, J. C. and Kim, HS. and Kratzenberg, E. and Lenc, E. and Loeb, A. and Lonsdale, C. J. and Lynch, M. J. and McKinley, B. and McWhirter, S. R. and Mitchell, D. A. and Morgan, E. and Neben, A. R. and Oberoi, D. and Offringa, A. R. and Ord, S. M. and Paul, S. and Pindor, B. and Prabu, T. and Procopio, P. and Riding, J. and Rogers, A. E. E. and Roshi, A. and Shankar, N. Udaya and Sethi, S. K. and Srivani, K. S. and Subrahmanyan, R. and Tegmark, M. and Thyagarajan, Nithyanandan and Tingay, S. J. and Trott, C. M. and Waterson, M. and Wayth, R. B. and Whitney, A. R. and Williams, A. and Williams, C. L. and Wu, C. and Wyithe, J. S. B.},
	Date-Added = {2016-07-14 15:13:47 +0000},
	Date-Modified = {2016-07-14 15:13:51 +0000},
	Doi = {10.1093/mnras/stw1599},
	Eprint = {http://mnras.oxfordjournals.org/content/early/2016/07/08/mnras.stw1599.full.pdf+html},
	Journal = {Monthly Notices of the Royal Astronomical Society},
	Title = {A High Reliability Survey of Discrete Epoch of Reionization Foreground Sources in the MWA EoR0 Field},
	Url = {http://mnras.oxfordjournals.org/content/early/2016/07/08/mnras.stw1599.abstract},
	Year = {2016},
	Bdsk-Url-1 = {http://mnras.oxfordjournals.org/content/early/2016/07/08/mnras.stw1599.abstract},
	Bdsk-Url-2 = {http://dx.doi.org/10.1093/mnras/stw1599}}

@article{Offringa:2016,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2016MNRAS.458.1057O},
	Archiveprefix = {arXiv},
	Author = {{Offringa}, A.~R. and {Trott}, C.~M. and {Hurley-Walker}, N. and {Johnston-Hollitt}, M. and {McKinley}, B. and {Barry}, N. and {Beardsley}, A.~P. and {Bowman}, J.~D. and {Briggs}, F. and {Carroll}, P. and {Dillon}, J.~S. and {Ewall-Wice}, A. and {Feng}, L. and {Gaensler}, B.~M. and {Greenhill}, L.~J. and {Hazelton}, B.~J. and {Hewitt}, J.~N. and {Jacobs}, D.~C. and {Kim}, H.-S. and {Kittiwisit}, P. and {Lenc}, E. and {Line}, J. and {Loeb}, A. and {Mitchell}, D.~A. and {Morales}, M.~F. and {Neben}, A.~R. and {Paul}, S. and {Pindor}, B. and {Pober}, J.~C. and {Procopio}, P. and {Riding}, J. and {Sethi}, S.~K. and {Shankar}, N.~U. and {Subrahmanyan}, R. and {Sullivan}, I.~S. and {Tegmark}, M. and {Thyagarajan}, N. and {Tingay}, S.~J. and {Wayth}, R.~B. and {Webster}, R.~L. and {Wyithe}, J.~S.~B.},
	Date-Added = {2016-07-07 20:15:06 +0000},
	Date-Modified = {2016-07-07 20:15:13 +0000},
	Doi = {10.1093/mnras/stw310},
	Eprint = {1602.02247},
	Journal = {\mnras},
	Keywords = {methods: observational, techniques: interferometric, dark ages, reionization, first stars, radio continuum: general, radio lines: galaxies},
	Month = may,
	Pages = {1057-1070},
	Primaryclass = {astro-ph.IM},
	Title = {{Parametrizing Epoch of Reionization foregrounds: a deep survey of low-frequency point-source spectra with the Murchison Widefield Array}},
	Volume = 458,
	Year = 2016,
	Bdsk-Url-1 = {http://dx.doi.org/10.1093/mnras/stw310}}

@article{Dillon:2015b,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2015PhRvD..91b3002D},
	Archiveprefix = {arXiv},
	Author = {{Dillon}, J.~S. and {Tegmark}, M. and {Liu}, A. and {Ewall-Wice}, A. and {Hewitt}, J.~N. and {Morales}, M.~F. and {Neben}, A.~R. and {Parsons}, A.~R. and {Zheng}, H.},
	Date-Added = {2016-07-07 19:54:08 +0000},
	Date-Modified = {2016-07-07 19:54:08 +0000},
	Doi = {10.1103/PhysRevD.91.023002},
	Eid = {023002},
	Eprint = {1410.0963},
	Journal = {\prd},
	Keywords = {Observation and data reduction techniques, computer modeling and simulation, Interferometry, Intergalactic matter, quasar absorption and emission-line systems, Lyman forest, Observational cosmology},
	Month = jan,
	Number = 2,
	Pages = {023002},
	Title = {{Mapmaking for precision 21 cm cosmology}},
	Volume = 91,
	Year = 2015,
	Bdsk-Url-1 = {http://dx.doi.org/10.1103/PhysRevD.91.023002}}

@book{Loeb:2013,
	Author = {Loeb, A. and Furlanetto, S.R.},
	Date-Added = {2016-07-07 19:53:00 +0000},
	Date-Modified = {2016-07-07 19:53:00 +0000},
	Isbn = {9780691144924},
	Lccn = {2012018181},
	Publisher = {Princeton University Press},
	Series = {Princeton series in astrophysics},
	Title = {The First Galaxies in the Universe},
	Url = {https://books.google.com/books?id=hj98RVlnRRgC},
	Year = {2013},
	Bdsk-Url-1 = {https://books.google.com/books?id=hj98RVlnRRgC}}

@inproceedings{Noordam:2004,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2004SPIE.5489..817N},
	Author = {{Noordam}, J.~E.},
	Booktitle = {Ground-based Telescopes},
	Date-Added = {2016-06-30 16:59:12 +0000},
	Date-Modified = {2016-06-30 16:59:17 +0000},
	Doi = {10.1117/12.544262},
	Editor = {{Oschmann}, Jr., J.~M.},
	Month = oct,
	Pages = {817-825},
	Series = {\procspie},
	Title = {{LOFAR calibration challenges}},
	Volume = 5489,
	Year = 2004,
	Bdsk-Url-1 = {http://dx.doi.org/10.1117/12.544262}}

@article{Condon:1998,
	Author = {Condon, J. J. and Cotton, W. D. and Greisen, E. W. and Yin, Q. F. and Perley, R. A. and Taylor, G. B. and Broderick, J. J.},
	Date-Added = {2016-06-30 16:24:25 +0000},
	Date-Modified = {2016-06-30 16:24:29 +0000},
	Doi = {10.1086/300337},
	File = {:home/jline/.local/share/data/Mendeley Ltd./Mendeley Desktop/Downloaded/Condon et al. - 1998 - The NRAO VLA Sky Survey.pdf:pdf},
	Issn = {00046256},
	Journal = {The Astronomical Journal},
	Month = {may},
	Number = {5},
	Pages = {1693--1716},
	Title = {{The NRAO VLA Sky Survey}},
	Url = {http://stacks.iop.org/1538-3881/115/i=5/a=1693},
	Volume = {115},
	Year = {1998},
	Bdsk-Url-1 = {http://stacks.iop.org/1538-3881/115/i=5/a=1693},
	Bdsk-Url-2 = {http://dx.doi.org/10.1086/300337}}

@article{Lane:2012,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2012RaSc...47.0K04L},
	Archiveprefix = {arXiv},
	Author = {{Lane}, W.~M. and {Cotton}, W.~D. and {Helmboldt}, J.~F. and {Kassim}, N.~E.},
	Date-Added = {2016-06-30 16:24:17 +0000},
	Date-Modified = {2016-06-30 16:24:17 +0000},
	Doi = {10.1029/2011RS004941},
	Eid = {RS0K04},
	Eprint = {1205.4695},
	Journal = {Radio Science},
	Keywords = {ionospheric calibration, low-frequency radio astronomy, surveys},
	Month = jan,
	Pages = {RS0K04},
	Primaryclass = {astro-ph.IM},
	Title = {{VLSS redux: Software improvements applied to the Very Large Array Low-Frequency Sky Survey}},
	Volume = 47,
	Year = 2012,
	Bdsk-Url-1 = {http://dx.doi.org/10.1029/2011RS004941}}

@article{Mauch:2003,
	Author = {Mauch, T. and Murphy, T. and Buttery, H. J. and Curran, J. and Hunstead, R. W. and Piestrzynski, B. and Robertson, J. G. and Sadler, E. M.},
	Date-Added = {2016-06-30 16:23:26 +0000},
	Date-Modified = {2016-06-30 16:23:31 +0000},
	Doi = {10.1046/j.1365-8711.2003.06605.x},
	File = {:home/jline/.local/share/data/Mendeley Ltd./Mendeley Desktop/Downloaded/Mauch et al. - 2003 - SUMSS a wide-field radio imaging survey of the southern sky - II. The source catalogue.pdf:pdf},
	Issn = {0035-8711},
	Journal = {Monthly Notices of the Royal Astronomical Society},
	Month = {jul},
	Number = {4},
	Pages = {1117--1130},
	Title = {{SUMSS: a wide-field radio imaging survey of the southern sky - II. The source catalogue}},
	Url = {http://medcontent.metapress.com/index/A65RM03P4874243N.pdf http://mnras.oxfordjournals.org/cgi/doi/10.1046/j.1365-8711.2003.06605.x},
	Volume = {342},
	Year = {2003},
	Bdsk-Url-1 = {http://medcontent.metapress.com/index/A65RM03P4874243N.pdf%20http://mnras.oxfordjournals.org/cgi/doi/10.1046/j.1365-8711.2003.06605.x},
	Bdsk-Url-2 = {http://dx.doi.org/10.1046/j.1365-8711.2003.06605.x}}

@article{Budavari:2008,
	Author = {Budav{\'{a}}ri, Tam{\'{a}}s and Szalay, Alexander S.},
	Date-Added = {2016-06-30 16:19:05 +0000},
	Date-Modified = {2016-06-30 16:19:11 +0000},
	Doi = {10.1086/587156},
	File = {:home/jline/.local/share/data/Mendeley Ltd./Mendeley Desktop/Downloaded/Budav{\'{a}}ri, Szalay - 2008 - Probabilistic Cross{\^a}€Identification of Astronomical Sources.pdf:pdf},
	Issn = {0004-637X},
	Journal = {The Astrophysical Journal},
	Month = {may},
	Number = {1},
	Pages = {301--309},
	Title = {{Probabilistic Cross{\^a}€Identification of Astronomical Sources}},
	Url = {http://stacks.iop.org/0004-637X/679/i=1/a=301},
	Volume = {679},
	Year = {2008},
	Bdsk-Url-1 = {http://stacks.iop.org/0004-637X/679/i=1/a=301},
	Bdsk-Url-2 = {http://dx.doi.org/10.1086/587156}}

@article{Voytek:2014,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2014ApJ...782L...9V},
	Archiveprefix = {arXiv},
	Author = {{Voytek}, T.~C. and {Natarajan}, A. and {J{\'a}uregui Garc{\'{\i}}a}, J.~M. and {Peterson}, J.~B. and {L{\'o}pez-Cruz}, O.},
	Date-Added = {2016-06-29 19:49:04 +0000},
	Date-Modified = {2016-06-29 19:49:09 +0000},
	Doi = {10.1088/2041-8205/782/1/L9},
	Eid = {L9},
	Eprint = {1311.0014},
	Journal = {\apjl},
	Keywords = {cosmology: observations, dark ages, reionization, first stars, methods: observational, radio continuum: general},
	Month = feb,
	Pages = {L9},
	Title = {{Probing the Dark Ages at z \~{} 20: The SCI-HI 21 cm All-sky Spectrum Experiment}},
	Volume = 782,
	Year = 2014,
	Bdsk-Url-1 = {http://dx.doi.org/10.1088/2041-8205/782/1/L9}}

@article{Patra:2013,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2013ExA....36..319P},
	Archiveprefix = {arXiv},
	Author = {{Patra}, N. and {Subrahmanyan}, R. and {Raghunathan}, A. and {Udaya Shankar}, N.},
	Date-Added = {2016-06-29 19:48:10 +0000},
	Date-Modified = {2016-06-29 19:48:10 +0000},
	Doi = {10.1007/s10686-013-9336-3},
	Eprint = {1211.3800},
	Journal = {Experimental Astronomy},
	Keywords = {Astronomical instrumentation, Methods and techniques, Methods: observational, Cosmic background radiation, Cosmology: observations, Dark ages, Reionization, First stars, Radio continuum: ISM},
	Month = aug,
	Pages = {319-370},
	Primaryclass = {astro-ph.IM},
	Title = {{SARAS: a precision system for measurement of the cosmic radio background and signatures from the epoch of reionization}},
	Volume = 36,
	Year = 2013,
	Bdsk-Url-1 = {http://dx.doi.org/10.1007/s10686-013-9336-3}}

@article{Sokolowski:2015,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2015PASA...32....4S},
	Archiveprefix = {arXiv},
	Author = {{Sokolowski}, M. and {Tremblay}, S.~E. and {Wayth}, R.~B. and {Tingay}, S.~J. and {Clarke}, N. and {Roberts}, P. and {Waterson}, M. and {Ekers}, R.~D. and {Hall}, P. and {Lewis}, M. and {Mossammaparast}, M. and {Padhi}, S. and {Schlagenhaufer}, F. and {Sutinjo}, A. and {Tickner}, J.},
	Date-Added = {2016-06-29 19:46:08 +0000},
	Date-Modified = {2016-06-29 19:50:24 +0000},
	Doi = {10.1017/pasa.2015.3},
	Eid = {e004},
	Eprint = {1501.02922},
	Journal = {PASA - Publications of the Astronomical Society of Australia},
	Keywords = {cosmology: observations, dark ages, reionisation, first stars, instrumentation: miscellaneous, methods: data analysis, methods: observational},
	Month = feb,
	Pages = {e004},
	Primaryclass = {astro-ph.IM},
	Title = {{BIGHORNS - Broadband Instrument for Global HydrOgen ReioNisation Signal}},
	Volume = 32,
	Year = 2015,
	Bdsk-Url-1 = {http://dx.doi.org/10.1017/pasa.2015.3}}

@article{Asad:2016,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2016arXiv160404534A},
	Archiveprefix = {arXiv},
	Author = {{Asad}, K.~M.~B. and {Koopmans}, L.~V.~E. and {Jeli{\'c}}, V. and {Ghosh}, A. and {Brentjens}, M.~A. and {de Bruyn}, A.~G. and {Ciardi}, B. and {Iliev}, I.~T. and {Mevius}, M. and {Pandey}, V.~N. and {Yatawatta}, S. and {Zaroubi}, S.},
	Date-Added = {2016-06-29 14:31:10 +0000},
	Date-Modified = {2016-08-04 22:46:23 +0000},
	Eprint = {1604.04534},
	Journal = {{ArXiv e-prints, arXiv:1604.04534}},
	Keywords = {Astrophysics - Instrumentation and Methods for Astrophysics},
	Month = apr,
	Primaryclass = {astro-ph.IM},
	Title = {{Polarization leakage in epoch of reionization windows -- II. Primary beam model and direction dependent calibration}},
	Year = 2016}

@article{Trott:2016b,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2016PASA...33...19T},
	Archiveprefix = {arXiv},
	Author = {{Trott}, C.~M. and {Wayth}, R.~B.},
	Date-Added = {2016-06-28 23:36:06 +0000},
	Date-Modified = {2016-06-28 23:39:47 +0000},
	Doi = {10.1017/pasa.2016.18},
	Eid = {e019},
	Eprint = {1604.03273},
	Journal = {PASA - Publications of the Astronomical Society of Australia},
	Keywords = {(cosmology:) dark ages, reionization, first stars, techniques: interferometric, instrumentation: interferometers},
	Month = may,
	Pages = {e019},
	Primaryclass = {astro-ph.IM},
	Title = {{Spectral Calibration Requirements of Radio Interferometers for Epoch of Reionisation Science with the SKA}},
	Volume = 33,
	Year = 2016,
	Bdsk-Url-1 = {http://dx.doi.org/10.1017/pasa.2016.18}}

@article{Patil:2016,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2016arXiv160507619P},
	Archiveprefix = {arXiv},
	Author = {{Patil}, A.~H. and {Yatawatta}, S. and {Zaroubi}, S. and {Koopmans}, L.~V.~E. and {de Bruyn}, A.~G. and {Jeli{\'c}}, V. and {Ciardi}, B. and {Iliev}, I.~T. and {Mevius}, M. and {Pandey}, V.~N. and {Gehlot}, B.~K.},
	Date-Added = {2016-06-28 20:39:20 +0000},
	Date-Modified = {2016-08-04 22:48:43 +0000},
	Eprint = {1605.07619},
	Journal = {{ArXiv e-prints, arXiv:1605.07619}},
	Keywords = {Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics},
	Month = may,
	Primaryclass = {astro-ph.IM},
	Title = {{Systematic biases in low frequency radio interferometric data due to calibration: the LOFAR EoR case}},
	Year = 2016}

@article{vanHaarlem:2013,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2013A%26A...556A...2V},
	Archiveprefix = {arXiv},
	Author = {{van Haarlem}, M.~P. and {Wise}, M.~W. and {Gunst}, A.~W. and {Heald}, G. and {McKean}, J.~P. and {Hessels}, J.~W.~T. and {de Bruyn}, A.~G. and {Nijboer}, R. and {Swinbank}, J. and {Fallows}, R. and {Brentjens}, M. and {Nelles}, A. and {Beck}, R. and {Falcke}, H. and {Fender}, R. and {H{\"o}randel}, J. and {Koopmans}, L.~V.~E. and {Mann}, G. and {Miley}, G. and {R{\"o}ttgering}, H. and {Stappers}, B.~W. and {Wijers}, R.~A.~M.~J. and {Zaroubi}, S. and {van den Akker}, M. and {Alexov}, A. and {Anderson}, J. and {Anderson}, K. and {van Ardenne}, A. and {Arts}, M. and {Asgekar}, A. and {Avruch}, I.~M. and {Batejat}, F. and {B{\"a}hren}, L. and {Bell}, M.~E. and {Bell}, M.~R. and {van Bemmel}, I. and {Bennema}, P. and {Bentum}, M.~J. and {Bernardi}, G. and {Best}, P. and {B{\^\i}rzan}, L. and {Bonafede}, A. and {Boonstra}, A.-J. and {Braun}, R. and {Bregman}, J. and {Breitling}, F. and {van de Brink}, R.~H. and {Broderick}, J. and {Broekema}, P.~C. and {Brouw}, W.~N. and {Br{\"u}ggen}, M. and {Butcher}, H.~R. and {van Cappellen}, W. and {Ciardi}, B. and {Coenen}, T. and {Conway}, J. and {Coolen}, A. and {Corstanje}, A. and {Damstra}, S. and {Davies}, O. and {Deller}, A.~T. and {Dettmar}, R.-J. and {van Diepen}, G. and {Dijkstra}, K. and {Donker}, P. and {Doorduin}, A. and {Dromer}, J. and {Drost}, M. and {van Duin}, A. and {Eisl{\"o}ffel}, J. and {van Enst}, J. and {Ferrari}, C. and {Frieswijk}, W. and {Gankema}, H. and {Garrett}, M.~A. and {de Gasperin}, F. and {Gerbers}, M. and {de Geus}, E. and {Grie{\ss}meier}, J.-M. and {Grit}, T. and {Gruppen}, P. and {Hamaker}, J.~P. and {Hassall}, T. and {Hoeft}, M. and {Holties}, H.~A. and {Horneffer}, A. and {van der Horst}, A. and {van Houwelingen}, A. and {Huijgen}, A. and {Iacobelli}, M. and {Intema}, H. and {Jackson}, N. and {Jelic}, V. and {de Jong}, A. and {Juette}, E. and {Kant}, D. and {Karastergiou}, A. and {Koers}, A. and {Kollen}, H. and {Kondratiev}, V.~I. and {Kooistra}, E. and {Koopman}, Y. and {Koster}, A. and {Kuniyoshi}, M. and {Kramer}, M. and {Kuper}, G. and {Lambropoulos}, P. and {Law}, C. and {van Leeuwen}, J. and {Lemaitre}, J. and {Loose}, M. and {Maat}, P. and {Macario}, G. and {Markoff}, S. and {Masters}, J. and {McFadden}, R.~A. and {McKay-Bukowski}, D. and {Meijering}, H. and {Meulman}, H. and {Mevius}, M. and {Middelberg}, E. and {Millenaar}, R. and {Miller-Jones}, J.~C.~A. and {Mohan}, R.~N. and {Mol}, J.~D. and {Morawietz}, J. and {Morganti}, R. and {Mulcahy}, D.~D. and {Mulder}, E. and {Munk}, H. and {Nieuwenhuis}, L. and {van Nieuwpoort}, R. and {Noordam}, J.~E. and {Norden}, M. and {Noutsos}, A. and {Offringa}, A.~R. and {Olofsson}, H. and {Omar}, A. and {Orr{\'u}}, E. and {Overeem}, R. and {Paas}, H. and {Pandey-Pommier}, M. and {Pandey}, V.~N. and {Pizzo}, R. and {Polatidis}, A. and {Rafferty}, D. and {Rawlings}, S. and {Reich}, W. and {de Reijer}, J.-P. and {Reitsma}, J. and {Renting}, G.~A. and {Riemers}, P. and {Rol}, E. and {Romein}, J.~W. and {Roosjen}, J. and {Ruiter}, M. and {Scaife}, A. and {van der Schaaf}, K. and {Scheers}, B. and {Schellart}, P. and {Schoenmakers}, A. and {Schoonderbeek}, G. and {Serylak}, M. and {Shulevski}, A. and {Sluman}, J. and {Smirnov}, O. and {Sobey}, C. and {Spreeuw}, H. and {Steinmetz}, M. and {Sterks}, C.~G.~M. and {Stiepel}, H.-J. and {Stuurwold}, K. and {Tagger}, M. and {Tang}, Y. and {Tasse}, C. and {Thomas}, I. and {Thoudam}, S. and {Toribio}, M.~C. and {van der Tol}, B. and {Usov}, O. and {van Veelen}, M. and {van der Veen}, A.-J. and {ter Veen}, S. and {Verbiest}, J.~P.~W. and {Vermeulen}, R. and {Vermaas}, N. and {Vocks}, C. and {Vogt}, C. and {de Vos}, M. and {van der Wal}, E. and {van Weeren}, R. and {Weggemans}, H. and {Weltevrede}, P. and {White}, S. and {Wijnholds}, S.~J. and {Wilhelmsson}, T. and {Wucknitz}, O. and {Yatawatta}, S. and {Zarka}, P. and {Zensus}, A. and {van Zwieten}, J.},
	Date-Added = {2016-06-27 21:57:42 +0000},
	Date-Modified = {2016-06-27 21:57:42 +0000},
	Doi = {10.1051/0004-6361/201220873},
	Eid = {A2},
	Eprint = {1305.3550},
	Journal = {\aap},
	Keywords = {instrumentation: interferometers, radio continuum: general, radio lines: general, dark ages, reionization, first stars, telescopes},
	Month = aug,
	Pages = {A2},
	Primaryclass = {astro-ph.IM},
	Title = {{LOFAR: The LOw-Frequency ARray}},
	Volume = 556,
	Year = 2013,
	Bdsk-Url-1 = {http://dx.doi.org/10.1051/0004-6361/201220873}}

@inproceedings{Zaroubi:2013,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2013ASSL..396...45Z},
	Archiveprefix = {arXiv},
	Author = {{Zaroubi}, S.},
	Booktitle = {The First Galaxies},
	Date-Added = {2016-06-27 21:52:37 +0000},
	Date-Modified = {2016-06-27 21:52:43 +0000},
	Doi = {10.1007/978-3-642-32362-1_2},
	Editor = {{Wiklind}, T. and {Mobasher}, B. and {Bromm}, V.},
	Eprint = {1206.0267},
	Keywords = {Physics},
	Pages = {45},
	Series = {Astrophysics and Space Science Library},
	Title = {{The Epoch of Reionization}},
	Volume = 396,
	Year = 2013,
	Bdsk-Url-1 = {http://dx.doi.org/10.1007/978-3-642-32362-1_2}}

@article{Pritchard:2012,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2012RPPh...75h6901P},
	Archiveprefix = {arXiv},
	Author = {{Pritchard}, J.~R. and {Loeb}, A.},
	Date-Added = {2016-06-27 21:49:40 +0000},
	Date-Modified = {2016-06-27 21:49:40 +0000},
	Doi = {10.1088/0034-4885/75/8/086901},
	Eid = {086901},
	Eprint = {1109.6012},
	Journal = {Reports on Progress in Physics},
	Month = aug,
	Number = 8,
	Pages = {086901},
	Primaryclass = {astro-ph.CO},
	Title = {{21 cm cosmology in the 21st century}},
	Volume = 75,
	Year = 2012,
	Bdsk-Url-1 = {http://dx.doi.org/10.1088/0034-4885/75/8/086901}}

@article{Vrbanec:2016,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2016MNRAS.457..666V},
	Archiveprefix = {arXiv},
	Author = {{Vrbanec}, D. and {Ciardi}, B. and {Jeli{\'c}}, V. and {Jensen}, H. and {Zaroubi}, S. and {Fernandez}, E.~R. and {Ghosh}, A. and {Iliev}, I.~T. and {Kakiichi}, K. and {Koopmans}, L.~V.~E. and {Mellema}, G.},
	Date-Added = {2016-06-27 21:41:18 +0000},
	Date-Modified = {2016-06-27 21:41:28 +0000},
	Doi = {10.1093/mnras/stv2993},
	Eprint = {1509.03464},
	Journal = {\mnras},
	Keywords = {galaxies: high-redshift, intergalactic medium, cosmology: observations},
	Month = mar,
	Pages = {666-675},
	Title = {{Predictions for the 21 cm-galaxy cross-power spectrum observable with LOFAR and Subaru}},
	Volume = 457,
	Year = 2016,
	Bdsk-Url-1 = {http://dx.doi.org/10.1093/mnras/stv2993}}

@article{Silva:2015,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2015ApJ...806..209S},
	Archiveprefix = {arXiv},
	Author = {{Silva}, M. and {Santos}, M.~G. and {Cooray}, A. and {Gong}, Y.},
	Date-Added = {2016-06-27 21:40:48 +0000},
	Date-Modified = {2016-06-27 21:40:53 +0000},
	Doi = {10.1088/0004-637X/806/2/209},
	Eid = {209},
	Eprint = {1410.4808},
	Journal = {\apj},
	Keywords = {galaxies: high-redshift, galaxies: ISM, galaxies: luminosity function, mass function, large-scale structure of universe, quasars: emission lines},
	Month = jun,
	Pages = {209},
	Title = {{Prospects for Detecting C II Emission during the Epoch of Reionization}},
	Volume = 806,
	Year = 2015,
	Bdsk-Url-1 = {http://dx.doi.org/10.1088/0004-637X/806/2/209}}

@article{Dore:2014,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2014arXiv1412.4872D},
	Archiveprefix = {arXiv},
	Author = {{Dor{\'e}}, O. and {Bock}, J. and {31 co-authors}},
	Date-Added = {2016-06-27 21:40:06 +0000},
	Date-Modified = {2016-08-04 22:47:14 +0000},
	Eprint = {1412.4872},
	Journal = {{ArXiv e-prints, arXiv:1412.4872}},
	Keywords = {Astrophysics - Cosmology and Nongalactic Astrophysics},
	Month = dec,
	Title = {{Cosmology with the SPHEREX All-Sky Spectral Survey}},
	Year = 2014}

@article{DeBoer:2016,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2016arXiv160607473D},
	Archiveprefix = {arXiv},
	Author = {{DeBoer}, D.~R. and {Parsons}, A.~R. and {Aguirre}, J.~E. and {Alexander}, P. and {Ali}, Z.~S. and {Beardsley}, A.~P. and {Bernardi}, G. and {Bowman}, J.~D. and {Bradley}, R.~F. and {Carilli}, C.~L. and {Cheng}, C. and {de Lera Acedo}, E. and {Dillon}, J.~S. and {Ewall-Wice}, A. and {Fadana}, G. and {Fagnoni}, N. and {Fritz}, R. and {Furlanetto}, S.~R. and {Glendenning}, B. and {Greig}, B. and {Grobbelaar}, J. and {Hazelton}, B.~J. and {Hewitt}, J.~N. and {Hickish}, J. and {Jacobs}, D.~C. and {Julius}, A. and {Kariseb}, M. and {Kohn}, S.~A. and {Lekalake}, T. and {Liu}, A. and {Loots}, A. and {MacMahon}, D. and {Malan}, L. and {Malgas}, C. and {Maree}, M. and {Mathison}, N. and {Matsetela}, E. and {Mesinger}, A. and {Morales}, M.~F. and {Neben}, A.~R. and {Patra}, N. and {Pieterse}, S. and {Pober}, J.~C. and {Razavi-Ghods}, N. and {Ringuette}, J. and {Robnett}, J. and {Rosie}, K. and {Sell}, R. and {Smith}, C. and {Syce}, A. and {Tegmark}, M. and {Thyagarajan}, N. and {Williams}, P.~K.~G. and {Zheng}, H.},
	Date-Added = {2016-06-27 21:35:50 +0000},
	Date-Modified = {2016-06-27 21:35:50 +0000},
	Eprint = {1606.07473},
	Journal = {{ArXiv e-prints, arXiv:1606.07473}},
	Keywords = {Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics},
	Month = jun,
	Primaryclass = {astro-ph.IM},
	Title = {{Hydrogen Epoch of Reionization Array (HERA)}},
	Year = 2016}

@article{Planck:2016,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2016arXiv160503507P},
	Archiveprefix = {arXiv},
	Author = {{Planck Collaboration} and {Adam}, R. and {Aghanim}, N. and {Ashdown}, M. and {Aumont}, J. and {Baccigalupi}, C. and {Ballardini}, M. and {Banday}, A.~J. and {Barreiro}, R.~B. and {Bartolo}, N. and {Basak}, S. and {Battye}, R. and {Benabed}, K. and {Bernard}, J.-P. and {Bersanelli}, M. and {Bielewicz}, P. and {Bock}, J.~J. and {Bonaldi}, A. and {Bonavera}, L. and {Bond}, J.~R. and {Borrill}, J. and {Bouchet}, F.~R. and {Bucher}, M. and {Burigana}, C. and {Calabrese}, E. and {Cardoso}, J.-F. and {Carron}, J. and {Chiang}, H.~C. and {Colombo}, L.~P.~L. and {Combet}, C. and {Comis}, B. and {Coulais}, A. and {Crill}, B.~P. and {Curto}, A. and {Cuttaia}, F. and {Davis}, R.~J. and {de Bernardis}, P. and {de Rosa}, A. and {de Zotti}, G. and {Delabrouille}, J. and {Di Valentino}, E. and {Dickinson}, C. and {Diego}, J.~M. and {Dor{\'e}}, O. and {Douspis}, M. and {Ducout}, A. and {Dupac}, X. and {Elsner}, F. and {En{\ss}lin}, T.~A. and {Eriksen}, H.~K. and {Falgarone}, E. and {Fantaye}, Y. and {Finelli}, F. and {Forastieri}, F. and {Frailis}, M. and {Fraisse}, A.~A. and {Franceschi}, E. and {Frolov}, A. and {Galeotta}, S. and {Galli}, S. and {Ganga}, K. and {G{\'e}nova-Santos}, R.~T. and {Gerbino}, M. and {Ghosh}, T. and {Gonz{\'a}lez-Nuevo}, J. and {G{\'o}rski}, K.~M. and {Gruppuso}, A. and {Gudmundsson}, J.~E. and {Hansen}, F.~K. and {Helou}, G. and {Henrot-Versill{\'e}}, S. and {Herranz}, D. and {Hivon}, E. and {Huang}, Z. and {Ili}, S. and {Jaffe}, A.~H. and {Jones}, W.~C. and {Keih{\"a}nen}, E. and {Keskitalo}, R. and {Kisner}, T.~S. and {Knox}, L. and {Krachmalnicoff}, N. and {Kunz}, M. and {Kurki-Suonio}, H. and {Lagache}, G. and {L{\"a}hteenm{\"a}ki}, A. and {Lamarre}, J.-M. and {Langer}, M. and {Lasenby}, A. and {Lattanzi}, M. and {Lawrence}, C.~R. and {Le Jeune}, M. and {Levrier}, F. and {Lewis}, A. and {Liguori}, M. and {Lilje}, P.~B. and {L{\'o}pez-Caniego}, M. and {Ma}, Y.-Z. and {Mac{\'{\i}}as-P{\'e}rez}, J.~F. and {Maggio}, G. and {Mangilli}, A. and {Maris}, M. and {Martin}, P.~G. and {Mart{\'{\i}}nez-Gonz{\'a}lez}, E. and {Matarrese}, S. and {Mauri}, N. and {McEwen}, J.~D. and {Meinhold}, P.~R. and {Melchiorri}, A. and {Mennella}, A. and {Migliaccio}, M. and {Miville-Desch{\^e}nes}, M.-A. and {Molinari}, D. and {Moneti}, A. and {Montier}, L. and {Morgante}, G. and {Moss}, A. and {Naselsky}, P. and {Natoli}, P. and {Oxborrow}, C.~A. and {Pagano}, L. and {Paoletti}, D. and {Partridge}, B. and {Patanchon}, G. and {Patrizii}, L. and {Perdereau}, O. and {Perotto}, L. and {Pettorino}, V. and {Piacentini}, F. and {Plaszczynski}, S. and {Polastri}, L. and {Polenta}, G. and {Puget}, J.-L. and {Rachen}, J.~P. and {Racine}, B. and {Reinecke}, M. and {Remazeilles}, M. and {Renzi}, A. and {Rocha}, G. and {Rossetti}, M. and {Roudier}, G. and {Rubi{\~n}o-Mart{\'{\i}}n}, J.~A. and {Ruiz-Granados}, B. and {Salvati}, L. and {Sandri}, M. and {Savelainen}, M. and {Scott}, D. and {Sirri}, G. and {Sunyaev}, R. and {Suur-Uski}, A.-S. and {Tauber}, J.~A. and {Tenti}, M. and {Toffolatti}, L. and {Tomasi}, M. and {Tristram}, M. and {Trombetti}, T. and {Valiviita}, J. and {Van Tent}, F. and {Vielva}, P. and {Villa}, F. and {Vittorio}, N. and {Wandelt}, B.~D. and {Wehus}, I.~K. and {White}, M. and {Zacchei}, A. and {Zonca}, A.},
	Date-Added = {2016-06-10 18:42:27 +0000},
	Date-Modified = {2016-08-04 22:49:22 +0000},
	Eprint = {1605.03507},
	Journal = {{ArXiv e-prints, arXiv:1605.03507}},
	Keywords = {Astrophysics - Cosmology and Nongalactic Astrophysics},
	Month = may,
	Title = {{Planck intermediate results. XLVII. Planck constraints on reionization history}},
	Year = 2016}

@article{Trott:2016,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2016ApJ...818..139T},
	Archiveprefix = {arXiv},
	Author = {{Trott}, C.~M. and {Pindor}, B. and {Procopio}, P. and {Wayth}, R.~B. and {Mitchell}, D.~A. and {McKinley}, B. and {Tingay}, S.~J. and {Barry}, N. and {Beardsley}, A.~P. and {Bernardi}, G. and {Bowman}, J.~D. and {Briggs}, F. and {Cappallo}, R.~J. and {Carroll}, P. and {de Oliveira-Costa}, A. and {Dillon}, J.~S. and {Ewall-Wice}, A. and {Feng}, L. and {Greenhill}, L.~J. and {Hazelton}, B.~J. and {Hewitt}, J.~N. and {Hurley-Walker}, N. and {Johnston-Hollitt}, M. and {Jacobs}, D.~C. and {Kaplan}, D.~L. and {Kim}, H.~S. and {Lenc}, E. and {Line}, J. and {Loeb}, A. and {Lonsdale}, C.~J. and {Morales}, M.~F. and {Morgan}, E. and {Neben}, A.~R. and {Thyagarajan}, N. and {Oberoi}, D. and {Offringa}, A.~R. and {Ord}, S.~M. and {Paul}, S. and {Pober}, J.~C. and {Prabu}, T. and {Riding}, J. and {Udaya Shankar}, N. and {Sethi}, S.~K. and {Srivani}, K.~S. and {Subrahmanyan}, R. and {Sullivan}, I.~S. and {Tegmark}, M. and {Webster}, R.~L. and {Williams}, A. and {Williams}, C.~L. and {Wu}, C. and {Wyithe}, J.~S.~B.},
	Date-Added = {2016-06-02 16:13:28 +0000},
	Date-Modified = {2016-06-02 16:13:28 +0000},
	Doi = {10.3847/0004-637X/818/2/139},
	Eid = {139},
	Eprint = {1601.02073},
	Journal = {\apj},
	Keywords = {Astronomical instrumentation, methods and techniques, early universe, methods: statistical, techniques: interferometric},
	Month = feb,
	Pages = {139},
	Primaryclass = {astro-ph.IM},
	Title = {{CHIPS: The Cosmological H{\nbsp}i{\nbsp}Power Spectrum Estimator}},
	Volume = 818,
	Year = 2016,
	Bdsk-Url-1 = {http://dx.doi.org/10.3847/0004-637X/818/2/139}}

@article{Ewall-Wice:2016,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2016MNRAS.tmp..877E},
	Archiveprefix = {arXiv},
	Author = {{Ewall-Wice}, A. and {Dillon}, J.~S. and {Hewitt}, J.~N. and {Loeb}, A. and {Mesinger}, A. and {Neben}, A.~R. and {Offringa}, A.~R. and {Tegmark}, M. and {Barry}, N. and {Beardsley}, A.~P. and {Bernardi}, G. and {Bowman}, J.~D. and {Briggs}, F. and {Cappallo}, R.~J. and {Carroll}, P. and {Corey}, B.~E. and {de Oliveira-Costa}, A. and {Emrich}, D. and {Feng}, L. and {Gaensler}, B.~M. and {Goeke}, R. and {Greenhill}, L.~J. and {Hazelton}, B.~J. and {Hurley-Walker}, N. and {Johnston-Hollitt}, M. and {Jacobs}, D.~C. and {Kaplan}, D.~L. and {Kasper}, J.~C. and {Kim}, H. and {Kratzenberg}, E. and {Lenc}, E. and {Line}, J. and {Lonsdale}, C.~J. and {Lynch}, M.~J. and {McKinley}, B. and {McWhirter}, S.~R. and {Mitchell}, D.~A. and {Morales}, M.~F. and {Morgan}, E. and {Thyagarajan}, N. and {Oberoi}, D. and {Ord}, S.~M. and {Paul}, S. and {Pindor}, B. and {Pober}, J.~C. and {Prabu}, T. and {Procopio}, P. and {Riding}, J. and {Rogers}, A.~E.~E. and {Roshi}, A. and {Shankar}, N.~U. and {Sethi}, S.~K. and {Srivani}, K.~S. and {Subrahmanyan}, R. and {Sullivan}, I.~S. and {Tingay}, S.~J. and {Trott}, C.~M. and {Waterson}, M. and {Wayth}, R.~B. and {Webster}, R.~L. and {Whitney}, A.~R. and {Williams}, A. and {Williams}, C.~L. and {Wu}, C. and {Wyithe}, J.~S.~B.},
	Date-Added = {2016-06-02 16:07:12 +0000},
	Date-Modified = {2016-06-02 16:07:12 +0000},
	Doi = {10.1093/mnras/stw1022},
	Eprint = {1605.00016},
	Journal = {\mnras},
	Keywords = {dark ages, reionization, first stars, techniques: interferometric, radio lines: general, X-rays: galaxies},
	Month = may,
	Title = {{First Limits on the 21 cm Power Spectrum during the Epoch of X-ray heating.}},
	Year = 2016,
	Bdsk-Url-1 = {http://dx.doi.org/10.1093/mnras/stw1022}}

@article{Ord:2010,
	Abstract = {The Murchison Wide-Field Array (MWA) is a low-frequency radio telescope, currently under construction, intended to search for the spectral signature of the epoch of reionization (EOR) and to probe the structure of the solar corona. Sited in western Australia, the full MWA will comprise 8192 dipoles grouped into 512 tiles and will be capable of imaging the sky south of 40$\,^{\circ}$ declination, from 80 MHz to 300 MHz with an instantaneous field of view that is tens of degrees wide and a resolution of a few arcminutes. A 32 station prototype of the MWA has been recently commissioned and a set of observations has been taken that exercise the whole acquisition and processing pipeline. We presentStokes I , Q , and U images from two ~4 hr integrations of a field 20$\,^{\circ}$ wide centered on Pictoris A. These images demonstrate the capacity and stability of a real-time calibration and imaging technique employing the weighted addition of warped snapshots to counter extreme wide-field imaging distortions.},
	Author = {S. M. Ord and D. A. Mitchell and R. B. Wayth and L. J. Greenhill and G. Bernardi and S. Gleadow and R. G. Edgar and M. A. Clark and G. Allen and W. Arcus and L. Benkevitch and J. D. Bowman and F. H. Briggs and J. D. Bunton and S. Burns and R. J. Cappallo and W. A. Coles and B. E. Corey and L. deSouza and S. S. Doeleman and M. Derome and A. Deshpande and D. Emrich and R. Goeke and M. R. Gopalakrishna and D. Herne and J. N. Hewitt and P. A. Kamini and D. L. Kaplan and J. C. Kasper and B. B. Kincaid and J. Kocz and E. Kowald and E. Kratzenberg and D. Kumar and C. J. Lonsdale and M. J. Lynch and S. R. McWhirter and S. Madhavi and M. Matejek and M. F. Morales and E. Morgan and D. Oberoi and J. Pathikulangara and T. Prabu and A. E. E. Rogers and A. Roshi and J. E. Salah and A. Schinkel and N. Udaya Shankar and K. S. Srivani and J. Stevens and S. J. Tingay and A. Vaccarella and M. Waterson and R. L. Webster and A. R. Whitney and A. Williams and C. Williams},
	Date-Added = {2016-05-04 18:09:04 +0000},
	Date-Modified = {2016-05-04 18:09:09 +0000},
	Journal = {Publications of the Astronomical Society of the Pacific},
	Number = {897},
	Pages = {1353},
	Title = {Interferometric Imaging with the 32 Element Murchison Wide-Field Array},
	Url = {http://stacks.iop.org/1538-3873/122/i=897/a=1353},
	Volume = {122},
	Year = {2010},
	Bdsk-Url-1 = {http://stacks.iop.org/1538-3873/122/i=897/a=1353}}

@article{McGreer:2015,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2015MNRAS.447..499M},
	Archiveprefix = {arXiv},
	Author = {{McGreer}, I.~D. and {Mesinger}, A. and {D'Odorico}, V.},
	Date-Added = {2016-03-17 21:13:24 +0000},
	Date-Modified = {2016-03-17 21:13:31 +0000},
	Doi = {10.1093/mnras/stu2449},
	Eprint = {1411.5375},
	Journal = {\mnras},
	Keywords = {galaxies: high-redshift, quasars: absorption lines, cosmology: observations, dark ages, reionization, first stars, diffuse radiation, early Universe},
	Month = feb,
	Pages = {499-505},
	Title = {{Model-independent evidence in favour of an end to reionization by z {\ap} 6}},
	Volume = 447,
	Year = 2015,
	Bdsk-Url-1 = {http://dx.doi.org/10.1093/mnras/stu2449}}

@article{Wayth:2015,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2015PASA...32...25W},
	Archiveprefix = {arXiv},
	Author = {{Wayth}, R.~B. and {Lenc}, E. and {Bell}, M.~E. and {Callingham}, J.~R. and {Dwarakanath}, K.~S. and {Franzen}, T.~M.~O. and {For}, B.-Q. and {Gaensler}, B. and {Hancock}, P. and {Hindson}, L. and {Hurley-Walker}, N. and {Jackson}, C.~A. and {Johnston-Hollitt}, M. and {Kapi{\'n}ska}, A.~D. and {McKinley}, B. and {Morgan}, J. and {Offringa}, A.~R. and {Procopio}, P. and {Staveley-Smith}, L. and {Wu}, C. and {Zheng}, Q. and {Trott}, C.~M. and {Bernardi}, G. and {Bowman}, J.~D. and {Briggs}, F. and {Cappallo}, R.~J. and {Corey}, B.~E. and {Deshpande}, A.~A. and {Emrich}, D. and {Goeke}, R. and {Greenhill}, L.~J. and {Hazelton}, B.~J. and {Kaplan}, D.~L. and {Kasper}, J.~C. and {Kratzenberg}, E. and {Lonsdale}, C.~J. and {Lynch}, M.~J. and {McWhirter}, S.~R. and {Mitchell}, D.~A. and {Morales}, M.~F. and {Morgan}, E. and {Oberoi}, D. and {Ord}, S.~M. and {Prabu}, T. and {Rogers}, A.~E.~E. and {Roshi}, A. and {Shankar}, N.~U. and {Srivani}, K.~S. and {Subrahmanyan}, R. and {Tingay}, S.~J. and {Waterson}, M. and {Webster}, R.~L. and {Whitney}, A.~R. and {Williams}, A. and {Williams}, C.~L.},
	Date-Added = {2016-03-10 22:59:48 +0000},
	Date-Modified = {2016-03-10 23:00:19 +0000},
	Doi = {10.1017/pasa.2015.26},
	Eid = {e025},
	Eprint = {1505.06041},
	Journal = {PASA - Publications of the Astronomical Society of Australia},
	Keywords = {Galaxy: general, radio continuum: general, radio lines: general, surveys},
	Month = jun,
	Pages = {e025},
	Primaryclass = {astro-ph.IM},
	Title = {{GLEAM: The GaLactic and Extragalactic All-Sky MWA Survey}},
	Volume = 32,
	Year = 2015,
	Bdsk-Url-1 = {http://dx.doi.org/10.1017/pasa.2015.26}}

@article{Pober:2016,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2016ApJ...819....8P},
	Archiveprefix = {arXiv},
	Author = {{Pober}, J.~C. and {Hazelton}, B.~J. and {Beardsley}, A.~P. and {Barry}, N.~A. and {Martinot}, Z.~E. and {Sullivan}, I.~S. and {Morales}, M.~F. and {Bell}, M.~E. and {Bernardi}, G. and {Bhat}, N.~D.~R. and {Bowman}, J.~D. and {Briggs}, F. and {Cappallo}, R.~J. and {Carroll}, P. and {Corey}, B.~E. and {de Oliveira-Costa}, A. and {Deshpande}, A.~A. and {Dillon}, J.~S. and {Emrich}, D. and {Ewall-Wice}, A.~M. and {Feng}, L. and {Goeke}, R. and {Greenhill}, L.~J. and {Hewitt}, J.~N. and {Hindson}, L. and {Hurley-Walker}, N. and {Jacobs}, D.~C. and {Johnston-Hollitt}, M. and {Kaplan}, D.~L. and {Kasper}, J.~C. and {Kim}, H.-S. and {Kittiwisit}, P. and {Kratzenberg}, E. and {Kudryavtseva}, N. and {Lenc}, E. and {Line}, J. and {Loeb}, A. and {Lonsdale}, C.~J. and {Lynch}, M.~J. and {McKinley}, B. and {McWhirter}, S.~R. and {Mitchell}, D.~A. and {Morgan}, E. and {Neben}, A.~R. and {Oberoi}, D. and {Offringa}, A.~R. and {Ord}, S.~M. and {Paul}, S. and {Pindor}, B. and {Prabu}, T. and {Procopio}, P. and {Riding}, J. and {Rogers}, A.~E.~E. and {Roshi}, A. and {Sethi}, S.~K. and {Udaya Shankar}, N. and {Srivani}, K.~S. and {Subrahmanyan}, R. and {Tegmark}, M. and {Thyagarajan}, N. and {Tingay}, S.~J. and {Trott}, C.~M. and {Waterson}, M. and {Wayth}, R.~B. and {Webster}, R.~L. and {Whitney}, A.~R. and {Williams}, A. and {Williams}, C.~L. and {Wyithe}, J.~S.~B.},
	Date-Added = {2016-03-08 21:07:50 +0000},
	Date-Modified = {2016-03-08 21:07:57 +0000},
	Doi = {10.3847/0004-637X/819/1/8},
	Eid = {8},
	Eprint = {1601.06177},
	Journal = {\apj},
	Keywords = {cosmology: observations, dark ages, reionization, first stars, techniques: interferometric},
	Month = mar,
	Pages = {8},
	Primaryclass = {astro-ph.IM},
	Title = {{The Importance of Wide-field Foreground Removal for 21 cm Cosmology: A Demonstration with Early MWA Epoch of Reionization Observations}},
	Volume = 819,
	Year = 2016,
	Bdsk-Url-1 = {http://dx.doi.org/10.3847/0004-637X/819/1/8}}

@article{Lorimer:2007,
	Abstract = {Pulsar surveys offer a rare opportunity to monitor the radio sky for impulsive burst-like events with millisecond durations. We analyzed archival survey data and found a 30-jansky dispersed burst, less than 5 milliseconds in duration, located 3{\textdegree} from the Small Magellanic Cloud. The burst properties argue against a physical association with our Galaxy or the Small Magellanic Cloud. Current models for the free electron content in the universe imply that the burst is less than 1 gigaparsec distant. No further bursts were seen in 90 hours of additional observations, which implies that it was a singular event such as a supernova or coalescence of relativistic objects. Hundreds of similar events could occur every day and, if detected, could serve as cosmological probes.},
	Author = {Lorimer, D. R. and Bailes, M. and McLaughlin, M. A. and Narkevic, D. J. and Crawford, F.},
	Date-Added = {2016-02-29 16:30:30 +0000},
	Date-Modified = {2016-02-29 16:30:37 +0000},
	Doi = {10.1126/science.1147532},
	Eprint = {http://science.sciencemag.org/content/318/5851/777.full.pdf},
	Issn = {0036-8075},
	Journal = {Science},
	Number = {5851},
	Pages = {777--780},
	Publisher = {American Association for the Advancement of Science},
	Title = {A Bright Millisecond Radio Burst of Extragalactic Origin},
	Url = {http://science.sciencemag.org/content/318/5851/777},
	Volume = {318},
	Year = {2007},
	Bdsk-Url-1 = {http://science.sciencemag.org/content/318/5851/777},
	Bdsk-Url-2 = {http://dx.doi.org/10.1126/science.1147532}}

@article{Abbot:2016a,
	Author = {Abbott, B. P. and Abbott, R. and Abbott, T. D. and Abernathy, M. R. and Acernese, F. and Ackley, K. and Adams, C. and Adams, T. and Addesso, P. and Adhikari, R. X. and Adya, V. B. and Affeldt, C. and Agathos, M. and Agatsuma, K. and Aggarwal, N. and Aguiar, O. D. and Aiello, L. and Ain, A. and Ajith, P. and Allen, B. and Allocca, A. and Altin, P. A. and Anderson, S. B. and Anderson, W. G. and Arai, K. and Arain, M. A. and Araya, M. C. and Arceneaux, C. C. and Areeda, J. S. and Arnaud, N. and Arun, K. G. and Ascenzi, S. and Ashton, G. and Ast, M. and Aston, S. M. and Astone, P. and Aufmuth, P. and Aulbert, C. and Babak, S. and Bacon, P. and Bader, M. K. M. and Baker, P. T. and Baldaccini, F. and Ballardin, G. and Ballmer, S. W. and Barayoga, J. C. and Barclay, S. E. and Barish, B. C. and Barker, D. and Barone, F. and Barr, B. and Barsotti, L. and Barsuglia, M. and Barta, D. and Bartlett, J. and Barton, M. A. and Bartos, I. and Bassiri, R. and Basti, A. and Batch, J. C. and Baune, C. and Bavigadda, V. and Bazzan, M. and Behnke, B. and Bejger, M. and Belczynski, C. and Bell, A. S. and Bell, C. J. and Berger, B. K. and Bergman, J. and Bergmann, G. and Berry, C. P. L. and Bersanetti, D. and Bertolini, A. and Betzwieser, J. and Bhagwat, S. and Bhandare, R. and Bilenko, I. A. and Billingsley, G. and Birch, J. and Birney, R. and Birnholtz, O. and Biscans, S. and Bisht, A. and Bitossi, M. and Biwer, C. and Bizouard, M. A. and Blackburn, J. K. and Blair, C. D. and Blair, D. G. and Blair, R. M. and Bloemen, S. and Bock, O. and Bodiya, T. P. and Boer, M. and Bogaert, G. and Bogan, C. and Bohe, A. and Bojtos, P. and Bond, C. and Bondu, F. and Bonnand, R. and Boom, B. A. and Bork, R. and Boschi, V. and Bose, S. and Bouffanais, Y. and Bozzi, A. and Bradaschia, C. and Brady, P. R. and Braginsky, V. B. and Branchesi, M. and Brau, J. E. and Briant, T. and Brillet, A. and Brinkmann, M. and Brisson, V. and Brockill, P. and Brooks, A. F. and Brown, D. A. and Brown, D. D. and Brown, N. M. and Buchanan, C. C. and Buikema, A. and Bulik, T. and Bulten, H. J. and Buonanno, A. and Buskulic, D. and Buy, C. and Byer, R. L. and Cabero, M. and Cadonati, L. and Cagnoli, G. and Cahillane, C. and Bustillo, J. Calder\'on and Callister, T. and Calloni, E. and Camp, J. B. and Cannon, K. C. and Cao, J. and Capano, C. D. and Capocasa, E. and Carbognani, F. and Caride, S. and Diaz, J. Casanueva and Casentini, C. and Caudill, S. and Cavagli\`a, M. and Cavalier, F. and Cavalieri, R. and Cella, G. and Cepeda, C. B. and Baiardi, L. Cerboni and Cerretani, G. and Cesarini, E. and Chakraborty, R. and Chalermsongsak, T. and Chamberlin, S. J. and Chan, M. and Chao, S. and Charlton, P. and Chassande-Mottin, E. and Chen, H. Y. and Chen, Y. and Cheng, C. and Chincarini, A. and Chiummo, A. and Cho, H. S. and Cho, M. and Chow, J. H. and Christensen, N. and Chu, Q. and Chua, S. and Chung, S. and Ciani, G. and Clara, F. and Clark, J. A. and Cleva, F. and Coccia, E. and Cohadon, P.-F. and Colla, A. and Collette, C. G. and Cominsky, L. and Constancio, M. and Conte, A. and Conti, L. and Cook, D. and Corbitt, T. R. and Cornish, N. and Corsi, A. and Cortese, S. and Costa, C. A. and Coughlin, M. W. and Coughlin, S. B. and Coulon, J.-P. and Countryman, S. T. and Couvares, P. and Cowan, E. E. and Coward, D. M. and Cowart, M. J. and Coyne, D. C. and Coyne, R. and Craig, K. and Creighton, J. D. E. and Creighton, T. D. and Cripe, J. and Crowder, S. G. and Cruise, A. M. and Cumming, A. and Cunningham, L. and Cuoco, E. and Canton, T. Dal and Danilishin, S. L. and D'Antonio, S. and Danzmann, K. and Darman, N. S. and Da Silva Costa, C. F. and Dattilo, V. and Dave, I. and Daveloza, H. P. and Davier, M. and Davies, G. S. and Daw, E. J. and Day, R. and De, S. and DeBra, D. and Debreczeni, G. and Degallaix, J. and De Laurentis, M. and Del\'eglise, S. and Del Pozzo, W. and Denker, T. and Dent, T. and Dereli, H. and Dergachev, V. and DeRosa, R. T. and De Rosa, R. and DeSalvo, R. and Dhurandhar, S. and D\'{\i}az, M. C. and Di Fiore, L. and Di Giovanni, M. and Di Lieto, A. and Di Pace, S. and Di Palma, I. and Di Virgilio, A. and Dojcinoski, G. and Dolique, V. and Donovan, F. and Dooley, K. L. and Doravari, S. and Douglas, R. and Downes, T. P. and Drago, M. and Drever, R. W. P. and Driggers, J. C. and Du, Z. and Ducrot, M. and Dwyer, S. E. and Edo, T. B. and Edwards, M. C. and Effler, A. and Eggenstein, H.-B. and Ehrens, P. and Eichholz, J. and Eikenberry, S. S. and Engels, W. and Essick, R. C. and Etzel, T. and Evans, M. and Evans, T. M. and Everett, R. and Factourovich, M. and Fafone, V. and Fair, H. and Fairhurst, S. and Fan, X. and Fang, Q. and Farinon, S. and Farr, B. and Farr, W. M. and Favata, M. and Fays, M. and Fehrmann, H. and Fejer, M. M. and Feldbaum, D. and Ferrante, I. and Ferreira, E. C. and Ferrini, F. and Fidecaro, F. and Finn, L. S. and Fiori, I. and Fiorucci, D. and Fisher, R. P. and Flaminio, R. and Fletcher, M. and Fong, H. and Fournier, J.-D. and Franco, S. and Frasca, S. and Frasconi, F. and Frede, M. and Frei, Z. and Freise, A. and Frey, R. and Frey, V. and Fricke, T. T. and Fritschel, P. and Frolov, V. V. and Fulda, P. and Fyffe, M. and Gabbard, H. A. G. and Gair, J. R. and Gammaitoni, L. and Gaonkar, S. G. and Garufi, F. and Gatto, A. and Gaur, G. and Gehrels, N. and Gemme, G. and Gendre, B. and Genin, E. and Gennai, A. and George, J. and Gergely, L. and Germain, V. and Ghosh, Abhirup and Ghosh, Archisman and Ghosh, S. and Giaime, J. A. and Giardina, K. D. and Giazotto, A. and Gill, K. and Glaefke, A. and Gleason, J. R. and Goetz, E. and Goetz, R. and Gondan, L. and Gonz\'alez, G. and Castro, J. M. Gonzalez and Gopakumar, A. and Gordon, N. A. and Gorodetsky, M. L. and Gossan, S. E. and Gosselin, M. and Gouaty, R. and Graef, C. and Graff, P. B. and Granata, M. and Grant, A. and Gras, S. and Gray, C. and Greco, G. and Green, A. C. and Greenhalgh, R. J. S. and Groot, P. and Grote, H. and Grunewald, S. and Guidi, G. M. and Guo, X. and Gupta, A. and Gupta, M. K. and Gushwa, K. E. and Gustafson, E. K. and Gustafson, R. and Hacker, J. J. and Hall, B. R. and Hall, E. D. and Hammond, G. and Haney, M. and Hanke, M. M. and Hanks, J. and Hanna, C. and Hannam, M. D. and Hanson, J. and Hardwick, T. and Harms, J. and Harry, G. M. and Harry, I. W. and Hart, M. J. and Hartman, M. T. and Haster, C.-J. and Haughian, K. and Healy, J. and Heefner, J. and Heidmann, A. and Heintze, M. C. and Heinzel, G. and Heitmann, H. and Hello, P. and Hemming, G. and Hendry, M. and Heng, I. S. and Hennig, J. and Heptonstall, A. W. and Heurs, M. and Hild, S. and Hoak, D. and Hodge, K. A. and Hofman, D. and Hollitt, S. E. and Holt, K. and Holz, D. E. and Hopkins, P. and Hosken, D. J. and Hough, J. and Houston, E. A. and Howell, E. J. and Hu, Y. M. and Huang, S. and Huerta, E. A. and Huet, D. and Hughey, B. and Husa, S. and Huttner, S. H. and Huynh-Dinh, T. and Idrisy, A. and Indik, N. and Ingram, D. R. and Inta, R. and Isa, H. N. and Isac, J.-M. and Isi, M. and Islas, G. and Isogai, T. and Iyer, B. R. and Izumi, K. and Jacobson, M. B. and Jacqmin, T. and Jang, H. and Jani, K. and Jaranowski, P. and Jawahar, S. and Jim\'enez-Forteza, F. and Johnson, W. W. and Johnson-McDaniel, N. K. and Jones, D. I. and Jones, R. and Jonker, R. J. G. and Ju, L. and Haris, K. and Kalaghatgi, C. V. and Kalogera, V. and Kandhasamy, S. and Kang, G. and Kanner, J. B. and Karki, S. and Kasprzack, M. and Katsavounidis, E. and Katzman, W. and Kaufer, S. and Kaur, T. and Kawabe, K. and Kawazoe, F. and K\'ef\'elian, F. and Kehl, M. S. and Keitel, D. and Kelley, D. B. and Kells, W. and Kennedy, R. and Keppel, D. G. and Key, J. S. and Khalaidovski, A. and Khalili, F. Y. and Khan, I. and Khan, S. and Khan, Z. and Khazanov, E. A. and Kijbunchoo, N. and Kim, C. and Kim, J. and Kim, K. and Kim, Nam-Gyu and Kim, Namjun and Kim, Y.-M. and King, E. J. and King, P. J. and Kinzel, D. L. and Kissel, J. S. and Kleybolte, L. and Klimenko, S. and Koehlenbeck, S. M. and Kokeyama, K. and Koley, S. and Kondrashov, V. and Kontos, A. and Koranda, S. and Korobko, M. and Korth, W. Z. and Kowalska, I. and Kozak, D. B. and Kringel, V. and Krishnan, B. and Kr\'olak, A. and Krueger, C. and Kuehn, G. and Kumar, P. and Kumar, R. and Kuo, L. and Kutynia, A. and Kwee, P. and Lackey, B. D. and Landry, M. and Lange, J. and Lantz, B. and Lasky, P. D. and Lazzarini, A. and Lazzaro, C. and Leaci, P. and Leavey, S. and Lebigot, E. O. and Lee, C. H. and Lee, H. K. and Lee, H. M. and Lee, K. and Lenon, A. and Leonardi, M. and Leong, J. R. and Leroy, N. and Letendre, N. and Levin, Y. and Levine, B. M. and Li, T. G. F. and Libson, A. and Littenberg, T. B. and Lockerbie, N. A. and Logue, J. and Lombardi, A. L. and London, L. T. and Lord, J. E. and Lorenzini, M. and Loriette, V. and Lormand, M. and Losurdo, G. and Lough, J. D. and Lousto, C. O. and Lovelace, G. and L\"uck, H. and Lundgren, A. P. and Luo, J. and Lynch, R. and Ma, Y. and MacDonald, T. and Machenschalk, B. and MacInnis, M. and Macleod, D. M. and Maga\~na-Sandoval, F. and Magee, R. M. and Mageswaran, M. and Majorana, E. and Maksimovic, I. and Malvezzi, V. and Man, N. and Mandel, I. and Mandic, V. and Mangano, V. and Mansell, G. L. and Manske, M. and Mantovani, M. and Marchesoni, F. and Marion, F. and M\'arka, S. and M\'arka, Z. and Markosyan, A. S. and Maros, E. and Martelli, F. and Martellini, L. and Martin, I. W. and Martin, R. M. and Martynov, D. V. and Marx, J. N. and Mason, K. and Masserot, A. and Massinger, T. J. and Masso-Reid, M. and Matichard, F. and Matone, L. and Mavalvala, N. and Mazumder, N. and Mazzolo, G. and McCarthy, R. and McClelland, D. E. and McCormick, S. and McGuire, S. C. and McIntyre, G. and McIver, J. and McManus, D. J. and McWilliams, S. T. and Meacher, D. and Meadors, G. D. and Meidam, J. and Melatos, A. and Mendell, G. and Mendoza-Gandara, D. and Mercer, R. A. and Merilh, E. and Merzougui, M. and Meshkov, S. and Messenger, C. and Messick, C. and Meyers, P. M. and Mezzani, F. and Miao, H. and Michel, C. and Middleton, H. and Mikhailov, E. E. and Milano, L. and Miller, J. and Millhouse, M. and Minenkov, Y. and Ming, J. and Mirshekari, S. and Mishra, C. and Mitra, S. and Mitrofanov, V. P. and Mitselmakher, G. and Mittleman, R. and Moggi, A. and Mohan, M. and Mohapatra, S. R. P. and Montani, M. and Moore, B. C. and Moore, C. J. and Moraru, D. and Moreno, G. and Morriss, S. R. and Mossavi, K. and Mours, B. and Mow-Lowry, C. M. and Mueller, C. L. and Mueller, G. and Muir, A. W. and Mukherjee, Arunava and Mukherjee, D. and Mukherjee, S. and Mukund, N. and Mullavey, A. and Munch, J. and Murphy, D. J. and Murray, P. G. and Mytidis, A. and Nardecchia, I. and Naticchioni, L. and Nayak, R. K. and Necula, V. and Nedkova, K. and Nelemans, G. and Neri, M. and Neunzert, A. and Newton, G. and Nguyen, T. T. and Nielsen, A. B. and Nissanke, S. and Nitz, A. and Nocera, F. and Nolting, D. and Normandin, M. E. N. and Nuttall, L. K. and Oberling, J. and Ochsner, E. and O'Dell, J. and Oelker, E. and Ogin, G. H. and Oh, J. J. and Oh, S. H. and Ohme, F. and Oliver, M. and Oppermann, P. and Oram, Richard J. and O'Reilly, B. and O'Shaughnessy, R. and Ott, C. D. and Ottaway, D. J. and Ottens, R. S. and Overmier, H. and Owen, B. J. and Pai, A. and Pai, S. A. and Palamos, J. R. and Palashov, O. and Palomba, C. and Pal-Singh, A. and Pan, H. and Pan, Y. and Pankow, C. and Pannarale, F. and Pant, B. C. and Paoletti, F. and Paoli, A. and Papa, M. A. and Paris, H. R. and Parker, W. and Pascucci, D. and Pasqualetti, A. and Passaquieti, R. and Passuello, D. and Patricelli, B. and Patrick, Z. and Pearlstone, B. L. and Pedraza, M. and Pedurand, R. and Pekowsky, L. and Pele, A. and Penn, S. and Perreca, A. and Pfeiffer, H. P. and Phelps, M. and Piccinni, O. and Pichot, M. and Pickenpack, M. and Piergiovanni, F. and Pierro, V. and Pillant, G. and Pinard, L. and Pinto, I. M. and Pitkin, M. and Poeld, J. H. and Poggiani, R. and Popolizio, P. and Post, A. and Powell, J. and Prasad, J. and Predoi, V. and Premachandra, S. S. and Prestegard, T. and Price, L. R. and Prijatelj, M. and Principe, M. and Privitera, S. and Prix, R. and Prodi, G. A. and Prokhorov, L. and Puncken, O. and Punturo, M. and Puppo, P. and P\"urrer, M. and Qi, H. and Qin, J. and Quetschke, V. and Quintero, E. A. and Quitzow-James, R. and Raab, F. J. and Rabeling, D. S. and Radkins, H. and Raffai, P. and Raja, S. and Rakhmanov, M. and Ramet, C. R. and Rapagnani, P. and Raymond, V. and Razzano, M. and Re, V. and Read, J. and Reed, C. M. and Regimbau, T. and Rei, L. and Reid, S. and Reitze, D. H. and Rew, H. and Reyes, S. D. and Ricci, F. and Riles, K. and Robertson, N. A. and Robie, R. and Robinet, F. and Rocchi, A. and Rolland, L. and Rollins, J. G. and Roma, V. J. and Romano, J. D. and Romano, R. and Romanov, G. and Romie, J. H. and Rosi\ifmmode \acute{n}\else \'{n}\fi{}ska, D. and Rowan, S. and R\"udiger, A. and Ruggi, P. and Ryan, K. and Sachdev, S. and Sadecki, T. and Sadeghian, L. and Salconi, L. and Saleem, M. and Salemi, F. and Samajdar, A. and Sammut, L. and Sampson, L. M. and Sanchez, E. J. and Sandberg, V. and Sandeen, B. and Sanders, G. H. and Sanders, J. R. and Sassolas, B. and Sathyaprakash, B. S. and Saulson, P. R. and Sauter, O. and Savage, R. L. and Sawadsky, A. and Schale, P. and Schilling, R. and Schmidt, J. and Schmidt, P. and Schnabel, R. and Schofield, R. M. S. and Sch\"onbeck, A. and Schreiber, E. and Schuette, D. and Schutz, B. F. and Scott, J. and Scott, S. M. and Sellers, D. and Sengupta, A. S. and Sentenac, D. and Sequino, V. and Sergeev, A. and Serna, G. and Setyawati, Y. and Sevigny, A. and Shaddock, D. A. and Shaffer, T. and Shah, S. and Shahriar, M. S. and Shaltev, M. and Shao, Z. and Shapiro, B. and Shawhan, P. and Sheperd, A. and Shoemaker, D. H. and Shoemaker, D. M. and Siellez, K. and Siemens, X. and Sigg, D. and Silva, A. D. and Simakov, D. and Singer, A. and Singer, L. P. and Singh, A. and Singh, R. and Singhal, A. and Sintes, A. M. and Slagmolen, B. J. J. and Smith, J. R. and Smith, M. R. and Smith, N. D. and Smith, R. J. E. and Son, E. J. and Sorazu, B. and Sorrentino, F. and Souradeep, T. and Srivastava, A. K. and Staley, A. and Steinke, M. and Steinlechner, J. and Steinlechner, S. and Steinmeyer, D. and Stephens, B. C. and Stevenson, S. P. and Stone, R. and Strain, K. A. and Straniero, N. and Stratta, G. and Strauss, N. A. and Strigin, S. and Sturani, R. and Stuver, A. L. and Summerscales, T. Z. and Sun, L. and Sutton, P. J. and Swinkels, B. L. and Szczepa\ifmmode \acute{n}\else \'{n}\fi{}czyk, M. J. and Tacca, M. and Talukder, D. and Tanner, D. B. and T\'apai, M. and Tarabrin, S. P. and Taracchini, A. and Taylor, R. and Theeg, T. and Thirugnanasambandam, M. P. and Thomas, E. G. and Thomas, M. and Thomas, P. and Thorne, K. A. and Thorne, K. S. and Thrane, E. and Tiwari, S. and Tiwari, V. and Tokmakov, K. V. and Tomlinson, C. and Tonelli, M. and Torres, C. V. and Torrie, C. I. and T\"oyr\"a, D. and Travasso, F. and Traylor, G. and Trifir\`o, D. and Tringali, M. C. and Trozzo, L. and Tse, M. and Turconi, M. and Tuyenbayev, D. and Ugolini, D. and Unnikrishnan, C. S. and Urban, A. L. and Usman, S. A. and Vahlbruch, H. and Vajente, G. and Valdes, G. and Vallisneri, M. and van Bakel, N. and van Beuzekom, M. and van den Brand, J. F. J. and Van Den Broeck, C. and Vander-Hyde, D. C. and van der Schaaf, L. and van Heijningen, J. V. and van Veggel, A. A. and Vardaro, M. and Vass, S. and Vas\'uth, M. and Vaulin, R. and Vecchio, A. and Vedovato, G. and Veitch, J. and Veitch, P. J. and Venkateswara, K. and Verkindt, D. and Vetrano, F. and Vicer\'e, A. and Vinciguerra, S. and Vine, D. J. and Vinet, J.-Y. and Vitale, S. and Vo, T. and Vocca, H. and Vorvick, C. and Voss, D. and Vousden, W. D. and Vyatchanin, S. P. and Wade, A. R. and Wade, L. E. and Wade, M. and Waldman, S. J. and Walker, M. and Wallace, L. and Walsh, S. and Wang, G. and Wang, H. and Wang, M. and Wang, X. and Wang, Y. and Ward, H. and Ward, R. L. and Warner, J. and Was, M. and Weaver, B. and Wei, L.-W. and Weinert, M. and Weinstein, A. J. and Weiss, R. and Welborn, T. and Wen, L. and We\ss{}els, P. and Westphal, T. and Wette, K. and Whelan, J. T. and Whitcomb, S. E. and White, D. J. and Whiting, B. F. and Wiesner, K. and Wilkinson, C. and Willems, P. A. and Williams, L. and Williams, R. D. and Williamson, A. R. and Willis, J. L. and Willke, B. and Wimmer, M. H. and Winkelmann, L. and Winkler, W. and Wipf, C. C. and Wiseman, A. G. and Wittel, H. and Woan, G. and Worden, J. and Wright, J. L. and Wu, G. and Yablon, J. and Yakushin, I. and Yam, W. and Yamamoto, H. and Yancey, C. C. and Yap, M. J. and Yu, H. and Yvert, M. and Zadro\ifmmode \dot{z}\else \.{z}\fi{}ny, A. and Zangrando, L. and Zanolin, M. and Zendri, J.-P. and Zevin, M. and Zhang, F. and Zhang, L. and Zhang, M. and Zhang, Y. and Zhao, C. and Zhou, M. and Zhou, Z. and Zhu, X. J. and Zucker, M. E. and Zuraw, S. E. and Zweizig, J.},
	Collaboration = {LIGO Scientific Collaboration and Virgo Collaboration},
	Date-Added = {2016-02-29 16:27:04 +0000},
	Date-Modified = {2016-02-29 16:27:12 +0000},
	Doi = {10.1103/PhysRevLett.116.061102},
	Issue = {6},
	Journal = {Phys. Rev. Lett.},
	Month = {Feb},
	Numpages = {16},
	Pages = {061102},
	Publisher = {American Physical Society},
	Title = {Observation of Gravitational Waves from a Binary Black Hole Merger},
	Url = {http://link.aps.org/doi/10.1103/PhysRevLett.116.061102},
	Volume = {116},
	Year = {2016},
	Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevLett.116.061102},
	Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevLett.116.061102}}

@article{Neben:2015,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2015RaSc...50..614N},
	Archiveprefix = {arXiv},
	Author = {{Neben}, A.~R. and {Bradley}, R.~F. and {Hewitt}, J.~N. and {Bernardi}, G. and {Bowman}, J.~D. and {Briggs}, F. and {Cappallo}, R.~J. and {Deshpande}, A.~A. and {Goeke}, R. and {Greenhill}, L.~J. and {Hazelton}, B.~J. and {Johnston-Hollitt}, M. and {Kaplan}, D.~L. and {Lonsdale}, C.~J. and {McWhirter}, S.~R. and {Mitchell}, D.~A. and {Morales}, M.~F. and {Morgan}, E. and {Oberoi}, D. and {Ord}, S.~M. and {Prabu}, T. and {Shankar}, N.~U. and {Srivani}, K.~S. and {Subrahmanyan}, R. and {Tingay}, S.~J. and {Wayth}, R.~B. and {Webster}, R.~L. and {Williams}, A. and {Williams}, C.~L.},
	Date-Added = {2016-01-28 18:57:47 +0000},
	Date-Modified = {2016-01-28 18:57:59 +0000},
	Doi = {10.1002/2015RS005678},
	Eprint = {1505.07114},
	Journal = {Radio Science},
	Keywords = {antenna arrays, radio astronomy, antennas},
	Month = jul,
	Pages = {614-629},
	Primaryclass = {astro-ph.IM},
	Title = {{Measuring phased-array antenna beampatterns with high dynamic range for the Murchison Widefield Array using 137 MHz ORBCOMM satellites}},
	Volume = 50,
	Year = 2015,
	Bdsk-Url-1 = {http://dx.doi.org/10.1002/2015RS005678}}

@article{Virone:2014,
	Author = {Virone, G. and Lingua, A.M. and Piras, M. and Cina, A. and Perini, F. and Monari, J. and Paonessa, F. and Peverini, O.A. and Addamo, G. and Tascone, R.},
	Date-Added = {2016-01-28 18:54:37 +0000},
	Date-Modified = {2016-01-28 18:54:43 +0000},
	Doi = {10.1109/LAWP.2014.2298250},
	Issn = {1536-1225},
	Journal = {Antennas and Wireless Propagation Letters, IEEE},
	Keywords = {HF antennas;UHF antennas;antenna radiation patterns;autonomous aerial vehicles;position measurement;wire antennas;UAV flying path;antenna radiation pattern verification system;autonomous flight;data processing;frequency 150 MHz;frequency 408 MHz;low-frequency antenna;microunmanned aerial vehicle;position measurement;remote topographic instrument;wire antenna;Accuracy;Antenna measurements;Antenna radiation patterns;Arrays;Power measurement;Soil;Soil measurements;Antenna measurements;antenna radiation pattern;radio astronomy;unmanned aerial vehicles},
	Pages = {169-172},
	Title = {Antenna Pattern Verification System Based on a Micro Unmanned Aerial Vehicle (UAV)},
	Volume = {13},
	Year = {2014},
	Bdsk-Url-1 = {http://dx.doi.org/10.1109/LAWP.2014.2298250}}

@article{Kazemi:2013,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2013MNRAS.430.1457K},
	Archiveprefix = {arXiv},
	Author = {{Kazemi}, S. and {Yatawatta}, S. and {Zaroubi}, S.},
	Date-Added = {2016-01-27 21:12:45 +0000},
	Date-Modified = {2016-01-27 21:12:53 +0000},
	Doi = {10.1093/mnras/stt018},
	Eprint = {1301.0633},
	Journal = {\mnras},
	Keywords = {methods: numerical, methods: statistical, techniques: interferometric},
	Month = apr,
	Pages = {1457-1472},
	Primaryclass = {astro-ph.IM},
	Title = {{Clustered calibration: an improvement to radio interferometric direction-dependent self-calibration}},
	Volume = 430,
	Year = 2013,
	Bdsk-Url-1 = {http://dx.doi.org/10.1093/mnras/stt018}}

@book{Kay:1993,
	Address = {Upper Saddle River, NJ, USA},
	Author = {Kay, Steven M.},
	Date-Added = {2016-01-27 21:11:39 +0000},
	Date-Modified = {2016-01-27 21:11:46 +0000},
	Isbn = {0-13-345711-7},
	Publisher = {Prentice-Hall, Inc.},
	Title = {Fundamentals of Statistical Signal Processing: Estimation Theory},
	Year = {1993}}

@article{Cohen:2007,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2007AJ....134.1245C},
	Archiveprefix = {arXiv},
	Author = {{Cohen}, A.~S. and {Lane}, W.~M. and {Cotton}, W.~D. and {Kassim}, N.~E. and {Lazio}, T.~J.~W. and {Perley}, R.~A. and {Condon}, J.~J. and {Erickson}, W.~C.},
	Date-Added = {2015-11-13 16:29:36 +0000},
	Date-Modified = {2015-11-13 16:29:48 +0000},
	Doi = {10.1086/520719},
	Eprint = {0706.1191},
	Journal = {\aj},
	Keywords = {atmospheric effects, catalogs, radio continuum: general, surveys, cyg-a},
	Month = sep,
	Pages = {1245-1262},
	Title = {{The VLA Low-Frequency Sky Survey}},
	Volume = 134,
	Year = 2007,
	Bdsk-Url-1 = {http://dx.doi.org/10.1086/520719}}

@article{Kassim:2007,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2007ApJS..172..686K},
	Archiveprefix = {arXiv},
	Author = {{Kassim}, N.~E. and {Lazio}, T.~J.~W. and {Erickson}, W.~C. and {Perley}, R.~A. and {Cotton}, W.~D. and {Greisen}, E.~W. and {Cohen}, A.~S. and {Hicks}, B. and {Schmitt}, H.~R. and {Katz}, D.},
	Date-Added = {2015-11-13 16:28:17 +0000},
	Date-Modified = {2015-11-13 16:29:08 +0000},
	Doi = {10.1086/519022},
	Eprint = {0704.3088},
	Journal = {\apjs},
	Keywords = {Astrometry, Instrumentation: Interferometers, Techniques: High Anular Resolution, Techniques: Image Processing, Techniques: Interferometric, cas-a},
	Month = oct,
	Pages = {686-719},
	Title = {{The 74 MHz System on the Very Large Array}},
	Volume = 172,
	Year = 2007,
	Bdsk-Url-1 = {http://dx.doi.org/10.1086/519022}}

@article{Thyagarajan:2015c,
	Author = {{Thyagarajan}, N. and {Beardsley}, A.~P. and {Bowman}, J.~D. and {Morales}, M.~F.},
	Date-Added = {2015-10-29 15:54:32 +0000},
	Date-Modified = {2015-10-29 16:11:38 +0000},
	Journal = {{arXiv:1510.08318}},
	Title = {{A Generic and Efficient E-field Parallel Imaging Correlator for Next-Generation Radio Telescopes}},
	Year = {2015}}

@inproceedings{Hay:2007,
	Author = {Hay, S.G. and O'Sullivan, J.D. and Kot, J.S. and Granet, C. and Grancea, A. and Forsyth, A.R. and Hayman, D.H.},
	Booktitle = {Antennas and Propagation, 2007. EuCAP 2007. The Second European Conference on},
	Date-Added = {2015-10-28 16:54:53 +0000},
	Date-Modified = {2015-10-28 16:54:53 +0000},
	Keywords = {focal planes;linear antenna arrays;radioastronomy;Australian SKA pathfinder;connected checkerboard array;linear array;radioastronomy;wideband focal plane array;Array;Focal plane;SKA},
	Month = {Nov},
	Pages = {1-5},
	Title = {Focal Plane Array Development for ASKAP (Australian SKA Pathfinder)},
	Year = {2007}}

@unpublished{Backer:2009,
	Author = {{Backer}, D.~C. and {Aguirre}, J.~E. and {Bowman}, J.~D. and {Bradley}, R. and {Carilli}, C.~L. and {Furlanetto}, S.~R. and {Greenhill}, L.~J. and {Hewitt}, J.~N. and {Lonsdale}, C. and {Ord}, S.~M. and Parsons, A. and {Whitney}, A.},
	Date-Added = {2015-10-28 00:13:22 +0000},
	Date-Modified = {2015-10-28 00:15:06 +0000},
	Title = {{HERA - Hydrogen Epoch of Reionization Arrays}},
	Url = {http://reionization.org/RFI2_HERA.pdf},
	Year = {2009},
	Bdsk-Url-1 = {http://reionization.org}}

@inproceedings{Benthem:2012,
	Author = {Benthem, P. and Kant, G.W.},
	Booktitle = {Antennas and Propagation (EUCAP), 2012 6th European Conference on},
	Date-Added = {2015-10-27 22:58:47 +0000},
	Date-Modified = {2015-10-27 22:58:51 +0000},
	Doi = {10.1109/EuCAP.2012.6206634},
	Keywords = {antenna phased arrays;aperture antennas;array signal processing;radioastronomy;radiotelescopes;EMBRACE;L-band;SKA;Square Kilometer Array frequencies;aperture array concept;electronic multibeam radio astronomy concept;phased array antenna;Antenna arrays;Apertures;Arrays;Bandwidth;Laser beams;Radio frequency;Tiles;antenna arrays;array design;array signal processing;mutual coupling;phased arrays;radio astronomy},
	Month = {March},
	Pages = {629-633},
	Title = {EMBRACE: Results from an aperture array for radio astronomy},
	Year = {2012},
	Bdsk-Url-1 = {http://dx.doi.org/10.1109/EuCAP.2012.6206634}}

@article{Obenberger:2014,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2014ApJ...785...27O},
	Archiveprefix = {arXiv},
	Author = {{Obenberger}, K.~S. and {Hartman}, J.~M. and {Taylor}, G.~B. and {Craig}, J. and {Dowell}, J. and {Helmboldt}, J.~F. and {Henning}, P.~A. and {Schinzel}, F.~K. and {Wilson}, T.~L.},
	Date-Added = {2015-10-26 18:51:54 +0000},
	Date-Modified = {2015-10-26 18:52:04 +0000},
	Doi = {10.1088/0004-637X/785/1/27},
	Eid = {27},
	Eprint = {1403.3674},
	Journal = {\apj},
	Keywords = {gamma-ray burst: general},
	Month = apr,
	Pages = {27},
	Primaryclass = {astro-ph.HE},
	Title = {{Limits on Gamma-Ray Burst Prompt Radio Emission Using the LWA1}},
	Volume = 785,
	Year = 2014,
	Bdsk-Url-1 = {http://dx.doi.org/10.1088/0004-637X/785/1/27}}

@article{Pober:2015,
	Abstract = {We present constraints on both the kinetic temperature of the intergalactic medium (IGM) at z = 8.4, and on models for heating the IGM at high-redshift with X-ray emission from the first collapsed objects. These constraints are derived using a semi-analytic method to explore the new measurements of the 21 cm power spectrum from the Donald C. Backer Precision Array for Probing the Epoch of Reionization (PAPER), which were presented in a companion paper, Ali et al. Twenty-one cm power spectra with amplitudes of hundreds of mK 2 can be generically produced if the kinetic temperature of the IGM is significantly below the temperature of the cosmic microwave background (CMB); as such, the new results from PAPER place lower limits on the IGM temperature at z = 8.4. Allowing for the unknown ionization state of the IGM, our measurements find the IGM temperature to be above ≈5 K for neutral fractions between 10% and 85%, above ≈7 K for neutral fractions between 15% and 80%, or above ≈10 K for neutral fractions between 30% and 70%. We also calculate the heating of the IGM that would be provided by the observed high redshift galaxy population, and find that for most models, these galaxies are sufficient to bring the IGM temperature above our lower limits. However, there are significant ranges of parameter space that could produce a signal ruled out by the PAPER measurements; models with a steep drop-off in the star formation rate density at high redshifts or with relatively low values for the X-ray to star formation rate efficiency of high redshift galaxies are generally disfavored. The PAPER measurements are consistent with (but do not constrain) a hydrogen spin temperature above the CMB temperature, a situation which we find to be generally predicted if galaxies fainter than the current detection limits of optical/NIR surveys are included in calculations of X-ray heating.},
	Author = {Jonathan C. Pober and Zaki S. Ali and Aaron R. Parsons and Matthew McQuinn and James E. Aguirre and Gianni Bernardi and Richard F. Bradley and Chris L. Carilli and Carina Cheng and David R. DeBoer and Matthew R. Dexter and Steven R. Furlanetto and Jasper Grobbelaar and Jasper Horrell and Daniel C. Jacobs and Patricia J. Klima and Saul A. Kohn and Adrian Liu and David H. E. MacMahon and Matthys Maree and Andrei Mesinger and David F. Moore and Nima Razavi-Ghods and Irina I. Stefan and William P. Walbrugh and Andre Walker and Haoxuan Zheng},
	Date-Added = {2015-10-23 15:46:57 +0000},
	Date-Modified = {2015-10-23 15:47:02 +0000},
	Journal = {The Astrophysical Journal},
	Number = {1},
	Pages = {62},
	Title = {PAPER-64 Constraints On Reionization. II. The Temperature of the z =8.4 Intergalactic Medium},
	Url = {http://stacks.iop.org/0004-637X/809/i=1/a=62},
	Volume = {809},
	Year = {2015},
	Bdsk-Url-1 = {http://stacks.iop.org/0004-637X/809/i=1/a=62}}

@article{Hicks:2012,
	Abstract = {ABSTRACT. We describe an ``active'' antenna system for HF/VHF (long wavelength) radio astronomy that has been successfully deployed 256-fold as the first station (LWA1) of the planned Long Wavelength Array. The antenna system, consisting of crossed dipoles, an active balun/preamp, a support structure, and a ground screen has been shown to successfully operate over at least the band from 20 MHz (15 m wavelength) to 80 MHz (3.75 m wavelength) with a noise figure that is at least 6 dB better than the Galactic background emission-noise temperature over that band. Thus, we met the goal to design and construct a compact, inexpensive, rugged, and easily assembled antenna system that can be deployed many-fold to form numerous large individual ``stations'' for the purpose of building a large, long wavelength synthesis array telescope for radio astronomical and ionospheric observations.},
	Author = {Hicks, Brian C. and Paravastu-Dalal, Nagini and Stewart, Kenneth P. and Erickson, William C. and Ray, Paul S. and Kassim, Namir E. and Burns, Steve and Clarke, Tracy and Schmitt, Henrique and Craig, Joe and Hartman, Jake and Weiler, Kurt W.},
	Copyright = {Copyright {\copyright} 2012 The University of Chicago Press},
	Date-Added = {2015-10-19 17:43:21 +0000},
	Date-Modified = {2015-10-19 17:43:26 +0000},
	Issn = {00046280},
	Journal = {Publications of the Astronomical Society of the Pacific},
	Jstor_Articletype = {research-article},
	Jstor_Formatteddate = {October 2012},
	Language = {English},
	Number = {920},
	Pages = {pp. 1090-1104},
	Publisher = {The University of Chicago Press on behalf of the Astronomical Society of the Pacific},
	Title = {A Wide-Band, Active Antenna System for Long Wavelength Radio Astronomy},
	Url = {http://www.jstor.org/stable/10.1086/668121},
	Volume = {124},
	Year = {2012},
	Bdsk-Url-1 = {http://www.jstor.org/stable/10.1086/668121}}

@article{Dowell:2012,
	Author = {DOWELL, JAYCE and WOOD, DANIEL and STOVALL, KEVIN and RAY, PAUL S. and CLARKE, TRACY and TAYLOR, GREGORY},
	Date-Added = {2015-10-19 17:07:06 +0000},
	Date-Modified = {2015-10-19 17:07:22 +0000},
	Doi = {10.1142/S2251171712500067},
	Eprint = {http://www.worldscientific.com/doi/pdf/10.1142/S2251171712500067},
	Journal = {Journal of Astronomical Instrumentation},
	Number = {01},
	Pages = {1250006},
	Title = {THE LONG WAVELENGTH ARRAY SOFTWARE LIBRARY},
	Url = {http://www.worldscientific.com/doi/abs/10.1142/S2251171712500067},
	Volume = {01},
	Year = {2012},
	Bdsk-Url-1 = {http://www.worldscientific.com/doi/abs/10.1142/S2251171712500067},
	Bdsk-Url-2 = {http://dx.doi.org/10.1142/S2251171712500067}}

@article{Zheng:2014,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2014MNRAS.445.1084Z},
	Archiveprefix = {arXiv},
	Author = {{Zheng}, H. and {Tegmark}, M. and {Buza}, V. and {Dillon}, J.~S. and {Gharibyan}, H. and {Hickish}, J. and {Kunz}, E. and {Liu}, A. and {Losh}, J. and {Lutomirski}, A. and {Morrison}, S. and {Narayanan}, S. and {Perko}, A. and {Rosner}, D. and {Sanchez}, N. and {Schutz}, K. and {Tribiano}, S.~M. and {Valdez}, M. and {Yang}, H. and {Adami}, K.~Z. and {Zelko}, I. and {Zheng}, K. and {Armstrong}, R.~P. and {Bradley}, R.~F. and {Dexter}, M.~R. and {Ewall-Wice}, A. and {Magro}, A. and {Matejek}, M. and {Morgan}, E. and {Neben}, A.~R. and {Pan}, Q. and {Penna}, R.~F. and {Peterson}, C.~M. and {Su}, M. and {Villasenor}, J. and {Williams}, C.~L. and {Zhu}, Y.},
	Date-Added = {2015-10-15 20:00:54 +0000},
	Date-Modified = {2015-10-15 20:01:01 +0000},
	Doi = {10.1093/mnras/stu1773},
	Eprint = {1405.5527},
	Journal = {\mnras},
	Keywords = {instrumentation: interferometers, methods: data analysis, techniques: interferometric, cosmology: observations, dark ages, reionization, first stars},
	Month = dec,
	Pages = {1084-1103},
	Primaryclass = {astro-ph.IM},
	Title = {{MITEoR: a scalable interferometer for precision 21 cm cosmology}},
	Volume = 445,
	Year = 2014,
	Bdsk-Url-1 = {http://dx.doi.org/10.1093/mnras/stu1773}}

@article{Mellema:2013,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2013ExA....36..235M},
	Archiveprefix = {arXiv},
	Author = {{Mellema}, G. and {Koopmans}, L.~V.~E. and {Abdalla}, F.~A. and {Bernardi}, G. and {Ciardi}, B. and {Daiboo}, S. and {de Bruyn}, A.~G. and {Datta}, K.~K. and {Falcke}, H. and {Ferrara}, A. and {Iliev}, I.~T. and {Iocco}, F. and {Jeli{\'c}}, V. and {Jensen}, H. and {Joseph}, R. and {Labroupoulos}, P. and {Meiksin}, A. and {Mesinger}, A. and {Offringa}, A.~R. and {Pandey}, V.~N. and {Pritchard}, J.~R. and {Santos}, M.~G. and {Schwarz}, D.~J. and {Semelin}, B. and {Vedantham}, H. and {Yatawatta}, S. and {Zaroubi}, S.},
	Date-Added = {2015-10-15 19:47:02 +0000},
	Date-Modified = {2015-10-15 19:47:08 +0000},
	Doi = {10.1007/s10686-013-9334-5},
	Eprint = {1210.0197},
	Journal = {Experimental Astronomy},
	Keywords = {Cosmology: Observations, Dark ages, Reionization, First stars, Diffuse radiation, Intergalactic medium, Radio lines: General, Techniques: Interferometric},
	Month = aug,
	Pages = {235-318},
	Title = {{Reionization and the Cosmic Dawn with the Square Kilometre Array}},
	Volume = 36,
	Year = 2013,
	Bdsk-Url-1 = {http://dx.doi.org/10.1007/s10686-013-9334-5}}

@article{Ellingson:2013,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2013ITAP...61.2540E},
	Archiveprefix = {arXiv},
	Author = {{Ellingson}, S.~W. and {Taylor}, G.~B. and {Craig}, J. and {Hartman}, J. and {Dowell}, J. and {Wolfe}, C.~N. and {Clarke}, T.~E. and {Hicks}, B.~C. and {Kassim}, N.~E. and {Ray}, P.~S. and {Rickard}, L.~J. and {Schinzel}, F.~K. and {Weiler}, K.~W.},
	Date-Added = {2015-10-15 17:17:33 +0000},
	Date-Modified = {2015-10-15 17:17:43 +0000},
	Doi = {10.1109/TAP.2013.2242826},
	Eprint = {1204.4816},
	Journal = {IEEE Transactions on Antennas and Propagation},
	Month = may,
	Pages = {2540-2549},
	Primaryclass = {astro-ph.IM},
	Title = {{The LWA1 Radio Telescope}},
	Volume = 61,
	Year = 2013,
	Bdsk-Url-1 = {http://dx.doi.org/10.1109/TAP.2013.2242826}}

@inproceedings{Bandura:2014,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2014SPIE.9145E..22B},
	Archiveprefix = {arXiv},
	Author = {{Bandura}, K. and {Addison}, G.~E. and {Amiri}, M. and {Bond}, J.~R. and {Campbell-Wilson}, D. and {Connor}, L. and {Cliche}, J.-F. and {Davis}, G. and {Deng}, M. and {Denman}, N. and {Dobbs}, M. and {Fandino}, M. and {Gibbs}, K. and {Gilbert}, A. and {Halpern}, M. and {Hanna}, D. and {Hincks}, A.~D. and {Hinshaw}, G. and {H{\"o}fer}, C. and {Klages}, P. and {Landecker}, T.~L. and {Masui}, K. and {Mena Parra}, J. and {Newburgh}, L.~B. and {Pen}, U.-l. and {Peterson}, J.~B. and {Recnik}, A. and {Shaw}, J.~R. and {Sigurdson}, K. and {Sitwell}, M. and {Smecher}, G. and {Smegal}, R. and {Vanderlinde}, K. and {Wiebe}, D.},
	Booktitle = {Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series},
	Date-Added = {2015-10-15 17:14:08 +0000},
	Date-Modified = {2015-10-15 17:14:15 +0000},
	Doi = {10.1117/12.2054950},
	Eid = {914522},
	Eprint = {1406.2288},
	Month = jul,
	Pages = {22},
	Primaryclass = {astro-ph.IM},
	Series = {Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series},
	Title = {{Canadian Hydrogen Intensity Mapping Experiment (CHIME) pathfinder}},
	Volume = 9145,
	Year = 2014,
	Bdsk-Url-1 = {http://dx.doi.org/10.1117/12.2054950}}

@article{Tegmark:2009,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2009PhRvD..79h3530T},
	Archiveprefix = {arXiv},
	Author = {{Tegmark}, M. and {Zaldarriaga}, M.},
	Date-Added = {2015-10-15 15:39:46 +0000},
	Date-Modified = {2015-10-15 15:39:55 +0000},
	Doi = {10.1103/PhysRevD.79.083530},
	Eid = {083530},
	Eprint = {0805.4414},
	Journal = {\prd},
	Keywords = {Observational cosmology},
	Month = apr,
	Number = 8,
	Pages = {083530},
	Title = {{Fast Fourier transform telescope}},
	Volume = 79,
	Year = 2009,
	Bdsk-Url-1 = {http://dx.doi.org/10.1103/PhysRevD.79.083530}}

@article{Bunton:2004,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2004ExA....17..251B},
	Author = {{Bunton}, J.~D.},
	Date-Added = {2015-10-15 15:37:27 +0000},
	Date-Modified = {2015-10-15 15:37:34 +0000},
	Doi = {10.1007/s10686-005-5661-5},
	Journal = {Experimental Astronomy},
	Keywords = {correlator, FX, XF, filterbank, radio astronomy, SKA},
	Month = jun,
	Pages = {251-259},
	Title = {{Ska Correlator Advances}},
	Volume = 17,
	Year = 2004,
	Bdsk-Url-1 = {http://dx.doi.org/10.1007/s10686-005-5661-5}}

@inproceedings{Lonsdale:2000,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2000SPIE.4015..126L},
	Author = {{Lonsdale}, C.~J. and {Doeleman}, S.~S. and {Cappallo}, R.~J. and {Hewitt}, J.~N. and {Whitney}, A.~R.},
	Booktitle = {Radio Telescopes},
	Date-Added = {2015-10-15 15:32:34 +0000},
	Date-Modified = {2015-10-15 15:32:38 +0000},
	Editor = {{Butcher}, H.~R.},
	Month = jul,
	Pages = {126-134},
	Series = {Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series},
	Title = {{Exploring the performance of large-N radio astronomical arrays}},
	Volume = 4015,
	Year = 2000}

@article{Jiang:2013,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2013ApJ...772...99J},
	Archiveprefix = {arXiv},
	Author = {{Jiang}, L. and {Egami}, E. and {Mechtley}, M. and {Fan}, X. and {Cohen}, S.~H. and {Windhorst}, R.~A. and {Dav{\'e}}, R. and {Finlator}, K. and {Kashikawa}, N. and {Ouchi}, M. and {Shimasaku}, K.},
	Date-Added = {2015-10-14 16:21:04 +0000},
	Date-Modified = {2015-10-14 16:21:11 +0000},
	Doi = {10.1088/0004-637X/772/2/99},
	Eid = {99},
	Eprint = {1303.0024},
	Journal = {\apj},
	Keywords = {cosmology: observations, galaxies: evolution, galaxies: high-redshift},
	Month = aug,
	Pages = {99},
	Title = {{Physical Properties of Spectroscopically Confirmed Galaxies at z {\gt}= 6. I. Basic Characteristics of the Rest-frame UV Continuum and Ly{$\alpha$} Emission}},
	Volume = 772,
	Year = 2013,
	Bdsk-Url-1 = {http://dx.doi.org/10.1088/0004-637X/772/2/99}}

@article{Ali:2015,
	Abstract = {In this paper, we report new limits on 21 cm emission from cosmic reionization based on a 135 day observing campaign with a 64-element deployment of the Donald C. Backer Precision Array for Probing the Epoch of Reionization in South Africa. This work extends the work presented in Parsons et al. with more collecting area, a longer observing period, improved redundancy-based calibration, improved fringe-rate filtering, and updated power-spectral analysis using optimal quadratic estimators. The result is a new 2 {\"I}ƒ upper limit on {\^I}” 2 ( k ) of (22.4 mK) 2 in the range ##IMG## [http://ej.iop.org/images/0004-637X/809/1/61/apj517488ieqn1.gif] {$0.15\lt k\lt 0.5h\;{\mathrm{Mpc}}^{-1}$} at z = 8.4. This represents a three-fold improvement over the previous best upper limit. As we discuss in more depth in a forthcoming paper, this upper limit supports and extends previous evidence against extremely cold reionization scenarios. We conclude with a discussion of implications for future 21 cm reionization experiments, including the newly funded Hydrogen Epoch of Reionization Array.},
	Author = {Zaki S. Ali and Aaron R. Parsons and Haoxuan Zheng and Jonathan C. Pober and Adrian Liu and James E. Aguirre and Richard F. Bradley and Gianni Bernardi and Chris L. Carilli and Carina Cheng and David R. DeBoer and Matthew R. Dexter and Jasper Grobbelaar and Jasper Horrell and Daniel C. Jacobs and Pat Klima and David H. E. MacMahon and Matthys Maree and David F. Moore and Nima Razavi and Irina I. Stefan and William P. Walbrugh and Andre Walker},
	Date-Added = {2015-10-13 17:35:17 +0000},
	Date-Modified = {2015-10-13 17:35:28 +0000},
	Journal = {The Astrophysical Journal},
	Number = {1},
	Pages = {61},
	Title = {PAPER-64 Constraints on Reionization: The 21 cm Power Spectrum at z = 8.4},
	Url = {http://stacks.iop.org/0004-637X/809/i=1/a=61},
	Volume = {809},
	Year = {2015},
	Bdsk-Url-1 = {http://stacks.iop.org/0004-637X/809/i=1/a=61}}

@phdthesis{Beardsley:thesis,
	Author = {{Beardsley}, A.~P.},
	Date-Added = {2015-10-12 17:00:35 +0000},
	Date-Modified = {2015-10-12 17:01:26 +0000},
	School = {{University of Washington}},
	Title = {{The Murchison Widefield Array 21cm Epoch of Reionization Experiment: Design, Construction, and First Season Results}},
	Year = {2015},
	Bdsk-File-1 = {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}}

@article{Foster:2014,
	Abstract = {A new digital backend has been developed for the Basic Element for SKA Training II (BEST-2) array at Radiotelescopi di Medicina, INAF-IRA, Italy, which allows concurrent operation of an FX correlator, and a direct-imaging correlator and beamformer. This backend serves as a platform for testing some of the spatial Fourier transform concepts which have been proposed for use in computing correlations on regularly gridded arrays. While spatial Fourier transform-based beamformers have been implemented previously, this is, to our knowledge, the first time a direct-imaging correlator has been deployed on a radio astronomy array. Concurrent observations with the FX and direct-imaging correlator allow for direct comparison between the two architectures. Additionally, we show the potential of the direct-imaging correlator for time-domain astronomy, by passing a subset of beams though a pulsar and transient detection pipeline. These results provide a timely verification for spatial Fourier transform-based instruments that are currently in commissioning. These instruments aim to detect highly redshifted hydrogen from the epoch of reionization and/or to perform wide-field surveys for time-domain studies of the radio sky. We experimentally show the direct-imaging correlator architecture to be a viable solution for correlation and beamforming.},
	Author = {Foster, G. and Hickish, J. and Magro, A. and Price, D. and Zarb Adami, K.},
	Date-Added = {2015-10-09 15:34:45 +0000},
	Date-Modified = {2015-10-09 15:34:52 +0000},
	Doi = {10.1093/mnras/stu188},
	Eprint = {http://mnras.oxfordjournals.org/content/439/3/3180.full.pdf+html},
	Journal = {Monthly Notices of the Royal Astronomical Society},
	Number = {3},
	Pages = {3180-3188},
	Title = {Implementation of a direct-imaging and FX correlator for the BEST-2 array},
	Url = {http://mnras.oxfordjournals.org/content/439/3/3180.abstract},
	Volume = {439},
	Year = {2014},
	Bdsk-Url-1 = {http://mnras.oxfordjournals.org/content/439/3/3180.abstract},
	Bdsk-Url-2 = {http://dx.doi.org/10.1093/mnras/stu188}}

@article{deVos:2009,
	Author = {de Vos, M. and Gunst, A.W. and Nijboer, R.},
	Date-Added = {2015-10-09 15:33:22 +0000},
	Date-Modified = {2015-10-09 15:33:30 +0000},
	Doi = {10.1109/JPROC.2009.2020509},
	Issn = {0018-9219},
	Journal = {Proceedings of the IEEE},
	Keywords = {antenna phased arrays;aperture antennas;array signal processing;directive antennas;radiotelescopes;LOFAR telescope;aperture synthesis array;distributed radio telescope;flexible station-based signal processing;low frequency array;omnidirectional antennas;phased array antenna;software correlator;square kilometer array;system architecture;tied array beamformer;Antenna arrays;Aperture antennas;Array signal processing;Calibration;Frequency synthesizers;Phased arrays;Radio astronomy;Signal processing;Signal synthesis;Telescopes;Aperture synthesis;low-frequency astronomy;multibeaming;phased array;radio astronomy},
	Month = {Aug},
	Number = {8},
	Pages = {1431-1437},
	Title = {The LOFAR Telescope: System Architecture and Signal Processing},
	Volume = {97},
	Year = {2009},
	Bdsk-Url-1 = {http://dx.doi.org/10.1109/JPROC.2009.2020509}}

@article{Wijnholds:2009,
	Author = {Wijnholds, S.J. and van der Veen, A.-J.},
	Date-Added = {2015-10-09 15:30:53 +0000},
	Date-Modified = {2015-10-09 15:31:01 +0000},
	Doi = {10.1109/TSP.2009.2022894},
	Issn = {1053-587X},
	Journal = {Signal Processing, IEEE Transactions on},
	Keywords = {Monte Carlo methods;array signal processing;iterative methods;least mean squares methods;Monte Carlo simulation;array signal processing;direction dependent gain pattern;iterative method;multiple calibrator sources;multisource self-calibration;refractive propagation path;sensor arrays;signal to noise ratio;weighted alternating least squares algorithm;weighted subspace fitting direction finding techniques;Array signal processing;radio astronomy;self-calibration},
	Month = {Sept},
	Number = {9},
	Pages = {3512-3522},
	Title = {Multisource Self-Calibration for Sensor Arrays},
	Volume = {57},
	Year = {2009},
	Bdsk-Url-1 = {http://dx.doi.org/10.1109/TSP.2009.2022894}}

@article{Liu:2015,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2015arXiv150908463L},
	Archiveprefix = {arXiv},
	Author = {{Liu}, A. and {Pritchard}, J.~R. and {Allison}, R. and {Parsons}, A.~R. and {Seljak}, U. and {Sherwin}, B.~D.},
	Date-Added = {2015-10-05 21:21:18 +0000},
	Date-Modified = {2015-10-05 21:21:23 +0000},
	Eprint = {1509.08463},
	Journal = {ArXiv e-prints},
	Keywords = {Astrophysics - Cosmology and Nongalactic Astrophysics},
	Month = sep,
	Title = {{Eliminating the optical depth nuisance from the CMB with 21 cm cosmology}},
	Year = 2015}

@article{Greig:2015,
	Abstract = {We introduce 21 CMMC: a parallelized, Monte Carlo Markov Chain analysis tool, incorporating the epoch of reionization (EoR) seminumerical simulation 21 CMFAST. 21 CMMC estimates astrophysical parameter constraints from 21 cm EoR experiments, accommodating a variety of EoR models, as well as priors on model parameters and the reionization history. To illustrate its utility, we consider two different EoR scenarios, one with a single population of galaxies
(with a mass-independent ionizing efficiency) and a second, more general model with two different, feedback-regulated populations (each with mass-dependent ionizing efficiencies). As an example, combining three observations (z = 8, 9 and 10) of the 21 cm power spectrum with a conservative noise estimate and uniform model priors, we find that interferometers with specifications like the Low Frequency Array/Hydrogen Epoch of Reionization Array (HERA)/Square Kilometre Array 1 (SKA1) can constrain common reionization parameters: the ionizing efficiency (or similarly the escape fraction), the mean free path of ionizing photons and the log of the minimum virial temperature of star-forming haloes to within 45.3/22.0/16.7, 33.5/18.4/17.8 and 6.3/3.3/2.4 per cent, ∼1σ fractional uncertainty, respectively. Instead, if we optimistically assume that we can perfectly characterize the EoR modelling uncertainties, we can improve on these constraints by up to a factor of ∼few. Similarly, the fractional uncertainty on the average neutral fraction can be constrained to within ≲ 10 per cent for HERA and SKA1. By studying the resulting impact on astrophysical constraints, 21 CMMC can be used to optimize (i) interferometer designs; (ii) foreground cleaning algorithms; (iii) observing strategies; (iv) alternative statistics characterizing the 21 cm signal; and (v) synergies with other observational programs.},
	Author = {Greig, Bradley and Mesinger, Andrei},
	Date-Added = {2015-10-05 18:41:13 +0000},
	Date-Modified = {2015-10-23 15:48:06 +0000},
	Doi = {10.1093/mnras/stv571},
	Journal = {Monthly Notices of the Royal Astronomical Society},
	Number = {4},
	Pages = {4246-4263},
	Title = {21CMMC: an MCMC analysis tool enabling astrophysical parameter studies of the cosmic 21 cm signal},
	Url = {http://mnras.oxfordjournals.org/content/449/4/4246.abstract},
	Volume = {449},
	Year = {2015},
	Bdsk-Url-1 = {http://mnras.oxfordjournals.org/content/449/4/4246.abstract},
	Bdsk-Url-2 = {http://dx.doi.org/10.1093/mnras/stv571}}

@article{Tremblay:2015,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2015PASA...32....5T},
	Archiveprefix = {arXiv},
	Author = {{Tremblay}, S.~E. and {Ord}, S.~M. and {Bhat}, N.~D.~R. and {Tingay}, S.~J. and {Crosse}, B. and {Pallot}, D. and {Oronsaye}, S.~I. and {Bernardi}, G. and {Bowman}, J.~D. and {Briggs}, F. and {Cappallo}, R.~J. and {Corey}, B.~E. and {Deshpande}, A.~A. and {Emrich}, D. and {Goeke}, R. and {Greenhill}, L.~J. and {Hazelton}, B.~J. and {Johnston-Hollitt}, M. and {Kaplan}, D.~L. and {Kasper}, J.~C. and {Kratzenberg}, E. and {Lonsdale}, C.~J. and {Lynch}, M.~J. and {McWhirter}, S.~R. and {Mitchell}, D.~A. and {Morales}, M.~F. and {Morgan}, E. and {Oberoi}, D. and {Prabu}, T. and {Rogers}, A.~E.~E. and {Roshi}, A. and {Udaya Shankar}, N. and {Srivani}, K.~S. and {Subrahmanyan}, R. and {Waterson}, M. and {Wayth}, R.~B. and {Webster}, R.~L. and {Whitney}, A.~R. and {Williams}, A. and {Williams}, C.~L.},
	Date-Added = {2015-09-21 19:31:51 +0000},
	Date-Modified = {2016-03-10 20:59:16 +0000},
	Doi = {10.1017/pasa.2015.6},
	Eid = {e005},
	Eprint = {1501.05723},
	Journal = {PASA - Publications of the Astronomical Society of Australia},
	Keywords = {instrumentation: interferometers, pulsars: general, radio continuum: general, Sun: radio radiation, techniques: radar astronomy},
	Month = feb,
	Pages = {5},
	Primaryclass = {astro-ph.IM},
	Title = {{The High Time and Frequency Resolution Capabilities of the Murchison Widefield Array}},
	Volume = 32,
	Year = 2015,
	Bdsk-Url-1 = {http://dx.doi.org/10.1017/pasa.2015.6}}

@article{Otobe:1994,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/1994PASJ...46..503O},
	Author = {{Otobe}, E. and {Nakajima}, J. and {Nishibori}, K. and {Saito}, T. and {Kobayashi}, H. and {Tanaka}, N. and {Watanabe}, N. and {Aramaki}, Y. and {Hoshikawa}, T. and {Asuma}, K. and {Daishido}, T.},
	Date-Added = {2015-09-21 18:49:31 +0000},
	Date-Modified = {2015-09-21 18:49:38 +0000},
	Journal = {\pasj},
	Keywords = {Calibrating, Crab Nebula, Error Analysis, Fast Fourier Transformations, Image Processing, Imaging Techniques, Radio Astronomy, Radio Emission, Instrument Errors, Phase Error, Pulsars, Radio Interferometers},
	Month = oct,
	Pages = {503-510},
	Title = {{Two-dimensional direct images with a spatial FFT interferometer}},
	Volume = 46,
	Year = 1994}

@article{Takeuchi:2000,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2000PASJ...52..267T},
	Author = {{Takeuchi}, H. and {Akamine}, Y. and {Fujii}, F. and {Kuniyoshi}, M. and {Suemitsu}, T. and {Gotoh}, K. and {Mizuki}, S. and {Mizuno}, K. and {Suzuki}, T. and {Fukuoka}, K. and {Tanaka}, N. and {Daishido}, T.},
	Date-Added = {2015-09-21 18:48:43 +0000},
	Date-Modified = {2015-09-21 18:48:50 +0000},
	Doi = {10.1093/pasj/52.2.267},
	Journal = {\pasj},
	Keywords = {GRAPH THEORY, INSTRUMENTATION: INTERFEROMETERS, METHODS: DATA ANALYSIS, SURVEYS},
	Month = apr,
	Pages = {267},
	Title = {{The Minimum Spanning Tree Problem in the Phase Calibration for the Spatial FFT Interferometer}},
	Volume = 52,
	Year = 2000,
	Bdsk-Url-1 = {http://dx.doi.org/10.1093/pasj/52.2.267}}

@article{Daishido:2000,
	Abstract = {An 8 X 8 equals 64 element digital interferometer was developed at Waseda University (1989 - 1995). It was an equally spaced two dimensional array of 2.4 m dishes at 10.6 GHz, and a 2D FFT processor was used for Nyquist rate imaging. Recently a spatial-temporal (2 + 1)D FFT processor has been developed for pulsar survey (1996 - 2000), in which a first 2D spatial FFT transforms the electric fields of coordinate represented to those of momentum represented. We obtain the electric fields in each 64 direction at Nyquist rate by the 2D spatial Fourier transform. The following temporal 1D FFT gives the spectrum of 64ch or 256ch to 64 directions respectively also at Nyquist rate. The total bandwidths of each direction are 20 MHz and the resulting frequency resolutions are 20/64 MHz or 20/256 MHz. For sensitive pulsar survey, we also have developed an interferometric array of 20 m spherical dishes in Nasu flat, 160 km north of Tokyo. Five dishes are completed at present. Normal temperature receivers of high electron mobility transistors (HEMT) are used at 1.4 GHz observation and the receiver noise temperatures are below 40 K. Expected rms detection limit (Delta) T is about 10-2K under the condition of 20 MHz band widths and 1s integration time. Preliminary results of zenith survey at (delta) equals 40 deg using a single dish show (Delta) T equals 0.03 K without switching. Sub-reflectors and feed horns were designed so as to observe 5 deg off directions from zenith and they rotate around Az axis. It enable us to survey the declination zone of 32 <EQ (delta) <EQ 42 deg.},
	Author = {Daishido, Tsuneaki and Tanaka, Naoki and Takeuchi, Hiroshi and Akamine, Yukinori and Fujii, Fumiyuki and Kuniyoshi, Masaya and Suemitsu, Taisei and Gotoh, Kentaro and Mizuki, Saori and Mizuno, Keiju and Suzuki, Tomoya and Asuma, Kuniyuki},
	Date-Added = {2015-09-21 18:43:31 +0000},
	Date-Modified = {2015-09-21 19:34:09 +0000},
	Doi = {10.1117/12.390458},
	Journal = {Proc. SPIE},
	Pages = {73-85},
	Title = {Pulsar huge array with Nyquist-rate digital lens and prism},
	Url = {http://dx.doi.org/10.1117/12.390458},
	Volume = {4015},
	Year = {2000},
	Bdsk-Url-1 = {http://dx.doi.org/10.1117/12.390458}}

@article{Tegmark:2010,
	Author = {Tegmark, Max and Zaldarriaga, Matias},
	Date-Added = {2015-09-21 18:13:30 +0000},
	Date-Modified = {2015-09-21 18:13:38 +0000},
	Doi = {10.1103/PhysRevD.82.103501},
	Issue = {10},
	Journal = {Phys. Rev. D},
	Month = {Nov},
	Numpages = {10},
	Pages = {103501},
	Publisher = {American Physical Society},
	Title = {Omniscopes: Large area telescope arrays with only $N\mathrm{log}{}N$ computational cost},
	Url = {http://link.aps.org/doi/10.1103/PhysRevD.82.103501},
	Volume = {82},
	Year = {2010},
	Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevD.82.103501},
	Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevD.82.103501}}

@article{Thyagarajan:2015,
	Abstract = {Detection of 21 cm emission of H i from the epoch of reionization, at redshifts ##IMG## [http://ej.iop.org/images/0004-637X/804/1/14/apj510820ieqn1.gif] {$z\gt 6$} , is limited primarily by foreground emission. We investigate the signatures of wide-field measurements and an all-sky foreground model using the delay spectrum technique that maps the measurements to foreground object locations through signal delays between antenna pairs. We demonstrate interferometric measurements are inherently sensitive to all scales, including the largest angular scales, owing to the nature of wide-field measurements. These wide-field effects are generic to all observations but antenna shapes impact their amplitudes substantially. A dish-shaped antenna yields the most desirable features from a foreground contamination viewpoint, relative to a dipole or a phased array. Comparing data from recent Murchison Widefield Array observations, we demonstrate that the foreground signatures that have the largest impact on the H i signal arise from power received far away from the primary field of view. We identify diffuse emission near the horizon as a significant contributing factor, even on wide antenna spacings that usually represent structures on small scales. For signals entering through the primary field of view, compact emission dominates the foreground contamination. These two mechanisms imprint a characteristic pitchfork signature on the ``foreground wedge'' in Fourier delay space. Based on these results, we propose that selective down-weighting of data based on antenna spacing and time can mitigate foreground contamination substantially by a factor of ∼100 with negligible loss of sensitivity.},
	Author = {Nithyanandan Thyagarajan and Daniel C. Jacobs and Judd D. Bowman and N. Barry and A. P. Beardsley and G. Bernardi and F. Briggs and R. J. Cappallo and P. Carroll and B. E. Corey and A. de Oliveira-Costa and Joshua S. Dillon and D. Emrich and A. Ewall-Wice and L. Feng and R. Goeke and L. J. Greenhill and B. J. Hazelton and J. N. Hewitt and N. Hurley-Walker and M. Johnston-Hollitt and D. L. Kaplan and J. C. Kasper and Han-Seek Kim and P. Kittiwisit and E. Kratzenberg and E. Lenc and J. Line and A. Loeb and C. J. Lonsdale and M. J. Lynch and B. McKinley and S. R. McWhirter and D. A. Mitchell and M. F. Morales and E. Morgan and A. R. Neben and D. Oberoi and A. R. Offringa and S. M. Ord and Sourabh Paul and B. Pindor and J. C. Pober and T. Prabu and P. Procopio and J. Riding and A. E. E. Rogers and A. Roshi and N. Udaya Shankar and Shiv K. Sethi and K. S. Srivani and R. Subrahmanyan and I. S. Sullivan and M. Tegmark and S. J. Tingay and C. M. Trott and M. Waterson and R. B. Wayth and R. L. Webster and A. R. Whitney and A. Williams and C. L. Williams and C. Wu and J. S. B. Wyithe},
	Date-Added = {2015-08-25 15:34:57 +0000},
	Date-Modified = {2015-08-25 15:35:05 +0000},
	Journal = {The Astrophysical Journal},
	Number = {1},
	Pages = {14},
	Title = {Foregrounds in Wide-field Redshifted 21 cm Power Spectra},
	Url = {http://stacks.iop.org/0004-637X/804/i=1/a=14},
	Volume = {804},
	Year = {2015},
	Bdsk-Url-1 = {http://stacks.iop.org/0004-637X/804/i=1/a=14}}

@article{Thyagarajan:2015b,
	Abstract = {We confirm our recent prediction of the ``pitchfork'' foreground signature in power spectra of high-redshift 21 cm measurements where the interferometer is sensitive to large-scale structure on all baselines. This is due to the inherent response of a wide-field instrument and is characterized by enhanced power from foreground emission in Fourier modes adjacent to those considered to be the most sensitive to the cosmological H i signal. In our recent paper, many signatures from the simulation that predicted this feature were validated against Murchison Widefield Array (MWA) data, but this key pitchfork signature was close to the noise level. In this paper, we improve the data sensitivity through the coherent averaging of 12 independent snapshots with identical instrument settings and provide the first confirmation of the prediction with a signal-to-noise ratio ##IMG## [http://ej.iop.org/images/2041-8205/807/2/L28/apjl516554ieqn1.gif] {$\gt 10$} . This wide-field effect can be mitigated by careful antenna designs that suppress sensitivity near the horizon. Simple models for antenna apertures that have been proposed for future instruments such as the Hydrogen Epoch of Reionization Array and the Square Kilometre Array indicate they should suppress foreground leakage from the pitchfork by ∼40 dB relative to the MWA and significantly increase the likelihood of cosmological signal detection in these critical Fourier modes in the three-dimensional power spectrum.},
	Author = {Nithyanandan Thyagarajan and Daniel C. Jacobs and Judd D. Bowman and N. Barry and A. P. Beardsley and G. Bernardi and F. Briggs and R. J. Cappallo and P. Carroll and A. A. Deshpande and A. de Oliveira-Costa and Joshua S. Dillon and A. Ewall-Wice and L. Feng and L. J. Greenhill and B. J. Hazelton and L. Hernquist and J. N. Hewitt and N. Hurley-Walker and M. Johnston-Hollitt and D. L. Kaplan and Han-Seek Kim and P. Kittiwisit and E. Lenc and J. Line and A. Loeb and C. J. Lonsdale and B. McKinley and S. R. McWhirter and D. A. Mitchell and M. F. Morales and E. Morgan and A. R. Neben and D. Oberoi and A. R. Offringa and S. M. Ord and Sourabh Paul and B. Pindor and J. C. Pober and T. Prabu and P. Procopio and J. Riding and N. Udaya Shankar and Shiv K. Sethi and K. S. Srivani and R. Subrahmanyan and I. S. Sullivan and M. Tegmark and S. J. Tingay and C. M. Trott and R. B. Wayth and R. L. Webster and A. Williams and C. L. Williams and J. S. B. Wyithe},
	Date-Added = {2015-08-25 15:33:29 +0000},
	Date-Modified = {2015-08-25 15:33:36 +0000},
	Journal = {The Astrophysical Journal Letters},
	Number = {2},
	Pages = {L28},
	Title = {Confirmation of Wide-field Signatures in Redshifted 21 cm Power Spectra},
	Url = {http://stacks.iop.org/2041-8205/807/i=2/a=L28},
	Volume = {807},
	Year = {2015},
	Bdsk-Url-1 = {http://stacks.iop.org/2041-8205/807/i=2/a=L28}}

@article{Offringa:2015,
	Abstract = { ABSTRACT The Murchison Widefield Array is a new low-frequency interferometric radio telescope built in Western Australia at one of the locations of the future Square Kilometre Array. We describe the automated radio-frequency interference detection strategy implemented for the Murchison Widefield Array, which is based on the aoflagger platform, and present 72--231 MHz radio-frequency interference statistics from 10 observing nights. Radio-frequency interference detection removes 1.1% of the data. Radio-frequency interference from digital TV is observed 3% of the time due to occasional ionospheric or atmospheric propagation. After radio-frequency interference detection and excision, almost all data can be calibrated and imaged without further radio-frequency interference mitigation efforts, including observations within the FM and digital TV bands. The results are compared to a previously published Low-Frequency Array radio-frequency interference survey. The remote location of the Murchison Widefield Array results in a substantially cleaner radio-frequency interference environment compared to Low-Frequency Array's radio environment, but adequate detection of radio-frequency interference is still required before data can be analysed. We include specific recommendations designed to make the Square Kilometre Array more robust to radio-frequency interference, including: the availability of sufficient computing power for radio-frequency interference detection; accounting for radio-frequency interference in the receiver design; a smooth band-pass response; and the capability of radio-frequency interference detection at high time and frequency resolution (second and kHz-scale respectively). },
	Author = {Offringa,A. R. and Wayth,R. B. and Hurley-Walker,N. and Kaplan,D. L. and Barry,N. and Beardsley,A. P. and Bell,M. E. and Bernardi,G. and Bowman,J. D. and Briggs,F. and Callingham,J. R. and Cappallo,R. J. and Carroll,P. and Deshpande,A. A. and Dillon,J. S. and Dwarakanath,K. S. and Ewall-Wice,A. and Feng,L. and For,B.-Q. and Gaensler,B. M. and Greenhill,L. J. and Hancock,P. and Hazelton,B. J. and Hewitt,J. N. and Hindson,L. and Jacobs,D. C. and Johnston-Hollitt,M. and Kapi{\'n}ska,A. D. and Kim,H.-S. and Kittiwisit,P. and Lenc,E. and Line,J. and Loeb,A. and Lonsdale,C. J. and McKinley,B. and McWhirter,S. R. and Mitchell,D. A. and Morales,M. F. and Morgan,E. and Morgan,J. and Neben,A. R. and Oberoi,D. and Ord,S. M. and Paul,S. and Pindor,B. and Pober,J. C. and Prabu,T. and Procopio,P. and Riding,J. and Udaya Shankar,N. and Sethi,S. and Srivani,K. S. and Staveley-Smith,L. and Subrahmanyan,R. and Sullivan,I. S. and Tegmark,M. and Thyagarajan,N. and Tingay,S. J. and Trott,C. M. and Webster,R. L. and Williams,A. and Williams,C. L. and Wu,C. and Wyithe,J. S. and Zheng,Q.},
	Date-Added = {2015-08-11 17:47:50 +0000},
	Date-Modified = {2015-08-11 17:47:56 +0000},
	Doi = {10.1017/pasa.2015.7},
	Issn = {1448-6083},
	Journal = {PASA - Publications of the Astronomical Society of Australia},
	Title = {The Low-Frequency Environment of the Murchison Widefield Array: Radio-Frequency Interference Analysis and Mitigation},
	Url = {http://journals.cambridge.org/article_S1323358015000077},
	Volume = {32},
	Year = {2015},
	Bdsk-Url-1 = {http://journals.cambridge.org/article_S1323358015000077},
	Bdsk-Url-2 = {http://dx.doi.org/10.1017/pasa.2015.7}}

@article{Dillon:2015,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2015PhRvD..91l3011D},
	Archiveprefix = {arXiv},
	Author = {{Dillon}, J.~S. and {Neben}, A.~R. and {Hewitt}, J.~N. and {Tegmark}, M. and {Barry}, N. and {Beardsley}, A.~P. and {Bowman}, J.~D. and {Briggs}, F. and {Carroll}, P. and {de Oliveira-Costa}, A. and {Ewall-Wice}, A. and {Feng}, L. and {Greenhill}, L.~J. and {Hazelton}, B.~J. and {Hernquist}, L. and {Hurley-Walker}, N. and {Jacobs}, D.~C. and {Kim}, H.~S. and {Kittiwisit}, P. and {Lenc}, E. and {Line}, J. and {Loeb}, A. and {McKinley}, B. and {Mitchell}, D.~A. and {Morales}, M.~F. and {Offringa}, A.~R. and {Paul}, S. and {Pindor}, B. and {Pober}, J.~C. and {Procopio}, P. and {Riding}, J. and {Sethi}, S. and {Shankar}, N.~U. and {Subrahmanyan}, R. and {Sullivan}, I. and {Thyagarajan}, N. and {Tingay}, S.~J. and {Trott}, C. and {Wayth}, R.~B. and {Webster}, R.~L. and {Wyithe}, S. and {Bernardi}, G. and {Cappallo}, R.~J. and {Deshpande}, A.~A. and {Johnston-Hollitt}, M. and {Kaplan}, D.~L. and {Lonsdale}, C.~J. and {McWhirter}, S.~R. and {Morgan}, E. and {Oberoi}, D. and {Ord}, S.~M. and {Prabu}, T. and {Srivani}, K.~S. and {Williams}, A. and {Williams}, C.~L.},
	Date-Added = {2015-08-03 17:06:52 +0000},
	Date-Modified = {2015-08-03 17:06:58 +0000},
	Doi = {10.1103/PhysRevD.91.123011},
	Eid = {123011},
	Eprint = {1506.01026},
	Journal = {\prd},
	Keywords = {Observation and data reduction techniques, computer modeling and simulation, Interferometry, Cosmology, Observational cosmology},
	Month = jun,
	Number = 12,
	Pages = {123011},
	Title = {{Empirical covariance modeling for 21 cm power spectrum estimation: A method demonstration and new limits from early Murchison Widefield Array 128-tile data}},
	Volume = 91,
	Year = 2015,
	Bdsk-Url-1 = {http://dx.doi.org/10.1103/PhysRevD.91.123011}}

@article{Planck:2015b,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2015arXiv150702704P},
	Archiveprefix = {arXiv},
	Author = {{Planck Collaboration} and {Aghanim}, N. and {Arnaud}, M. and {Ashdown}, M. and {Aumont}, J. and {Baccigalupi}, C. and {Banday}, A.~J. and {Barreiro}, R.~B. and {Bartlett}, J.~G. and {Bartolo}, N. and et al.},
	Date-Added = {2015-07-29 17:31:40 +0000},
	Date-Modified = {2016-06-03 20:33:38 +0000},
	Eprint = {1507.02704},
	Journal = {{ArXiv e-prints, arXiv:1507.02704}},
	Keywords = {Astrophysics - Cosmology and Nongalactic Astrophysics},
	Month = jul,
	Title = {{Planck 2015 results. XI. CMB power spectra, likelihoods, and robustness of parameters}},
	Year = 2015}

@article{Shaw:2014,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2014ApJ...781...57S},
	Archiveprefix = {arXiv},
	Author = {{Shaw}, J.~R. and {Sigurdson}, K. and {Pen}, U.-L. and {Stebbins}, A. and {Sitwell}, M.},
	Date-Added = {2015-03-27 18:12:36 +0000},
	Date-Modified = {2015-03-27 18:12:42 +0000},
	Doi = {10.1088/0004-637X/781/2/57},
	Eid = {57},
	Eprint = {1302.0327},
	Journal = {\apj},
	Keywords = {cosmology: observations, dark energy, large-scale structure of universe, methods: data analysis, radio continuum: general},
	Month = feb,
	Pages = {57},
	Primaryclass = {astro-ph.CO},
	Title = {{All-sky Interferometry with Spherical Harmonic Transit Telescopes}},
	Volume = 781,
	Year = 2014,
	Bdsk-Url-1 = {http://dx.doi.org/10.1088/0004-637X/781/2/57}}

@article{Greenhill:2012,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2012arXiv1201.1700G},
	Archiveprefix = {arXiv},
	Author = {{Greenhill}, L.~J. and {Bernardi}, G.},
	Date-Added = {2015-03-27 16:52:11 +0000},
	Date-Modified = {2015-03-27 16:52:17 +0000},
	Eprint = {1201.1700},
	Journal = {ArXiv e-prints},
	Keywords = {Astrophysics - Cosmology and Extragalactic Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics},
	Month = jan,
	Primaryclass = {astro-ph.CO},
	Title = {{HI Epoch of Reionization Arrays}},
	Year = 2012}

@article{Bowman:2010,
	Annote = {10.1038/nature09601},
	Author = {Bowman, Judd D. and Rogers, Alan E. E.},
	Date = {2010/12/09/print},
	Date-Added = {2015-03-27 16:48:57 +0000},
	Date-Modified = {2015-03-27 16:49:03 +0000},
	Day = {09},
	Isbn = {0028-0836},
	Journal = {Nature},
	L3 = {http://www.nature.com/nature/journal/v468/n7325/abs/nature09601.html#supplementary-information},
	M3 = {10.1038/nature09601},
	Month = {12},
	Number = {7325},
	Pages = {796--798},
	Publisher = {Nature Publishing Group, a division of Macmillan Publishers Limited. All Rights Reserved.},
	Title = {A lower limit of {$[$}Dgr{$]$}z{$[$}thinsp{$]$}>{$[$}thinsp{$]$}0.06 for the duration of the reionization epoch},
	Ty = {JOUR},
	Url = {http://dx.doi.org/10.1038/nature09601},
	Volume = {468},
	Year = {2010},
	Bdsk-Url-1 = {http://dx.doi.org/10.1038/nature09601}}

@article{Burns:2012,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2012AdSpR..49..433B},
	Archiveprefix = {arXiv},
	Author = {{Burns}, J.~O. and {Lazio}, J. and {Bale}, S. and {Bowman}, J. and {Bradley}, R. and {Carilli}, C. and {Furlanetto}, S. and {Harker}, G. and {Loeb}, A. and {Pritchard}, J.},
	Date-Added = {2015-03-27 16:48:36 +0000},
	Date-Modified = {2015-03-27 16:48:42 +0000},
	Doi = {10.1016/j.asr.2011.10.014},
	Eprint = {1106.5194},
	Journal = {Advances in Space Research},
	Month = feb,
	Pages = {433-450},
	Primaryclass = {astro-ph.CO},
	Title = {{Probing the first stars and black holes in the early Universe with the Dark Ages Radio Explorer (DARE)}},
	Volume = 49,
	Year = 2012,
	Bdsk-Url-1 = {http://dx.doi.org/10.1016/j.asr.2011.10.014}}

@article{Liu:2010,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2010MNRAS.408.1029L},
	Archiveprefix = {arXiv},
	Author = {{Liu}, A. and {Tegmark}, M. and {Morrison}, S. and {Lutomirski}, A. and {Zaldarriaga}, M.},
	Date-Added = {2015-03-27 15:17:53 +0000},
	Date-Modified = {2015-03-27 15:17:57 +0000},
	Doi = {10.1111/j.1365-2966.2010.17174.x},
	Eprint = {1001.5268},
	Journal = {\mnras},
	Keywords = {instrumentation: interferometers, methods: data analysis, cosmology: observations, radio continuum: general},
	Month = oct,
	Pages = {1029-1050},
	Primaryclass = {astro-ph.IM},
	Title = {{Precision calibration of radio interferometers using redundant baselines}},
	Volume = 408,
	Year = 2010,
	Bdsk-Url-1 = {http://dx.doi.org/10.1111/j.1365-2966.2010.17174.x}}

@article{Jacobs:2015,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2015ApJ...801...51J},
	Archiveprefix = {arXiv},
	Author = {{Jacobs}, D.~C. and {Pober}, J.~C. and {Parsons}, A.~R. and {Aguirre}, J.~E. and {Ali}, Z.~S. and {Bowman}, J. and {Bradley}, R.~F. and {Carilli}, C.~L. and {DeBoer}, D.~R. and {Dexter}, M.~R. and {Gugliucci}, N.~E. and {Klima}, P. and {Liu}, A. and {MacMahon}, D.~H.~E. and {Manley}, J.~R. and {Moore}, D.~F. and {Stefan}, I.~I. and {Walbrugh}, W.~P.},
	Date-Added = {2015-03-25 19:00:53 +0000},
	Date-Modified = {2015-03-25 19:01:00 +0000},
	Doi = {10.1088/0004-637X/801/1/51},
	Eid = {51},
	Eprint = {1408.3389},
	Journal = {\apj},
	Keywords = {dark ages, reionization, first stars, techniques: interferometric},
	Month = mar,
	Pages = {51},
	Title = {{Multiredshift Limits on the 21 cm Power Spectrum from PAPER}},
	Volume = 801,
	Year = 2015,
	Bdsk-Url-1 = {http://dx.doi.org/10.1088/0004-637X/801/1/51}}

@article{Parsons:2014,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2014ApJ...788..106P},
	Archiveprefix = {arXiv},
	Author = {{Parsons}, A.~R. and {Liu}, A. and {Aguirre}, J.~E. and {Ali}, Z.~S. and {Bradley}, R.~F. and {Carilli}, C.~L. and {DeBoer}, D.~R. and {Dexter}, M.~R. and {Gugliucci}, N.~E. and {Jacobs}, D.~C. and {Klima}, P. and {MacMahon}, D.~H.~E. and {Manley}, J.~R. and {Moore}, D.~F. and {Pober}, J.~C. and {Stefan}, I.~I. and {Walbrugh}, W.~P.},
	Date-Added = {2015-03-25 18:59:06 +0000},
	Date-Modified = {2015-03-25 18:59:12 +0000},
	Doi = {10.1088/0004-637X/788/2/106},
	Eid = {106},
	Eprint = {1304.4991},
	Journal = {\apj},
	Keywords = {cosmology: observations, dark ages, reionization, first stars, early universe, instrumentation: interferometers, intergalactic medium, radio continuum: general},
	Month = jun,
	Pages = {106},
	Title = {{New Limits on 21 cm Epoch of Reionization from PAPER-32 Consistent with an X-Ray Heated Intergalactic Medium at z = 7.7}},
	Volume = 788,
	Year = 2014,
	Bdsk-Url-1 = {http://dx.doi.org/10.1088/0004-637X/788/2/106}}

@article{Dillon:2014,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2014PhRvD..89b3002D},
	Archiveprefix = {arXiv},
	Author = {{Dillon}, J.~S. and {Liu}, A. and {Williams}, C.~L. and {Hewitt}, J.~N. and {Tegmark}, M. and {Morgan}, E.~H. and {Levine}, A.~M. and {Morales}, M.~F. and {Tingay}, S.~J. and {Bernardi}, G. and {Bowman}, J.~D. and {Briggs}, F.~H. and {Cappallo}, R.~C. and {Emrich}, D. and {Mitchell}, D.~A. and {Oberoi}, D. and {Prabu}, T. and {Wayth}, R. and {Webster}, R.~L.},
	Date-Added = {2015-03-25 18:57:23 +0000},
	Date-Modified = {2015-03-25 18:57:32 +0000},
	Doi = {10.1103/PhysRevD.89.023002},
	Eid = {023002},
	Eprint = {1304.4229},
	Journal = {\prd},
	Keywords = {Observation and data reduction techniques, computer modeling and simulation, Radio microwave, Cosmology, Observational cosmology},
	Month = jan,
	Number = 2,
	Pages = {023002},
	Primaryclass = {astro-ph.CO},
	Title = {{Overcoming real-world obstacles in 21 cm power spectrum estimation: A method demonstration and results from early Murchison Widefield Array data}},
	Volume = 89,
	Year = 2014,
	Bdsk-Url-1 = {http://dx.doi.org/10.1103/PhysRevD.89.023002}}

@article{Large:1981,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/1981MNRAS.194..693L},
	Author = {{Large}, M.~I. and {Mills}, B.~Y. and {Little}, A.~G. and {Crawford}, D.~F. and {Sutton}, J.~M.},
	Date-Added = {2015-03-18 14:13:09 +0000},
	Date-Modified = {2015-03-18 14:13:19 +0000},
	Journal = {\mnras},
	Month = feb,
	Pages = {693},
	Title = {{The Molonglo Reference Catalogue of Radio Sources}},
	Volume = 194,
	Year = 1981}

@article{deOliveira-Costa:2008,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2008MNRAS.388..247D},
	Archiveprefix = {arXiv},
	Author = {{de Oliveira-Costa}, A. and {Tegmark}, M. and {Gaensler}, B.~M. and {Jonas}, J. and {Landecker}, T.~L. and {Reich}, P.},
	Date-Added = {2015-03-16 15:01:49 +0000},
	Date-Modified = {2015-03-16 15:02:09 +0000},
	Doi = {10.1111/j.1365-2966.2008.13376.x},
	Eprint = {0802.1525},
	Journal = {\mnras},
	Keywords = {methods: data analysis , astronomical data bases: miscellaneous , ISM: structure , diffuse radiation , radio continuum: ISM},
	Month = jul,
	Pages = {247-260},
	Title = {{A model of diffuse Galactic radio emission from 10 MHz to 100 GHz}},
	Volume = 388,
	Year = 2008,
	Bdsk-Url-1 = {http://dx.doi.org/10.1111/j.1365-2966.2008.13376.x}}

@article{Slee:1977,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/1977AuJPA..43....1S},
	Author = {{Slee}, O.~B.},
	Date-Added = {2015-03-16 14:48:23 +0000},
	Date-Modified = {2015-03-16 14:48:31 +0000},
	Journal = {Australian Journal of Physics Astrophysical Supplement},
	Keywords = {Astronomical Maps, Radio Sources (Astronomy), Tables (Data), Very High Frequencies, Astronomical Catalogs, Astronomical Observatories, Spectroheliographs},
	Month = nov,
	Pages = {1-123},
	Title = {{Culgoora-3 list of radio source measurements}},
	Volume = 43,
	Year = 1977}

@article{Scargle:1982,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/1982ApJ...263..835S},
	Author = {{Scargle}, J.~D.},
	Date-Added = {2015-03-09 14:04:19 +0000},
	Date-Modified = {2015-03-09 14:04:29 +0000},
	Doi = {10.1086/160554},
	Journal = {\apj},
	Keywords = {Astronomy, Signal Detection, Spectrum Analysis, Statistical Distributions, Time Series Analysis, Fourier Transformation, Frequency Response, Power Spectra, Signal To Noise Ratios},
	Month = dec,
	Pages = {835-853},
	Title = {{Studies in astronomical time series analysis. II - Statistical aspects of spectral analysis of unevenly spaced data}},
	Volume = 263,
	Year = 1982,
	Bdsk-Url-1 = {http://dx.doi.org/10.1086/160554}}

@article{Gorski:2005,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2005ApJ...622..759G},
	Author = {{G{\'o}rski}, K.~M. and {Hivon}, E. and {Banday}, A.~J. and {Wandelt}, B.~D. and {Hansen}, F.~K. and {Reinecke}, M. and {Bartelmann}, M.},
	Date-Added = {2015-02-27 15:08:13 +0000},
	Date-Modified = {2015-02-27 15:08:21 +0000},
	Doi = {10.1086/427976},
	Eprint = {astro-ph/0409513},
	Journal = {\apj},
	Keywords = {Cosmology: Cosmic Microwave Background, Cosmology: Observations, Methods: Statistical},
	Month = apr,
	Pages = {759-771},
	Title = {{HEALPix: A Framework for High-Resolution Discretization and Fast Analysis of Data Distributed on the Sphere}},
	Volume = 622,
	Year = 2005,
	Bdsk-Url-1 = {http://dx.doi.org/10.1086/427976}}

@article{Cornwell:2008,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2008ISTSP...2..647C},
	Archiveprefix = {arXiv},
	Author = {{Cornwell}, T.~J. and {Golap}, K. and {Bhatnagar}, S.},
	Date-Added = {2015-02-27 14:43:14 +0000},
	Date-Modified = {2015-02-27 14:43:21 +0000},
	Doi = {10.1109/JSTSP.2008.2005290},
	Eprint = {0807.4161},
	Journal = {IEEE Journal of Selected Topics in Signal Processing},
	Month = nov,
	Pages = {647-657},
	Title = {{The Noncoplanar Baselines Effect in Radio Interferometry: The W-Projection Algorithm}},
	Volume = 2,
	Year = 2008,
	Bdsk-Url-1 = {http://dx.doi.org/10.1109/JSTSP.2008.2005290}}

@article{Sutinjo:2015,
	Author = {Sutinjo, A. and O'Sullivan, J. and Lenc, E. and Wayth, R. B. and Padhi, S. and Hall, P. and Tingay, S. J.},
	Date-Added = {2015-02-25 14:48:51 +0000},
	Date-Modified = {2015-02-25 14:48:59 +0000},
	Doi = {10.1002/2014RS005517},
	Issn = {1944-799X},
	Journal = {Radio Science},
	Keywords = {polarimetry, antenna arrays, radio astronomy, antennas},
	Number = {1},
	Pages = {52--65},
	Title = {Understanding instrumental Stokes leakage in Murchison Widefield Array polarimetry},
	Url = {http://dx.doi.org/10.1002/2014RS005517},
	Volume = {50},
	Year = {2015},
	Bdsk-Url-1 = {http://dx.doi.org/10.1002/2014RS005517}}

@article{Prabu:2015,
	Author = {Prabu, Thiagaraj and Srivani, K.S. and Roshi, D.Anish and Kamini, P.A. and Madhavi, S. and Emrich, David and Crosse, Brian and Williams, AndrewJ. and Waterson, Mark and Deshpande, AvinashA. and Shankar, N.Udaya and Subrahmanyan, Ravi and Briggs, FrankH. and Goeke, RobertF. and Tingay, StevenJ. and Johnston-Hollitt, Melanie and R, GopalakrishnaM and Morgan, EdwardH. and Pathikulangara, Joseph and Bunton, JohnD. and Hampson, Grant and Williams, Christopher and Ord, StephenM. and Wayth, RandallB. and Kumar, Deepak and Morales, MiguelF. and deSouza, Ludi and Kratzenberg, Eric and Pallot, D. and McWhirter, Russell and Hazelton, BrynaJ. and Arcus, Wayne and Barnes, DavidG. and Bernardi, Gianni and Booler, T. and Bowman, JuddD. and Cappallo, RogerJ. and Corey, BrianE. and Greenhill, LincolnJ. and Herne, David and Hewitt, JacquelineN. and Kaplan, DavidL. and Kasper, JustinC. and Kincaid, BartonB. and Koenig, Ronald and Lonsdale, ColinJ. and Lynch, MervynJ. and Mitchell, DanielA. and Oberoi, Divya and Remillard, RonaldA. and Rogers, AlanE. and Salah, JosephE. and Sault, RobertJ. and Stevens, JamieB. and Tremblay, S. and Webster, RachelL. and Whitney, AlanR. and Wyithe, StuartB.},
	Date-Added = {2015-02-25 14:17:38 +0000},
	Date-Modified = {2015-02-25 14:17:38 +0000},
	Doi = {10.1007/s10686-015-9444-3},
	Issn = {0922-6435},
	Journal = {Experimental Astronomy},
	Keywords = {ADC; Channelizer; Digital-receiver; FPGA; MWA; MRO; PFB; Radio astronomy instrumentation; Radio telescope; SKA},
	Language = {English},
	Pages = {1-21},
	Publisher = {Springer Netherlands},
	Title = {A digital-receiver for the MurchisonWidefield Array},
	Url = {http://dx.doi.org/10.1007/s10686-015-9444-3},
	Year = {2015},
	Bdsk-Url-1 = {http://dx.doi.org/10.1007/s10686-015-9444-3}}

@article{Hurley-Walker:2014,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2014PASA...31...45H},
	Archiveprefix = {arXiv},
	Author = {{Hurley-Walker}, N. and {Morgan}, J. and {Wayth}, R.~B. and {Hancock}, P.~J. and {Bell}, M.~E. and {Bernardi}, G. and {Bhat}, R. and {Briggs}, F. and {Deshpande}, A.~A. and {Ewall-Wice}, A. and {Feng}, L. and {Hazelton}, B.~J. and {Hindson}, L. and {Jacobs}, D.~C. and {Kaplan}, D.~L. and {Kudryavtseva}, N. and {Lenc}, E. and {McKinley}, B. and {Mitchell}, D. and {Pindor}, B. and {Procopio}, P. and {Oberoi}, D. and {Offringa}, A. and {Ord}, S. and {Riding}, J. and {Bowman}, J.~D. and {Cappallo}, R. and {Corey}, B. and {Emrich}, D. and {Gaensler}, B.~M. and {Goeke}, R. and {Greenhill}, L. and {Hewitt}, J. and {Johnston-Hollitt}, M. and {Kasper}, J. and {Kratzenberg}, E. and {Lonsdale}, C. and {Lynch}, M. and {McWhirter}, R. and {Morales}, M.~F. and {Morgan}, E. and {Prabu}, T. and {Rogers}, A. and {Roshi}, A. and {Shankar}, U. and {Srivani}, K. and {Subrahmanyan}, R. and {Tingay}, S. and {Waterson}, M. and {Webster}, R. and {Whitney}, A. and {Williams}, A. and {Williams}, C.},
	Date-Added = {2015-02-25 13:18:07 +0000},
	Date-Modified = {2016-03-10 20:59:01 +0000},
	Doi = {10.1017/pasa.2014.40},
	Eid = {e045},
	Eprint = {1410.0790},
	Journal = {PASA - Publications of the Astronomical Society of Australia},
	Keywords = {radio continuum: general, surveys, techniques: interferometric},
	Month = nov,
	Pages = {45},
	Primaryclass = {astro-ph.IM},
	Title = {{The Murchison Widefield Array Commissioning Survey: A Low-Frequency Catalogue of 14 110 Compact Radio Sources over 6 100 Square Degrees}},
	Volume = 31,
	Year = 2014,
	Bdsk-Url-1 = {http://dx.doi.org/10.1017/pasa.2014.40}}

@article{Salvini:2014,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2014A%26A...571A..97S},
	Archiveprefix = {arXiv},
	Author = {{Salvini}, S. and {Wijnholds}, S.~J.},
	Date-Added = {2015-02-24 20:58:41 +0000},
	Date-Modified = {2015-02-24 20:58:52 +0000},
	Doi = {10.1051/0004-6361/201424487},
	Eid = {A97},
	Eprint = {1410.2101},
	Journal = {\aap},
	Keywords = {instrumentation: interferometers, methods: numerical, methods: statistical, techniques: interferometric},
	Month = nov,
	Pages = {A97},
	Primaryclass = {astro-ph.IM},
	Title = {{Fast gain calibration in radio astronomy using alternating direction implicit methods: Analysis and applications}},
	Volume = 571,
	Year = 2014,
	Bdsk-Url-1 = {http://dx.doi.org/10.1051/0004-6361/201424487}}

@article{Wells:1981,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/1981A%26AS...44..363W},
	Author = {{Wells}, D.~C. and {Greisen}, E.~W. and {Harten}, R.~H.},
	Date-Added = {2015-02-24 17:50:43 +0000},
	Date-Modified = {2015-02-24 17:50:51 +0000},
	Journal = {\aaps},
	Month = jun,
	Pages = {363},
	Title = {{FITS - a Flexible Image Transport System}},
	Volume = 44,
	Year = 1981}

@techreport{Greisen:2012,
	Author = {{Greisen}, E.W.},
	Date-Added = {2015-02-24 17:45:52 +0000},
	Date-Modified = {2015-02-24 17:50:29 +0000},
	Number = {117},
	Title = {{AIPS FITS File Format}},
	Type = {AIPS Memo},
	Year = {2012}}

@article{Trott:2014,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2014PASA...31...26T},
	Archiveprefix = {arXiv},
	Author = {{Trott}, C.~M.},
	Date-Added = {2015-02-23 15:37:53 +0000},
	Date-Modified = {2016-03-10 20:59:24 +0000},
	Doi = {10.1017/pasa.2014.23},
	Eid = {e026},
	Eprint = {1405.0357},
	Journal = {PASA - Publications of the Astronomical Society of Australia},
	Keywords = {methods: analytical, methods: statistical, early universe, instrumentation: interferometers},
	Month = jul,
	Pages = {26},
	Title = {{Comparison of Observing Modes for Statistical Estimation of the 21 cm Signal from the Epoch of Reionisation}},
	Volume = 31,
	Year = 2014,
	Bdsk-Url-1 = {http://dx.doi.org/10.1017/pasa.2014.23}}

@article{Ord:2009,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2009arXiv0902.0915O},
	Archiveprefix = {arXiv},
	Author = {{Ord}, S. and {Greenhill}, L. and {Wayth}, R. and {Mitchell}, D. and {Dale}, K. and {Pfister}, H. and {Edgar}, R.~G.},
	Date-Added = {2015-02-23 15:19:15 +0000},
	Date-Modified = {2015-02-23 15:19:22 +0000},
	Eprint = {0902.0915},
	Journal = {ArXiv e-prints},
	Keywords = {Astrophysics - Instrumentation and Methods for Astrophysics},
	Month = feb,
	Primaryclass = {astro-ph.IM},
	Title = {{GPUs for data processing in the MWA}},
	Year = 2009}

@article{Wayth:2009,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2009PASP..121..857W},
	Archiveprefix = {arXiv},
	Author = {{Wayth}, R.~B. and {Greenhill}, L.~J. and {Briggs}, F.~H.},
	Date-Added = {2015-02-23 15:18:11 +0000},
	Date-Modified = {2015-02-23 15:18:17 +0000},
	Doi = {10.1086/605334},
	Eprint = {0906.1887},
	Journal = {\pasp},
	Keywords = {Astronomical Instrumentation},
	Month = aug,
	Pages = {857-865},
	Primaryclass = {astro-ph.IM},
	Title = {{A GPU-based Real-time Software Correlation System for the Murchison Widefield Array Prototype}},
	Volume = 121,
	Year = 2009,
	Bdsk-Url-1 = {http://dx.doi.org/10.1086/605334}}

@article{Beardsley:2015,
	Abstract = {Infrared and radio observations of the Epoch of Reionization promise to revolutionize our understanding of the cosmic dawn, and major efforts with the JWST , MWA, and HERA are underway. While measurements of the ionizing sources with infrared telescopes and the effect of these sources on the intergalactic medium with radio telescopes should be complementary, to date the wildly disparate angular resolutions and survey speeds have made connecting proposed observations difficult. In this paper we develop a method to bridge the gap between radio and infrared studies. While the radio images may not have the sensitivity and resolution to identify individual bubbles with high fidelity, by leveraging knowledge of the measured power spectrum we are able to separate regions that are likely ionized from largely neutral, providing context for the JWST observations of galaxy counts and properties in each. By providing the ionization context for infrared galaxy observations, this method can significantly enhance the science returns of JWST and other infrared observations.},
	Author = {A. P. Beardsley and M. F. Morales and A. Lidz and M. Malloy and P. M. Sutter},
	Date-Added = {2015-02-20 16:44:05 +0000},
	Date-Modified = {2015-02-20 16:44:18 +0000},
	Journal = {The Astrophysical Journal},
	Number = {2},
	Pages = {128},
	Title = {Adding Context to James Webb Space Telescope Surveys with Current and Future 21 cm Radio Observations},
	Url = {http://stacks.iop.org/0004-637X/800/i=2/a=128},
	Volume = {800},
	Year = {2015},
	Bdsk-Url-1 = {http://stacks.iop.org/0004-637X/800/i=2/a=128}}

@book{jackson1999classical,
	Author = {Jackson, J.D.},
	Date-Added = {2015-02-19 16:21:31 +0000},
	Date-Modified = {2015-02-19 16:21:31 +0000},
	Isbn = {9780471309321},
	Lccn = {97046873},
	Publisher = {Wiley},
	Title = {Classical electrodynamics},
	Url = {http://books.google.com/books?id=U3LBQgAACAAJ},
	Year = {1999},
	Bdsk-Url-1 = {http://books.google.com/books?id=U3LBQgAACAAJ}}

@techreport{Lal:2009,
	Author = {{Lal}, D.V. and {Lobanov}, A.P. and {Jim{\'e}nez-Monferrer}, S.},
	Date-Added = {2015-02-19 16:04:29 +0000},
	Date-Modified = {2015-02-19 16:06:47 +0000},
	Number = {107},
	Title = {Array configuration studies for the Square Kilometre Array - Implementation of figures of merit based on spatial dynamic range},
	Type = {SKA Memo},
	Year = {2009}}

@techreport{Kogan:2005,
	Author = {{Kogan}, L. and {Cohen}, A.},
	Date-Added = {2015-02-19 15:58:20 +0000},
	Date-Modified = {2015-02-19 16:02:06 +0000},
	Number = {21},
	Title = {Optimization of the LWA antenna station configuration minimizing side lobes},
	Type = {LWA Memo},
	Year = {2005}}

@inproceedings{Thompson:1999,
	Author = {Thompson, A. Richard},
	Booktitle = {Synthesis Imaging in Radio Astronomy II},
	Date-Added = {2015-02-17 15:47:10 +0000},
	Date-Modified = {2015-02-17 15:52:00 +0000},
	Pages = {11},
	Title = {Fundamentals of Radio Interferometry},
	Volume = {180},
	Year = {1999}}

@article{Parsons:2009,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2009AJ....138..219P},
	Archiveprefix = {arXiv},
	Author = {{Parsons}, A.~R. and {Backer}, D.~C.},
	Date-Added = {2015-02-16 16:02:09 +0000},
	Date-Modified = {2015-02-18 17:35:51 +0000},
	Doi = {10.1088/0004-6256/138/1/219},
	Eprint = {0901.2575},
	Journal = {\aj},
	Keywords = {instrumentation: interferometers, methods: data analysis, techniques: interferometric},
	Month = jul,
	Pages = {219-226},
	Primaryclass = {astro-ph.IM},
	Title = {{Calibration of Low-Frequency, Wide-Field Radio Interferometers Using Delay/Delay-Rate Filtering}},
	Volume = 138,
	Year = 2009,
	Bdsk-Url-1 = {http://dx.doi.org/10.1088/0004-6256/138/1/219}}

@article{Bouwens:2014,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2014ApJ...795..126B},
	Archiveprefix = {arXiv},
	Author = {{Bouwens}, R.~J. and {Bradley}, L. and {Zitrin}, A. and {Coe}, D. and {Franx}, M. and {Zheng}, W. and {Smit}, R. and {Host}, O. and {Postman}, M. and {Moustakas}, L. and {Labb{\'e}}, I. and {Carrasco}, M. and {Molino}, A. and {Donahue}, M. and {Kelson}, D.~D. and {Meneghetti}, M. and {Ben{\'{\i}}tez}, N. and {Lemze}, D. and {Umetsu}, K. and {Broadhurst}, T. and {Moustakas}, J. and {Rosati}, P. and {Jouvel}, S. and {Bartelmann}, M. and {Ford}, H. and {Graves}, G. and {Grillo}, C. and {Infante}, L. and {Jimenez-Teja}, Y. and {Lahav}, O. and {Maoz}, D. and {Medezinski}, E. and {Melchior}, P. and {Merten}, J. and {Nonino}, M. and {Ogaz}, S. and {Seitz}, S.},
	Date-Added = {2015-02-10 21:45:30 +0000},
	Date-Modified = {2015-02-10 21:45:38 +0000},
	Doi = {10.1088/0004-637X/795/2/126},
	Eid = {126},
	Eprint = {1211.2230},
	Journal = {\apj},
	Keywords = {galaxies: evolution, galaxies: high-redshift},
	Month = nov,
	Pages = {126},
	Title = {{A Census of Star-forming Galaxies in the Z \~{} 9-10 Universe based on HST+Spitzer Observations over 19 Clash Clusters: Three Candidate Z \~{} 9-10 Galaxies and Improved Constraints on the Star Formation Rate Density at Z \~{} 9.2}},
	Volume = 795,
	Year = 2014,
	Bdsk-Url-1 = {http://dx.doi.org/10.1088/0004-637X/795/2/126}}

@article{Santos:2008,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2008ApJ...689....1S},
	Archiveprefix = {arXiv},
	Author = {{Santos}, M.~G. and {Amblard}, A. and {Pritchard}, J. and {Trac}, H. and {Cen}, R. and {Cooray}, A.},
	Date-Added = {2015-02-09 16:41:13 +0000},
	Date-Modified = {2015-02-09 16:41:22 +0000},
	Doi = {10.1086/592487},
	Eprint = {0708.2424},
	Journal = {\apj},
	Keywords = {Cosmology: Theory, Cosmology: Diffuse Radiation, Cosmology: Large-Scale Structure of Universe},
	Month = dec,
	Pages = {1-16},
	Title = {{Cosmic Reionization and the 21 cm Signal: Comparison between an Analytical Model and a Simulation}},
	Volume = 689,
	Year = 2008,
	Bdsk-Url-1 = {http://dx.doi.org/10.1086/592487}}

@article{Choudhury:2014,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2014arXiv1412.4790C},
	Archiveprefix = {arXiv},
	Author = {{Choudhury}, T.~R. and {Puchwein}, E. and {Haehnelt}, M.~G. and {Bolton}, J.~S.},
	Date-Added = {2015-02-09 14:43:01 +0000},
	Date-Modified = {2015-02-09 14:43:11 +0000},
	Eprint = {1412.4790},
	Journal = {ArXiv e-prints},
	Keywords = {Astrophysics - Cosmology and Nongalactic Astrophysics},
	Month = dec,
	Title = {{Lyman-\$$\backslash$alpha\$ emitters gone missing: evidence for late reionization?}},
	Year = 2014}

@article{Gunn:1965,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/1965ApJ...142.1633G},
	Author = {{Gunn}, J.~E. and {Peterson}, B.~A.},
	Date-Added = {2015-02-09 14:41:26 +0000},
	Date-Modified = {2015-02-09 14:41:38 +0000},
	Doi = {10.1086/148444},
	Journal = {\apj},
	Month = nov,
	Pages = {1633-1641},
	Title = {{On the Density of Neutral Hydrogen in Intergalactic Space.}},
	Volume = 142,
	Year = 1965,
	Bdsk-Url-1 = {http://dx.doi.org/10.1086/148444}}

@article{Planck:2013,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2014A%26A...571A..15P},
	Archiveprefix = {arXiv},
	Author = {{Planck Collaboration} and {Ade}, P.~A.~R. and {Aghanim}, N. and {Armitage-Caplan}, C. and {Arnaud}, M. and {Ashdown}, M. and {Atrio-Barandela}, F. and {Aumont}, J. and {Baccigalupi}, C. and {Banday}, A.~J. and et al.},
	Date-Added = {2015-02-09 14:39:56 +0000},
	Date-Modified = {2015-02-09 14:40:04 +0000},
	Doi = {10.1051/0004-6361/201321573},
	Eid = {A15},
	Eprint = {1303.5075},
	Journal = {\aap},
	Keywords = {cosmic background radiation, cosmological parameters, cosmology: observations, methods: data analysis},
	Month = nov,
	Pages = {A15},
	Title = {{Planck 2013 results. XV. CMB power spectra and likelihood}},
	Volume = 571,
	Year = 2014,
	Bdsk-Url-1 = {http://dx.doi.org/10.1051/0004-6361/201321573}}

@article{WMAP9,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2013ApJS..208...20B},
	Archiveprefix = {arXiv},
	Author = {{Bennett}, C.~L. and {Larson}, D. and {Weiland}, J.~L. and {Jarosik}, N. and {Hinshaw}, G. and {Odegard}, N. and {Smith}, K.~M. and {Hill}, R.~S. and {Gold}, B. and {Halpern}, M. and {Komatsu}, E. and {Nolta}, M.~R. and {Page}, L. and {Spergel}, D.~N. and {Wollack}, E. and {Dunkley}, J. and {Kogut}, A. and {Limon}, M. and {Meyer}, S.~S. and {Tucker}, G.~S. and {Wright}, E.~L.},
	Date-Added = {2015-02-09 14:34:49 +0000},
	Date-Modified = {2015-02-09 14:34:59 +0000},
	Doi = {10.1088/0067-0049/208/2/20},
	Eid = {20},
	Eprint = {1212.5225},
	Journal = {\apjs},
	Keywords = {cosmic background radiation, cosmology: observations, dark matter, early universe, instrumentation: detectors, space vehicles, space vehicles: instruments, telescopes},
	Month = oct,
	Pages = {20},
	Primaryclass = {astro-ph.CO},
	Title = {{Nine-year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Final Maps and Results}},
	Volume = 208,
	Year = 2013,
	Bdsk-Url-1 = {http://dx.doi.org/10.1088/0067-0049/208/2/20}}

@article{Planck:2015,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2015arXiv150201589P},
	Archiveprefix = {arXiv},
	Author = {{Planck Collaboration} and {Ade}, P.~A.~R. and {Aghanim}, N. and {Arnaud}, M. and {Ashdown}, M. and {Aumont}, J. and {Baccigalupi}, C. and {Banday}, A.~J. and {Barreiro}, R.~B. and {Bartlett}, J.~G. and et al.},
	Date-Added = {2015-02-09 14:27:33 +0000},
	Date-Modified = {2016-06-03 20:33:24 +0000},
	Eprint = {1502.01589},
	Journal = {{ArXiv e-prints, arXiv:1502.01589}},
	Keywords = {Astrophysics - Cosmology and Nongalactic Astrophysics},
	Month = feb,
	Title = {{Planck 2015 results. XIII. Cosmological parameters}},
	Year = 2015}

@article{Fan:2006b,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2006ARA%26A..44..415F},
	Author = {{Fan}, X. and {Carilli}, C.~L. and {Keating}, B.},
	Date-Added = {2015-02-05 18:13:28 +0000},
	Date-Modified = {2015-02-05 18:45:43 +0000},
	Doi = {10.1146/annurev.astro.44.051905.092514},
	Eprint = {astro-ph/0602375},
	Journal = {\araa},
	Keywords = {contraints,observational,review},
	Month = sep,
	Pages = {415-462},
	Title = {{Observational Constraints on Cosmic Reionization}},
	Volume = 44,
	Year = 2006,
	Bdsk-Url-1 = {http://dx.doi.org/10.1146/annurev.astro.44.051905.092514}}

@article{Beardsley:2013,
	Abstract = {Using the final 128 antenna locations of the Murchison Widefield Array (MWA), we calculate its sensitivity to the epoch of reionization (EoR) power spectrum of redshifted 21 cm emission for a fiducial model and provide the tools to calculate the sensitivity for any model. Our calculation takes into account synthesis rotation, chromatic and asymmetrical baseline effects, and excludes modes that will be contaminated by foreground subtraction. For the fiducial model, the MWA will be capable of a 14σ detection of the EoR signal with one full season of observation on two fields (900 and 700 h).},
	Author = {Beardsley, A. P. and Hazelton, B. J. and Morales, M. F. and Arcus, W. and Barnes, D. and Bernardi, G. and Bowman, J. D. and Briggs, F. H. and Bunton, J. D. and Cappallo, R. J. and Corey, B. E. and Deshpande, A. and deSouza, L. and Emrich, D. and Gaensler, B. M. and Goeke, R. and Greenhill, L. J. and Herne, D. and Hewitt, J. N. and Johnston-Hollitt, M. and Kaplan, D. L. and Kasper, J. C. and Kincaid, B. B. and Koenig, R. and Kratzenberg, E. and Lonsdale, C. J. and Lynch, M. J. and McWhirter, S. R. and Mitchell, D. A. and Morgan, E. and Oberoi, D. and Ord, S. M. and Pathikulangara, J. and Prabu, T. and Remillard, R. A. and Rogers, A. E. E. and Roshi, A. and Salah, J. E. and Sault, R. J. and Udaya, Shankar N. and Srivani, K. S. and Stevens, J. and Subrahmanyan, R. and Tingay, S. J. and Wayth, R. B. and Waterson, M. and Webster, R. L. and Whitney, A. R. and Williams, A. and Williams, C. L. and Wyithe, J. S. B.},
	Date-Added = {2014-10-27 15:45:18 +0000},
	Date-Modified = {2015-10-23 15:47:47 +0000},
	Doi = {10.1093/mnrasl/sls013},
	Journal = {Monthly Notices of the Royal Astronomical Society: Letters},
	Number = {1},
	Pages = {L5-L9},
	Title = {The EoR sensitivity of the Murchison Widefield Array},
	Url = {http://mnrasl.oxfordjournals.org/content/429/1/L5.abstract},
	Volume = {429},
	Year = {2013},
	Bdsk-Url-1 = {http://mnrasl.oxfordjournals.org/content/429/1/L5.abstract},
	Bdsk-Url-2 = {http://dx.doi.org/10.1093/mnrasl/sls013}}

@article{Beardsley:2014,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2014arXiv1410.5427B},
	Archiveprefix = {arXiv},
	Author = {{Beardsley}, A.~P. and {Morales}, M.~F. and {Lidz}, A. and {Malloy}, M. and {Sutter}, P.~M.},
	Date-Added = {2014-10-22 15:22:56 +0000},
	Date-Modified = {2014-10-22 15:30:02 +0000},
	Eprint = {1410.5427},
	Journal = {arXiv:1410.5427},
	Keywords = {Astrophysics - Cosmology and Nongalactic Astrophysics},
	Month = oct,
	Title = {{Adding Context to JWST Surveys with Current and Future 21cm Radio Observations}},
	Year = 2014}

@article{Chapman:2013,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2013MNRAS.429..165C},
	Archiveprefix = {arXiv},
	Author = {{Chapman}, E. and {Abdalla}, F.~B. and {Bobin}, J. and {Starck}, J.-L. and {Harker}, G. and {Jeli{\'c}}, V. and {Labropoulos}, P. and {Zaroubi}, S. and {Brentjens}, M.~A. and {de Bruyn}, A.~G. and {Koopmans}, L.~V.~E.},
	Date-Added = {2014-10-15 20:16:08 +0000},
	Date-Modified = {2015-02-18 17:35:33 +0000},
	Doi = {10.1093/mnras/sts333},
	Eprint = {1209.4769},
	Journal = {\mnras},
	Keywords = {methods: statistical, cosmology: theory, dark ages, reionization, first stars, diffuse radiation},
	Month = feb,
	Pages = {165-176},
	Primaryclass = {astro-ph.CO},
	Title = {{The scale of the problem: recovering images of reionization with Generalized Morphological Component Analysis}},
	Volume = 429,
	Year = 2013,
	Bdsk-Url-1 = {http://dx.doi.org/10.1093/mnras/sts333}}

@article{Morales:2011,
	Abstract = {ABSTRACT. Proposed 21 cm cosmology observatories for studying the epoch of reionization (  ≈ 6--15 ) and dark energy (  ≈ 0--6 ) envision compact arrays with tens of thousands of antenna elements. Fully correlating this many elements is computationally expensive using traditional XF or FX correlators and has led some groups to reconsider direct imaging/FFT correlators. In this article we develop a variation of the direct imaging correlator that we call the MOFF correlator. The MOFF correlator shares the computational advantages of a direct imaging correlator, while avoiding a number of its shortcomings. In particular, the MOFF correlator makes no constraints on the antenna arrangement or type; provides a fully calibrated output image, including wide-field polarimetry and noncoplanar baseline effects; and can be orders of magnitude more efficient than XF or FX correlators for compact radio cosmology arrays.},
	Author = {Morales, Miguel F.},
	Copyright = {Copyright {\copyright} 2011 The University of Chicago Press},
	Date-Added = {2014-10-14 21:37:58 +0000},
	Date-Modified = {2014-10-14 21:38:04 +0000},
	Issn = {00046280},
	Journal = {Publications of the Astronomical Society of the Pacific},
	Jstor_Articletype = {research-article},
	Jstor_Formatteddate = {November 2011},
	Language = {English},
	Number = {909},
	Pages = {pp. 1265-1272},
	Publisher = {The University of Chicago Press on behalf of the Astronomical Society of the Pacific},
	Title = {Enabling Next-Generation Dark Energy and Epoch of Reionization Radio Observatories with the MOFF Correlator},
	Url = {http://www.jstor.org/stable/10.1086/663092},
	Volume = {123},
	Year = {2011},
	Bdsk-Url-1 = {http://www.jstor.org/stable/10.1086/663092}}

@article{Kashikawa:2006,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2006ApJ...648....7K},
	Author = {{Kashikawa}, N. and {Shimasaku}, K. and {Malkan}, M.~A. and {Doi}, M. and {Matsuda}, Y. and {Ouchi}, M. and {Taniguchi}, Y. and {Ly}, C. and {Nagao}, T. and {Iye}, M. and {Motohara}, K. and {Murayama}, T. and {Murozono}, K. and {Nariai}, K. and {Ohta}, K. and {Okamura}, S. and {Sasaki}, T. and {Shioya}, Y. and {Umemura}, M.},
	Date-Added = {2014-10-12 22:13:49 +0000},
	Date-Modified = {2014-10-12 22:14:02 +0000},
	Doi = {10.1086/504966},
	Eprint = {astro-ph/0604149},
	Journal = {\apj},
	Keywords = {Cosmology: Observations, Cosmology: Early Universe, Galaxies: Formation, Galaxies: High-Redshift},
	Month = sep,
	Pages = {7-22},
	Title = {{The End of the Reionization Epoch Probed by Ly{$\alpha$} Emitters at z = 6.5 in the Subaru Deep Field}},
	Volume = 648,
	Year = 2006,
	Bdsk-Url-1 = {http://dx.doi.org/10.1086/504966}}

@article{Lidz:2009,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2009ApJ...690..252L},
	Archiveprefix = {arXiv},
	Author = {{Lidz}, A. and {Zahn}, O. and {Furlanetto}, S.~R. and {McQuinn}, M. and {Hernquist}, L. and {Zaldarriaga}, M.},
	Date-Added = {2014-10-10 15:59:31 +0000},
	Date-Modified = {2014-10-10 15:59:36 +0000},
	Doi = {10.1088/0004-637X/690/1/252},
	Eprint = {0806.1055},
	Journal = {\apj},
	Keywords = {cosmology: theory, intergalactic medium, large-scale structure of universe},
	Month = jan,
	Pages = {252-266},
	Title = {{Probing Reionization with the 21 cm Galaxy Cross-Power Spectrum}},
	Volume = 690,
	Year = 2009,
	Bdsk-Url-1 = {http://dx.doi.org/10.1088/0004-637X/690/1/252}}

@article{Spergel:2013,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2013arXiv1305.5422S},
	Archiveprefix = {arXiv},
	Author = {{Spergel}, D. and {Gehrels}, N. and {Breckinridge}, J. and {Donahue}, M. and {Dressler}, A. and {Gaudi}, B.~S. and {Greene}, T. and {Guyon}, O. and {Hirata}, C. and {Kalirai}, J. and {Kasdin}, N.~J. and {Moos}, W. and {Perlmutter}, S. and {Postman}, M. and {Rauscher}, B. and {Rhodes}, J. and {Wang}, Y. and {Weinberg}, D. and {Centrella}, J. and {Traub}, W. and {Baltay}, C. and {Colbert}, J. and {Bennett}, D. and {Kiessling}, A. and {Macintosh}, B. and {Merten}, J. and {Mortonson}, M. and {Penny}, M. and {Rozo}, E. and {Savransky}, D. and {Stapelfeldt}, K. and {Zu}, Y. and {Baker}, C. and {Cheng}, E. and {Content}, D. and {Dooley}, J. and {Foote}, M. and {Goullioud}, R. and {Grady}, K. and {Jackson}, C. and {Kruk}, J. and {Levine}, M. and {Melton}, M. and {Peddie}, C. and {Ruffa}, J. and {Shaklan}, S.},
	Date-Added = {2014-10-09 23:12:26 +0000},
	Date-Modified = {2014-10-09 23:12:32 +0000},
	Eprint = {1305.5422},
	Journal = {ArXiv e-prints},
	Keywords = {Astrophysics - Instrumentation and Methods for Astrophysics},
	Month = may,
	Primaryclass = {astro-ph.IM},
	Title = {{Wide-Field InfraRed Survey Telescope-Astrophysics Focused Telescope Assets WFIRST-AFTA Final Report}},
	Year = 2013}

@article{Giavalisco:2004,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2004ApJ...600L..93G},
	Author = {{Giavalisco}, M. and {Ferguson}, H.~C. and {Koekemoer}, A.~M. and {Dickinson}, M. and {Alexander}, D.~M. and {Bauer}, F.~E. and {Bergeron}, J. and {Biagetti}, C. and {Brandt}, W.~N. and {Casertano}, S. and {Cesarsky}, C. and {Chatzichristou}, E. and {Conselice}, C. and {Cristiani}, S. and {Da Costa}, L. and {Dahlen}, T. and {de Mello}, D. and {Eisenhardt}, P. and {Erben}, T. and {Fall}, S.~M. and {Fassnacht}, C. and {Fosbury}, R. and {Fruchter}, A. and {Gardner}, J.~P. and {Grogin}, N. and {Hook}, R.~N. and {Hornschemeier}, A.~E. and {Idzi}, R. and {Jogee}, S. and {Kretchmer}, C. and {Laidler}, V. and {Lee}, K.~S. and {Livio}, M. and {Lucas}, R. and {Madau}, P. and {Mobasher}, B. and {Moustakas}, L.~A. and {Nonino}, M. and {Padovani}, P. and {Papovich}, C. and {Park}, Y. and {Ravindranath}, S. and {Renzini}, A. and {Richardson}, M. and {Riess}, A. and {Rosati}, P. and {Schirmer}, M. and {Schreier}, E. and {Somerville}, R.~S. and {Spinrad}, H. and {Stern}, D. and {Stiavelli}, M. and {Strolger}, L. and {Urry}, C.~M. and {Vandame}, B. and {Williams}, R. and {Wolf}, C.},
	Date-Added = {2014-10-09 23:04:18 +0000},
	Date-Modified = {2014-10-09 23:04:25 +0000},
	Doi = {10.1086/379232},
	Eprint = {astro-ph/0309105},
	Journal = {\apjl},
	Keywords = {Cosmology: Observations, Galaxies: Distances and Redshifts, Galaxies: Evolution, Galaxies: Formation},
	Month = jan,
	Pages = {L93-L98},
	Title = {{The Great Observatories Origins Deep Survey: Initial Results from Optical and Near-Infrared Imaging}},
	Volume = 600,
	Year = 2004,
	Bdsk-Url-1 = {http://dx.doi.org/10.1086/379232}}

@article{Lazio:2014,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2014PASP..126..196L},
	Author = {{Lazio}, J.~W. and {Kimball}, A. and {Barger}, A.~J. and {Brandt}, W.~N. and {Chatterjee}, S. and {Clarke}, T.~E. and {Condon}, J.~J. and {Dickman}, R.~L. and {Hunyh}, M.~T. and {Jarvis}, M.~J. and {Juri{\'c}}, M. and {Kassim}, N.~E. and {Myers}, S.~T. and {Nissanke}, S. and {Osten}, R. and {Zauderer}, B.~A.},
	Date-Added = {2014-10-09 22:42:06 +0000},
	Date-Modified = {2014-10-09 22:42:13 +0000},
	Doi = {10.1086/675262},
	Journal = {\pasp},
	Month = feb,
	Pages = {196-209},
	Title = {{Radio Astronomy in LSST Era}},
	Volume = 126,
	Year = 2014,
	Bdsk-Url-1 = {http://dx.doi.org/10.1086/675262}}

@article{Zackrisson:2011,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2011ApJ...740...13Z},
	Archiveprefix = {arXiv},
	Author = {{Zackrisson}, E. and {Rydberg}, C.-E. and {Schaerer}, D. and {{\"O}stlin}, G. and {Tuli}, M.},
	Date-Added = {2014-10-09 16:03:38 +0000},
	Date-Modified = {2014-10-09 16:03:43 +0000},
	Doi = {10.1088/0004-637X/740/1/13},
	Eid = {13},
	Eprint = {1105.0921},
	Journal = {\apj},
	Keywords = {dark ages, reionization, first stars, galaxies: high-redshift, stars: Population III},
	Month = oct,
	Pages = {13},
	Primaryclass = {astro-ph.CO},
	Title = {{The Spectral Evolution of the First Galaxies. I. James Webb Space Telescope Detection Limits and Color Criteria for Population III Galaxies}},
	Volume = 740,
	Year = 2011,
	Bdsk-Url-1 = {http://dx.doi.org/10.1088/0004-637X/740/1/13}}

@article{Zackrisson:2012,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2012MNRAS.427.2212Z},
	Archiveprefix = {arXiv},
	Author = {{Zackrisson}, E. and {Zitrin}, A. and {Trenti}, M. and {Rydberg}, C.-E. and {Guaita}, L. and {Schaerer}, D. and {Broadhurst}, T. and {{\"O}stlin}, G. and {Str{\"o}m}, T.},
	Date-Added = {2014-10-09 16:01:12 +0000},
	Date-Modified = {2014-10-09 16:01:22 +0000},
	Doi = {10.1111/j.1365-2966.2012.22078.x},
	Eprint = {1204.0517},
	Journal = {\mnras},
	Keywords = {stars: Population III, galaxies: high-redshift, dark ages, reionization, first stars},
	Month = dec,
	Pages = {2212-2223},
	Primaryclass = {astro-ph.CO},
	Title = {{Detecting gravitationally lensed Population III galaxies with the Hubble Space Telescope and the James Webb Space Telescope}},
	Volume = 427,
	Year = 2012,
	Bdsk-Url-1 = {http://dx.doi.org/10.1111/j.1365-2966.2012.22078.x}}

@article{Gardner:2006,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2006SSRv..123..485G},
	Author = {{Gardner}, J.~P. and {Mather}, J.~C. and {Clampin}, M. and {Doyon}, R. and {Greenhouse}, M.~A. and {Hammel}, H.~B. and {Hutchings}, J.~B. and {Jakobsen}, P. and {Lilly}, S.~J. and {Long}, K.~S. and {Lunine}, J.~I. and {McCaughrean}, M.~J. and {Mountain}, M. and {Nella}, J. and {Rieke}, G.~H. and {Rieke}, M.~J. and {Rix}, H.-W. and {Smith}, E.~P. and {Sonneborn}, G. and {Stiavelli}, M. and {Stockman}, H.~S. and {Windhorst}, R.~A. and {Wright}, G.~S.},
	Date-Added = {2014-10-09 15:59:04 +0000},
	Date-Modified = {2014-10-09 15:59:19 +0000},
	Doi = {10.1007/s11214-006-8315-7},
	Eprint = {astro-ph/0606175},
	Journal = {\ssr},
	Keywords = {galaxies: formation, infrared: general, planetary systems, space vehicles: instruments, stars: formation},
	Month = apr,
	Pages = {485-606},
	Title = {{The James Webb Space Telescope}},
	Volume = 123,
	Year = 2006,
	Bdsk-Url-1 = {http://dx.doi.org/10.1007/s11214-006-8315-7}}

@book{DecadalSurvey:2010,
	Address = {Washington, DC},
	Author = {{National Research Council}},
	Date-Added = {2014-10-08 15:22:23 +0000},
	Date-Modified = {2014-11-21 16:53:53 +0000},
	Publisher = {The National Academies Press},
	Title = {New Worlds, New Horizons in Astronomy and Astrophysics},
	Year = {2010},
	Bdsk-Url-1 = {http://www.nap.edu/catalog.php?record_id=12951}}

@article{Bouwens:2010,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2010ApJ...709L.133B},
	Archiveprefix = {arXiv},
	Author = {{Bouwens}, R.~J. and {Illingworth}, G.~D. and {Oesch}, P.~A. and {Stiavelli}, M. and {van Dokkum}, P. and {Trenti}, M. and {Magee}, D. and {Labb{\'e}}, I. and {Franx}, M. and {Carollo}, C.~M. and {Gonzalez}, V.},
	Date-Added = {2014-10-07 15:05:52 +0000},
	Date-Modified = {2014-10-15 16:48:10 +0000},
	Doi = {10.1088/2041-8205/709/2/L133},
	Eprint = {0909.1803},
	Journal = {ApJ},
	Keywords = {galaxies: evolution, galaxies: high-redshift},
	Month = feb,
	Pages = {L133-L137},
	Primaryclass = {astro-ph.CO},
	Title = {{Discovery of z \~{} 8 Galaxies in the Hubble Ultra Deep Field from Ultra-Deep WFC3/IR Observations}},
	Volume = 709,
	Year = 2010,
	Bdsk-Url-1 = {http://dx.doi.org/10.1088/2041-8205/709/2/L133}}

@article{Fan:2006a,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2006AJ....132..117F},
	Author = {{Fan}, X. and {Strauss}, M.~A. and {Becker}, R.~H. and {White}, R.~L. and {Gunn}, J.~E. and {Knapp}, G.~R. and {Richards}, G.~T. and {Schneider}, D.~P. and {Brinkmann}, J. and {Fukugita}, M.},
	Date-Added = {2014-10-07 15:03:09 +0000},
	Date-Modified = {2015-02-05 18:13:52 +0000},
	Doi = {10.1086/504836},
	Eprint = {astro-ph/0512082},
	Journal = {AJ},
	Keywords = {Cosmology: Observations, Galaxies: Intergalactic Medium, Galaxies: Quasars: Absorption Lines, Galaxies: Quasars: General},
	Month = jul,
	Pages = {117-136},
	Title = {{Constraining the Evolution of the Ionizing Background and the Epoch of Reionization with z\~{}6 Quasars. II. A Sample of 19 Quasars}},
	Volume = 132,
	Year = 2006,
	Bdsk-Url-1 = {http://dx.doi.org/10.1086/504836}}

@article{Dunkley:2009,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2009ApJS..180..306D},
	Archiveprefix = {arXiv},
	Author = {{Dunkley}, J. and {Komatsu}, E. and {Nolta}, M.~R. and {Spergel}, D.~N. and {Larson}, D. and {Hinshaw}, G. and {Page}, L. and {Bennett}, C.~L. and {Gold}, B. and {Jarosik}, N. and {Weiland}, J.~L. and {Halpern}, M. and {Hill}, R.~S. and {Kogut}, A. and {Limon}, M. and {Meyer}, S.~S. and {Tucker}, G.~S. and {Wollack}, E. and {Wright}, E.~L.},
	Date-Added = {2014-10-07 14:42:47 +0000},
	Date-Modified = {2014-10-07 14:42:54 +0000},
	Doi = {10.1088/0067-0049/180/2/306},
	Eprint = {0803.0586},
	Journal = {\apjs},
	Keywords = {cosmic microwave background, cosmology: observations, early universe, polarization},
	Month = feb,
	Pages = {306-329},
	Title = {{Five-Year Wilkinson Microwave Anisotropy Probe Observations: Likelihoods and Parameters from the WMAP Data}},
	Volume = 180,
	Year = 2009,
	Bdsk-Url-1 = {http://dx.doi.org/10.1088/0067-0049/180/2/306}}

@article{Mesinger:2011,
	Abstract = {We introduce a powerful seminumeric modelling tool, 21cmfast, designed to efficiently simulate the cosmological 21-cm signal. Our code generates 3D realizations of evolved density, ionization, peculiar velocity and spin temperature fields, which it then combines to compute the 21-cm brightness temperature. Although the physical processes are treated with approximate methods, we compare our results to a state-of-the-art large-scale hydrodynamic simulation, and find good agreement on scales pertinent to the upcoming observations (≳1 Mpc). The power spectra from 21cmfast agree with those generated from the numerical simulation to within 10s of per cent, down to the Nyquist frequency. We show results from a 1-Gpc simulation which tracks the cosmic 21-cm signal down from z= 250, highlighting the various interesting epochs. Depending on the desired resolution, 21cmfast can compute a redshift realization on a single processor in just a few minutes. Our code is fast, efficient, customizable and publicly available, making it a useful tool for 21-cm parameter studies.},
	Author = {Mesinger, Andrei and Furlanetto, Steven and Cen, Renyue},
	Date-Added = {2014-10-06 17:36:58 +0000},
	Date-Modified = {2015-10-23 15:48:23 +0000},
	Doi = {10.1111/j.1365-2966.2010.17731.x},
	Journal = {Monthly Notices of the Royal Astronomical Society},
	Number = {2},
	Pages = {955-972},
	Title = {21cmfast: a fast, seminumerical simulation of the high-redshift 21-cm signal},
	Url = {http://mnras.oxfordjournals.org/content/411/2/955.abstract},
	Volume = {411},
	Year = {2011},
	Bdsk-Url-1 = {http://mnras.oxfordjournals.org/content/411/2/955.abstract},
	Bdsk-Url-2 = {http://dx.doi.org/10.1111/j.1365-2966.2010.17731.x}}

@article{Furlanetto:2004,
	Abstract = {Recently, there has been a great deal of interest in understanding the reionization of hydrogen in the intergalactic medium (IGM). One of the major outstanding questions is how this event proceeds on large scales. Motivated by numerical simulations, we develop a model for the growth of H II regions during the reionization era. We associate ionized regions with large-scale density fluctuations and use the excursion set formalism to model the resulting size distribution. We then consider ways in which to characterize the morphology of ionized regions. We show how to construct the power spectrum of fluctuations in the neutral hydrogen field. The power spectrum contains definite features from the H II regions that should be observable with the next generation of low-frequency radio telescopes through surveys of redshifted 21 cm emission from the reionization era. Finally, we also consider statistical descriptions beyond the power spectrum and show that our model of reionization qualitatively changes the distribution of neutral gas in the IGM.},
	Author = {Steven R. Furlanetto and Matias Zaldarriaga and Lars Hernquist},
	Date-Added = {2014-10-06 17:34:00 +0000},
	Date-Modified = {2015-02-05 18:46:00 +0000},
	Journal = {The Astrophysical Journal},
	Number = {1},
	Pages = {1},
	Title = {The Growth of H II Regions During Reionization},
	Url = {http://stacks.iop.org/0004-637X/613/i=1/a=1},
	Volume = {613},
	Year = {2004},
	Bdsk-Url-1 = {http://stacks.iop.org/0004-637X/613/i=1/a=1}}

@article{Rogers:2012,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2012JAtOT..29.1492R},
	Author = {{Rogers}, A.~E.~E. and {Erickson}, P. and {Fish}, V.~L. and {Kittredge}, J. and {Danford}, S. and {Marr}, J.~M. and {Arndt}, M.~B. and {Sarabia}, J. and {Costa}, D. and {May}, S.~K.},
	Date-Added = {2014-10-05 01:25:48 +0000},
	Date-Modified = {2014-10-05 01:25:53 +0000},
	Doi = {10.1175/JTECH-D-11-00193.1},
	Journal = {Journal of Atmospheric and Oceanic Technology},
	Month = oct,
	Pages = {1492-1504},
	Title = {{Repeatability of the Seasonal Variations of Ozone near the Mesopause from Observations of the 11.072-GHz Line}},
	Volume = 29,
	Year = 2012,
	Bdsk-Url-1 = {http://dx.doi.org/10.1175/JTECH-D-11-00193.1}}

@article{Pober:2014,
	Abstract = {A number of experiments are currently working toward a measurement of the 21 cm signal from the epoch of reionization (EoR). Whether or not these experiments deliver a detection of cosmological emission, their limited sensitivity will prevent them from providing detailed information about the astrophysics of reionization. In this work, we consider what types of measurements will be enabled by the next generation of larger 21 cm EoR telescopes. To calculate the type of constraints that will be possible with such arrays, we use simple models for the instrument, foreground emission, and the reionization history. We focus primarily on an instrument modeled after the ~0.1 km 2 collecting area Hydrogen Epoch of Reionization Array concept design and parameterize the uncertainties with regard to foreground emission by considering different limits to the recently described "wedge" footprint in k space. Uncertainties in the reionization history are accounted for using a series of simulations that vary the ionizing efficiency and minimum virial temperature of the galaxies responsible for reionization, as well as the mean free path of ionizing photons through the intergalactic medium. Given various combinations of models, we consider the significance of the possible power spectrum detections, the ability to trace the power spectrum evolution versus redshift, the detectability of salient power spectrum features, and the achievable level of quantitative constraints on astrophysical parameters. Ultimately, we find that 0.1 km 2 of collecting area is enough to ensure a very high significance ( ##IMG## [http://ej.iop.org/icons/Entities/gsim.gif] {gsim} 30σ) detection of the reionization power spectrum in even the most pessimistic scenarios. This sensitivity should allow for meaningful constraints on the reionization history and astrophysical parameters, especially if foreground subtraction techniques can be improved and successfully implemented.},
	Author = {Jonathan C. Pober and Adrian Liu and Joshua S. Dillon and James E. Aguirre and Judd D. Bowman and Richard F. Bradley and Chris L. Carilli and David R. DeBoer and Jacqueline N. Hewitt and Daniel C. Jacobs and Matthew McQuinn and Miguel F. Morales and Aaron R. Parsons and Max Tegmark and Dan J. Werthimer},
	Date-Added = {2014-10-04 21:32:02 +0000},
	Date-Modified = {2015-02-18 17:36:14 +0000},
	Journal = {The Astrophysical Journal},
	Number = {2},
	Pages = {66},
	Title = {What Next-generation 21 cm Power Spectrum Measurements can Teach us About the Epoch of Reionization},
	Url = {http://stacks.iop.org/0004-637X/782/i=2/a=66},
	Volume = {782},
	Year = {2014},
	Bdsk-Url-1 = {http://stacks.iop.org/0004-637X/782/i=2/a=66}}

@article{Ellingson:2009,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2009IEEEP..97.1421E},
	Author = {{Ellingson}, S.~W. and {Clarke}, T.~E. and {Cohen}, A. and {Craig}, J. and {Kassim}, N.~E. and {Pihlstrom}, Y. and {Rickard}, L.~J. and {Taylor}, G.~B.},
	Date-Added = {2014-10-04 17:17:24 +0000},
	Date-Modified = {2014-10-04 17:17:35 +0000},
	Doi = {10.1109/JPROC.2009.2015683},
	Journal = {IEEE Proceedings},
	Month = aug,
	Pages = {1421-1430},
	Title = {{The Long Wavelength Array}},
	Volume = 97,
	Year = 2009,
	Bdsk-Url-1 = {http://dx.doi.org/10.1109/JPROC.2009.2015683}}

@article{Parsons:2012a,
	Author = {Parsons, Aaron and Pober, Jonathan and McQuinn, Matthew and Jacobs, Daniel and Aguirre, James},
	Date-Added = {2014-10-03 19:28:25 +0000},
	Date-Modified = {2015-02-18 17:35:56 +0000},
	Journal = {ApJ},
	Number = {1},
	Pages = {81},
	Publisher = {IOP Publishing},
	Title = {A sensitivity and array-configuration study for measuring the power spectrum of 21 cm emission from reionization},
	Volume = {753},
	Year = {2012}}

@article{Liu:2014b,
	Author = {Liu, Adrian and Parsons, Aaron R. and Trott, Cathryn M.},
	Date-Added = {2014-08-31 18:43:24 +0000},
	Date-Modified = {2014-08-31 18:46:11 +0000},
	Doi = {10.1103/PhysRevD.90.023019},
	Issue = {2},
	Journal = {Phys. Rev. D},
	Keywords = {wedge},
	Month = {Jul},
	Numpages = {20},
	Pages = {023019},
	Publisher = {American Physical Society},
	Title = {Epoch of reionization window. II. Statistical methods for foreground wedge reduction},
	Url = {http://link.aps.org/doi/10.1103/PhysRevD.90.023019},
	Volume = {90},
	Year = {2014},
	Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevD.90.023019},
	Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevD.90.023019}}

@article{Liu:2014a,
	Author = {Liu, Adrian and Parsons, Aaron R. and Trott, Cathryn M.},
	Date-Added = {2014-08-31 18:41:27 +0000},
	Date-Modified = {2014-08-31 18:46:02 +0000},
	Doi = {10.1103/PhysRevD.90.023018},
	Issue = {2},
	Journal = {Phys. Rev. D},
	Keywords = {wedge},
	Month = {Jul},
	Numpages = {27},
	Pages = {023018},
	Publisher = {American Physical Society},
	Title = {Epoch of reionization window. I. Mathematical formalism},
	Url = {http://link.aps.org/doi/10.1103/PhysRevD.90.023018},
	Volume = {90},
	Year = {2014},
	Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevD.90.023018},
	Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevD.90.023018}}

@article{Hogg:1999,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/1999astro.ph..5116H},
	Author = {{Hogg}, D.~W.},
	Date-Added = {2014-08-31 17:48:26 +0000},
	Date-Modified = {2014-08-31 17:48:33 +0000},
	Eprint = {astro-ph/9905116},
	Journal = {ArXiv Astrophysics e-prints},
	Keywords = {Astrophysics},
	Month = may,
	Title = {{Distance measures in cosmology}},
	Year = 1999}

@article{Mortlock:2011,
	Annote = {10.1038/nature10159},
	Author = {Mortlock, Daniel J. and Warren, Stephen J. and Venemans, Bram P. and Patel, Mitesh and Hewett, Paul C. and McMahon, Richard G. and Simpson, Chris and Theuns, Tom and Gonzales-Solares, Eduardo A. and Adamson, Andy and Dye, Simon and Hambly, Nigel C. and Hirst, Paul and Irwin, Mike J. and Kuiper, Ernst and Lawrence, Andy and Rottgering, Huub J. A.},
	Date = {2011/06/30/print},
	Date-Added = {2014-08-26 19:48:47 +0000},
	Date-Modified = {2014-08-26 19:48:47 +0000},
	Day = {30},
	Isbn = {0028-0836},
	Journal = {Nature},
	M3 = {10.1038/nature10159},
	Month = {06},
	Number = {7353},
	Pages = {616--619},
	Publisher = {Nature Publishing Group, a division of Macmillan Publishers Limited. All Rights Reserved.},
	Title = {A luminous quasar at a redshift of z = 7.085},
	Ty = {JOUR},
	Url = {http://dx.doi.org/10.1038/nature10159},
	Volume = {474},
	Year = {2011},
	Bdsk-Url-1 = {http://dx.doi.org/10.1038/nature10159}}

@article{Offringa:2014,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2014arXiv1407.1943O},
	Archiveprefix = {arXiv},
	Author = {{Offringa}, A.~R. and {McKinley}, B. and {Hurley-Walker}, N. and {Briggs}, F.~H. and {Wayth}, R.~B. and {Kaplan}, D.~L. and {Bell}, M.~E. and {Feng}, L. and {Neben}, A.~R. and {Hughes}, J.~D. and {Rhee}, J. and {Murphy}, T. and {Bhat}, N.~D.~R. and {Bernardi}, G. and {Bowman}, J.~D. and {Cappallo}, R.~J. and {Corey}, B.~E. and {Deshpande}, A.~A. and {Emrich}, D. and {Ewall-Wice}, A. and {Gaensler}, B.~M. and {Goeke}, R. and {Greenhill}, L.~J. and {Hazelton}, B.~J. and {Hindson}, L. and {Johnston-Hollitt}, M. and {Jacobs}, D.~C. and {Kasper}, J.~C. and {Kratzenberg}, E. and {Lenc}, E. and {Lonsdale}, C.~J. and {Lynch}, M.~J. and {McWhirter}, S.~R. and {Mitchell}, D.~A. and {Morales}, M.~F. and {Morgan}, E. and {Kudryavtseva}, N. and {Oberoi}, D. and {Ord}, S.~M. and {Pindor}, B. and {Procopio}, P. and {Prabu}, T. and {Riding}, J. and {Roshi}, D.~A. and {Udaya Shankar}, N. and {Srivani}, K.~S. and {Subrahmanyan}, R. and {Tingay}, S.~J. and {Waterson}, M. and {Webster}, R.~L. and {Whitney}, A.~R. and {Williams}, A. and {Williams}, C.~L.},
	Date-Added = {2014-08-04 14:29:50 +0000},
	Date-Modified = {2014-08-04 14:30:00 +0000},
	Eprint = {1407.1943},
	Journal = {ArXiv e-prints},
	Keywords = {Astrophysics - Instrumentation and Methods for Astrophysics},
	Month = jul,
	Primaryclass = {astro-ph.IM},
	Title = {{WSClean: an implementation of a fast, generic wide-field imager for radio astronomy}},
	Year = 2014}

@inproceedings{Cornwell:1989,
	Author = {Cornwell, Tim and Fomalont, Edward B},
	Booktitle = {Synthesis Imaging in Radio Astronomy},
	Date-Added = {2014-06-05 20:42:55 +0000},
	Date-Modified = {2014-06-05 20:43:37 +0000},
	Pages = {185},
	Title = {Self-calibration},
	Volume = {6},
	Year = {1989}}

@article{Tingay:2013,
	Author = {Tingay,S. J. and Goeke,R. and Bowman,J. D. and Emrich,D. and Ord,S. M. and Mitchell,D. A. and Morales,M. F. and Booler,T. and Crosse,B. and Wayth,R. B. and Lonsdale,C. J. and Tremblay,S. and Pallot,D. and Colegate,T. and Wicenec,A. and Kudryavtseva,N. and Arcus,W. and Barnes,D. and Bernardi,G. and Briggs,F. and Burns,S. and Bunton,J. D. and Cappallo,R. J. and Corey,B. E. and Deshpande,A. and Desouza,L. and Gaensler,B. M. and Greenhill,L. J. and Hall,P. J. and Hazelton,B. J. and Herne,D. and Hewitt,J. N. and Johnston-Hollitt,M. and Kaplan,D. L. and Kasper,J. C. and Kincaid,B. B. and Koenig,R. and Kratzenberg,E. and Lynch,M. J. and Mckinley,B. and Mcwhirter,S. R. and Morgan,E. and Oberoi,D. and Pathikulangara,J. and Prabu,T. and Remillard,R. A. and Rogers,A. E. E. and Roshi,A. and Salah,J. E. and Sault,R. J. and Udaya-Shankar,N. and Schlagenhaufer,F. and Srivani,K. S. and Stevens,J. and Subrahmanyan,R. and Waterson,M. and Webster,R. L. and Whitney,A. R. and Williams,A. and Williams,C. L. and Wyithe,J. S. B.},
	Date-Added = {2014-05-28 19:52:15 +0000},
	Date-Modified = {2015-08-05 17:33:34 +0000},
	Doi = {10.1017/pasa.2012.007},
	Issn = {1448-6083},
	Journal = {PASA - Publications of the Astronomical Society of Australia},
	Month = {1},
	Number = {e007},
	Title = {The Murchison Widefield Array: The Square Kilometre Array Precursor at Low Radio Frequencies},
	Url = {http://journals.cambridge.org/article_S1323358012000070},
	Volume = {30},
	Year = {2013},
	Bdsk-Url-1 = {http://journals.cambridge.org/article_S1323358012000070},
	Bdsk-Url-2 = {http://dx.doi.org/10.1017/pasa.2012.007}}

@article{Parsons:2010,
	Abstract = {We are developing the Precision Array for Probing the Epoch of Re-ionization (PAPER) to detect 21 cm emission from the early universe, when the first stars and galaxies were forming. We describe the overall experiment strategy and architecture and summarize two PAPER deployments: a four-antenna array in the low radio frequency interference (RFI) environment of Western Australia and an eight-antenna array at a prototyping site at the NRAO facilities near Green Bank, WV. From these activities we report on system performance, including primary beam model verification, dependence of system gain on ambient temperature, measurements of receiver and overall system temperatures, and characterization of the RFI environment at each deployment site. We present an all-sky map synthesized between 139 MHz and 174 MHz using data from both arrays that reaches down to 80 mJy (4.9 K, for a beam size of 2.15e--5 sr at 156 MHz), with a 10 mJy (620 mK) thermal noise level that indicates what would be achievable with better foreground subtraction. We calculate angular power spectra ( C ℓ ) in a cold patch and determine them to be dominated by point sources, but with contributions from galactic synchrotron emission at lower radio frequencies and angular wavemodes. Although the sample variance of foregrounds dominates errors in these power spectra, we measure a thermal noise level of 310 mK at ℓ = 100 for a 1.46 MHz band centered at 164.5 MHz. This sensitivity level is approximately 3 orders of magnitude in temperature above the level of the fluctuations in 21 cm emission associated with re-ionization.},
	Author = {Aaron R. Parsons and Donald C. Backer and Griffin S. Foster and Melvyn C. H. Wright and Richard F. Bradley and Nicole E. Gugliucci and Chaitali R. Parashare and Erin E. Benoit and James E. Aguirre and Daniel C. Jacobs and Chris L. Carilli and David Herne and Mervyn J. Lynch and Jason R. Manley and Daniel J. Werthimer},
	Date-Added = {2014-05-28 18:41:09 +0000},
	Date-Modified = {2014-05-28 18:41:19 +0000},
	Journal = {The Astronomical Journal},
	Number = {4},
	Pages = {1468},
	Title = {The Precision Array for Probing the Epoch of Re-ionization: Eight Station Results},
	Url = {http://stacks.iop.org/1538-3881/139/i=4/a=1468},
	Volume = {139},
	Year = {2010},
	Bdsk-Url-1 = {http://stacks.iop.org/1538-3881/139/i=4/a=1468}}

@article{Yatawatta:2013,
	Author = {Yatawatta, S. and de Bruyn, A. G. and Brentjens, M. A. and {Labropoulos, P.} and {Pandey, V. N.} and {Kazemi, S.} and {Zaroubi, S.} and {Koopmans, L. V. E.} and {Offringa, A. R.} and {Jeli{\'c}, V.} and {Martinez Rubi, O.} and {Veligatla, V.} and {Wijnholds, S. J.} and {Brouw, W. N.} and {Bernardi, G.} and {Ciardi, B.} and {Daiboo, S.} and {Harker, G.} and {Mellema, G.} and {Schaye, J.} and {Thomas, R.} and {Vedantham, H.} and {Chapman, E.} and {Abdalla, F. B.} and {Alexov, A.} and {Anderson, J.} and {Avruch, I. M.} and {Batejat, F.} and {Bell, M. E.} and {Bell, M. R.} and {Bentum, M.} and {Best, P.} and {Bonafede, A.} and {Bregman, J.} and {Breitling, F.} and {van de Brink, R. H.} and {Broderick, J. W.} and {Br{\"u}ggen, M.} and {Conway, J.} and {de Gasperin, F.} and {de Geus, E.} and {Duscha, S.} and {Falcke, H.} and {Fallows, R. A.} and {Ferrari, C.} and {Frieswijk, W.} and {Garrett, M. A.} and {Griessmeier, J. M.} and {Gunst, A. W.} and {Hassall, T. E.} and {Hessels, J. W. T.} and {Hoeft, M.} and {Iacobelli, M.} and {Juette, E.} and {Karastergiou, A.} and {Kondratiev, V. I.} and {Kramer, M.} and {Kuniyoshi, M.} and {Kuper, G.} and {van Leeuwen, J.} and {Maat, P.} and {Mann, G.} and {McKean, J. P.} and {Mevius, M.} and {Mol, J. D.} and {Munk, H.} and {Nijboer, R.} and {Noordam, J. E.} and {Norden, M. J.} and {Orru, E.} and {Paas, H.} and {Pandey-Pommier, M.} and {Pizzo, R.} and {Polatidis, A. G.} and {Reich, W.} and {R{\"o}ttgering, H. J. A.} and {Sluman, J.} and {Smirnov, O.} and {Stappers, B.} and {Steinmetz, M.} and {Tagger, M.} and {Tang, Y.} and {Tasse, C.} and {ter Veen, S.} and {Vermeulen, R.} and {van Weeren, R. J.} and {Wise, M.} and {Wucknitz, O.} and {Zarka, P.}},
	Date-Added = {2014-05-28 18:36:12 +0000},
	Date-Modified = {2014-10-12 20:53:10 +0000},
	Doi = {10.1051/0004-6361/201220874},
	Journal = {Astronomy and Astrophysics},
	Pages = {A136},
	Title = {Initial deep LOFAR observations of epoch of reionization windows},
	Url = {http://dx.doi.org/10.1051/0004-6361/201220874},
	Volume = 550,
	Year = 2013,
	Bdsk-Url-1 = {http://dx.doi.org/10.1051/0004-6361/201220874}}

@article{Paciga:2013,
	Abstract = {The Giant Metrewave Radio Telescope Epoch of Reionization experiment is an ongoing effort to measure the power spectrum from neutral hydrogen at high redshift. We have previously reported an upper limit of (70 mK)2 at wavenumbers of k ≈ 0.65 h Mpc−1 using a basic piecewise-linear foreground subtraction. In this paper, we explore the use of a singular value decomposition to remove foregrounds with fewer assumptions about the foreground structure. Using this method, we also quantify, for the first time, the signal loss due to the foreground filter and present new power spectra adjusted for this loss, providing a revised measurement of a 2σ upper limit at (248 mK)2 for k = 0.50 h Mpc−1. While this revised limit is larger than previously reported, we believe it to be more robust and still represents the best current constraint on reionization at z ≈ 8.6.},
	Author = {Paciga, Gregory and Albert, Joshua G. and Bandura, Kevin and Chang, Tzu-Ching and Gupta, Yashwant and Hirata, Christopher and Odegova, Julia and Pen, Ue-Li and Peterson, Jeffrey B. and Roy, Jayanta and Shaw, J. Richard and Sigurdson, Kris and Voytek, Tabitha},
	Date-Added = {2014-05-28 18:28:28 +0000},
	Date-Modified = {2014-05-28 18:28:42 +0000},
	Doi = {10.1093/mnras/stt753},
	Eprint = {http://mnras.oxfordjournals.org/content/433/1/639.full.pdf+html},
	Journal = {Monthly Notices of the Royal Astronomical Society},
	Number = {1},
	Pages = {639-647},
	Title = {A simulation-calibrated limit on the H i power spectrum from the GMRT Epoch of Reionization experiment},
	Url = {http://mnras.oxfordjournals.org/content/433/1/639.abstract},
	Volume = {433},
	Year = {2013},
	Bdsk-Url-1 = {http://mnras.oxfordjournals.org/content/433/1/639.abstract},
	Bdsk-Url-2 = {http://dx.doi.org/10.1093/mnras/stt753}}

@article{Offringa:2010,
	Abstract = {We describe and compare several post-correlation radio frequency interference (RFI) classification methods. As data sizes of observations grow with new and improved telescopes, the need for completely automated, robust methods for RFI mitigation is pressing. We investigated several classification methods and find that, for the data sets we used, the most accurate among them is the SumThreshold method. This is a new method formed from a combination of existing techniques, including a new way of thresholding. This iterative method estimates the astronomical signal by carrying out a surface fit in the time-frequency plane. With a theoretical accuracy of 95 per cent recognition and an approximately 0.1 per cent false probability rate in simple simulated cases, the method is in practice as good as the human eye in finding RFI. In addition, it is fast, robust, does not need a data model before it can be executed and works in almost all configurations with its default parameters. The method has been compared using simulated data with several other mitigation techniques, including one based upon the singular value decomposition of the time-frequency matrix, and has shown better results than the rest.},
	Author = {Offringa, A. R. and de Bruyn, A. G. and Biehl, M. and Zaroubi, S. and Bernardi, G. and Pandey, V. N.},
	Date-Added = {2014-05-22 21:33:11 +0000},
	Date-Modified = {2014-05-22 21:33:21 +0000},
	Doi = {10.1111/j.1365-2966.2010.16471.x},
	Eprint = {http://mnras.oxfordjournals.org/content/405/1/155.full.pdf+html},
	Journal = {Monthly Notices of the Royal Astronomical Society},
	Number = {1},
	Pages = {155-167},
	Title = {Post-correlation radio frequency interference classification methods},
	Url = {http://mnras.oxfordjournals.org/content/405/1/155.abstract},
	Volume = {405},
	Year = {2010},
	Bdsk-Url-1 = {http://mnras.oxfordjournals.org/content/405/1/155.abstract},
	Bdsk-Url-2 = {http://dx.doi.org/10.1111/j.1365-2966.2010.16471.x}}

@article{Jacobs:2013,
	Abstract = {We present a catalog of spectral measurements covering a 100-200 MHz band for 32 sources, derived from observations with a 64 antenna deployment of the Donald C. Backer Precision Array for Probing the Epoch of Reionization (PAPER) in South Africa. For transit telescopes such as PAPER, calibration of the primary beam is a difficult endeavor and errors in this calibration are a major source of error in the determination of source spectra. In order to decrease our reliance on an accurate beam calibration, we focus on calibrating sources in a narrow declination range from --46$\,^{\circ}$ to --40$\,^{\circ}$. Since sources at similar declinations follow nearly identical paths through the primary beam, this restriction greatly reduces errors associated with beam calibration, yielding a dramatic improvement in the accuracy of derived source spectra. Extrapolating from higher frequency catalogs, we derive the flux scale using a Monte Carlo fit across multiple sources that includes uncertainty from both catalog and measurement errors. Fitting spectral models to catalog data and these new PAPER measurements, we derive new flux models for Pictor A and 31 other sources at nearby declinations; 90% are found to confirm and refine a power-law model for flux density. Of particular importance is the new Pictor A flux model, which is accurate to 1.4% and shows that between 100 MHz and 2 GHz, in contrast with previous models, the spectrum of Pictor A is consistent with a single power law given by a flux at 150 MHz of 382 $\pm$ 5.4 Jy and a spectral index of --0.76 $\pm$ 0.01. This accuracy represents an order of magnitude improvement over previous measurements in this band and is limited by the uncertainty in the catalog measurements used to estimate the absolute flux scale. The simplicity and improved accuracy of Pictor A's spectrum make it an excellent calibrator in a band important for experiments seeking to measure 21 cm emission from the epoch of reionization.},
	Author = {Daniel C. Jacobs and Aaron R. Parsons and James E. Aguirre and Zaki Ali and Judd Bowman and Richard F. Bradley and Chris L. Carilli and David R. DeBoer and Matthew R. Dexter and Nicole E. Gugliucci and Pat Klima and Dave H. E. MacMahon and Jason R. Manley and David F. Moore and Jonathan C. Pober and Irina I. Stefan and William P. Walbrugh},
	Date-Added = {2014-05-22 15:32:24 +0000},
	Date-Modified = {2014-05-22 15:32:34 +0000},
	Journal = {The Astrophysical Journal},
	Number = {2},
	Pages = {108},
	Title = {A Flux Scale for Southern Hemisphere 21 cm Epoch of Reionization Experiments},
	Url = {http://stacks.iop.org/0004-637X/776/i=2/a=108},
	Volume = {776},
	Year = {2013},
	Bdsk-Url-1 = {http://stacks.iop.org/0004-637X/776/i=2/a=108}}

@article{Pober:2013,
	Abstract = {We present new observations with the Precision Array for Probing the Epoch of Reionization with the aim of measuring the properties of foreground emission for 21 cm epoch of reionization (EoR) experiments at 150 MHz. We focus on the footprint of the foregrounds in cosmological Fourier space to understand which modes of the 21 cm power spectrum will most likely be compromised by foreground emission. These observations confirm predictions that foregrounds can be isolated to a "wedge"-like region of two-dimensional ( k ⊥ , k ∥ )-space, creating a window for cosmological studies at higher k ∥ values. We also find that the emission extends past the nominal edge of this wedge due to spectral structure in the foregrounds, with this feature most prominent on the shortest baselines. Finally, we filter the data to retain only this "unsmooth" emission and image its specific k ∥ modes. The resultant images show an excess of power at the lowest modes, but no emission can be clearly localized to any one region of the sky. This image is highly suggestive that the most problematic foregrounds for 21 cm EoR studies will not be easily identifiable bright sources, but rather an aggregate of fainter emission.},
	Author = {Jonathan C. Pober and Aaron R. Parsons and James E. Aguirre and Zaki Ali and Richard F. Bradley and Chris L. Carilli and Dave DeBoer and Matthew Dexter and Nicole E. Gugliucci and Daniel C. Jacobs and Patricia J. Klima and Dave MacMahon and Jason Manley and David F. Moore and Irina I. Stefan and William P. Walbrugh},
	Date-Added = {2014-05-21 19:54:42 +0000},
	Date-Modified = {2015-02-18 17:36:06 +0000},
	Journal = {The Astrophysical Journal Letters},
	Keywords = {wedge},
	Number = {2},
	Pages = {L36},
	Title = {Opening the 21 cm Epoch of Reionization Window: Measurements of Foreground Isolation with PAPER},
	Url = {http://stacks.iop.org/2041-8205/768/i=2/a=L36},
	Volume = {768},
	Year = {2013},
	Bdsk-Url-1 = {http://stacks.iop.org/2041-8205/768/i=2/a=L36}}

@article{Mitchell:2008,
	Author = {Mitchell, D.A. and Greenhill, L.J. and Wayth, R.B. and Sault, R.J. and Lonsdale, C.J. and Cappallo, R.J. and Morales, M.F. and Ord, S.M.},
	Date-Added = {2014-04-08 15:57:35 +0000},
	Date-Modified = {2014-04-08 15:57:44 +0000},
	Doi = {10.1109/JSTSP.2008.2005327},
	Issn = {1932-4553},
	Journal = {Selected Topics in Signal Processing, IEEE Journal of},
	Keywords = {VHF antennas;array signal processing;dipole antenna arrays;interferometers;Australia;Murchison Widefield array;antenna array;array signal processing;frequency 80 MHz to 300 MHz;galactic emission;high-throughput real-time computing cluster;interferometric technique;ionospheric condition;low-frequency fixed dipole array;low-frequency radio array;next-generation radio interferometer;real-time calibration;real-time peeling implementation;Australia;Calibration;Dipole antennas;Image resolution;Instruments;Polarization;Radio interferometry;Signal synthesis;Structural beams;Tiles;Antenna arrays;array signal processing;calibration;dipole arrays;radio astronomy;radio interferometry},
	Month = {Oct},
	Number = {5},
	Pages = {707-717},
	Title = {Real-Time Calibration of the Murchison Widefield Array},
	Volume = {2},
	Year = {2008},
	Bdsk-Url-1 = {http://dx.doi.org/10.1109/JSTSP.2008.2005327}}

@article{Pail:2014,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2014arXiv1401.4172P},
	Archiveprefix = {arXiv},
	Author = {{Patil}, A.~H. and {Zaroubi}, S. and {Chapman}, E. and {Jeli{\'c}}, V. and {Harker}, G. and {Abdalla}, F.~B. and {Asad}, K.~M.~B. and {Bernardi}, G. and {Brentjens}, M.~A. and {de Bruyn}, A.~G. and {Bus}, S. and {Ciardi}, B. and {Daiboo}, S. and {Fernandez}, E.~R. and {Ghosh}, A. and {Jensen}, H. and {Kazemi}, S. and {Koopmans}, L.~V.~E. and {Labropoulos}, P. and {Mevius}, M. and {Martinez}, O. and {Mellema}, G. and {Offringa}, A.~R. and {Pandey}, V.~N. and {Schaye}, J. and {Thomas}, R.~M. and {Vedantham}, H.~K. and {Veligatla}, V. and {Wijnholds}, S.~J. and {Yatawatta}, S.},
	Date-Added = {2014-02-13 19:10:30 +0000},
	Date-Modified = {2014-02-13 19:10:42 +0000},
	Eprint = {1401.4172},
	Journal = {ArXiv e-prints},
	Keywords = {Astrophysics - Cosmology and Extragalactic Astrophysics},
	Month = jan,
	Primaryclass = {astro-ph.CO},
	Title = {{Constraining the epoch of reionization with the variance statistic: simulations of the LOFAR case}},
	Year = 2014}

@article{Datta:2010,
	Abstract = {The H I 21 cm transition line is expected to be an important probe into the cosmic dark ages and epoch of reionization. Foreground source removal is one of the principal challenges for the detection of this signal. This paper investigates the extragalactic point source contamination and how accurately bright sources ( ##IMG## [http://ej.iop.org/icons/Entities/gsim.gif] {gsim} 1 Jy) must be removed in order to detect 21 cm emission with upcoming radio telescopes such as the Murchison Widefield Array. We consider the residual contamination in 21 cm maps and power spectra due to position errors in the sky model for bright sources, as well as frequency-independent calibration errors. We find that a source position accuracy of 0.1 arcsec will suffice for detection of the H I power spectrum. For calibration errors, 0.05% accuracy in antenna gain amplitude is required in order to detect the cosmic signal. Both sources of subtraction error produce residuals that are localized to small angular scales, k ⊥ ##IMG## [http://ej.iop.org/icons/Entities/gsim.gif] {gsim} 0.05 Mpc --1 , in the two-dimensional power spectrum.},
	Author = {A. Datta and J. D. Bowman and C. L. Carilli},
	Date-Added = {2014-02-06 22:28:04 +0000},
	Date-Modified = {2014-08-31 18:45:13 +0000},
	Journal = {The Astrophysical Journal},
	Keywords = {wedge, simulation},
	Number = {1},
	Pages = {526},
	Title = {Bright Source Subtraction Requirements for Redshifted 21 cm Measurements},
	Url = {http://stacks.iop.org/0004-637X/724/i=1/a=526},
	Volume = {724},
	Year = {2010},
	Bdsk-Url-1 = {http://stacks.iop.org/0004-637X/724/i=1/a=526}}

@article{Liu:2009b,
	Abstract = {21-cm tomography is expected to be difficult in part because of serious foreground contamination. Previous studies have found that line-of-sight approaches are capable of cleaning foregrounds to an acceptable level on large spatial scales, but not on small spatial scales. In this paper, we introduce a Fourier space formalism for describing the line-of-sight methods, and use it to introduce an improved new method for 21-cm foreground cleaning. Heuristically, this method involves fitting foregrounds in Fourier space using weighted polynomial fits, with each pixel weighted according to its information content. We show that the new method reproduces the old one on large angular scales, and gives marked improvements on small scales at essentially no extra computational cost.},
	Author = {Liu, Adrian and Tegmark, Max and Bowman, Judd and Hewitt, Jacqueline and Zaldarriaga, Matias},
	Date-Added = {2014-02-04 22:12:04 +0000},
	Date-Modified = {2014-02-04 22:12:12 +0000},
	Doi = {10.1111/j.1365-2966.2009.15156.x},
	Eprint = {http://mnras.oxfordjournals.org/content/398/1/401.full.pdf+html},
	Journal = {Monthly Notices of the Royal Astronomical Society},
	Number = {1},
	Pages = {401-406},
	Title = {An improved method for 21-cm foreground removal},
	Url = {http://mnras.oxfordjournals.org/content/398/1/401.abstract},
	Volume = {398},
	Year = {2009},
	Bdsk-Url-1 = {http://mnras.oxfordjournals.org/content/398/1/401.abstract},
	Bdsk-Url-2 = {http://dx.doi.org/10.1111/j.1365-2966.2009.15156.x}}

@article{Liu:2009a,
	Abstract = {21-cm tomography is emerging as a promising probe of the cosmological dark ages and the epoch of reionization, as well as a tool for observational cosmology in general. However, serious sources of foreground contamination must be subtracted for experimental efforts to be viable. In this paper, we focus on the removal of unresolved extragalactic point sources with smooth spectra, and evaluate how the residual foreground contamination after cleaning depends on instrumental and algorithmic parameters. A crucial but often ignored complication is that the synthesized beam of an interferometer array shrinks towards higher frequency, causing complicated frequency structure in each sky pixel as `frizz' far from the beam centre contracts across unresolved radio sources. We find that current-generation experiments should none the less be able to clean out this point source contamination adequately, and quantify the instrumental and algorithmic design specifications required to meet this foreground challenge.},
	Author = {Liu, Adrian and Tegmark, Max and Zaldarriaga, Matias},
	Date-Added = {2014-02-04 22:10:47 +0000},
	Date-Modified = {2014-02-04 22:11:11 +0000},
	Doi = {10.1111/j.1365-2966.2009.14426.x},
	Eprint = {http://mnras.oxfordjournals.org/content/394/3/1575.full.pdf+html},
	Journal = {Monthly Notices of the Royal Astronomical Society},
	Number = {3},
	Pages = {1575-1587},
	Title = {Will point sources spoil 21-cm tomography?},
	Url = {http://mnras.oxfordjournals.org/content/394/3/1575.abstract},
	Volume = {394},
	Year = {2009},
	Bdsk-Url-1 = {http://mnras.oxfordjournals.org/content/394/3/1575.abstract},
	Bdsk-Url-2 = {http://dx.doi.org/10.1111/j.1365-2966.2009.14426.x}}

@article{Thyagarajan:2013,
	Abstract = {In this paper, we explore for the first time the relative magnitudes of three fundamental sources of uncertainty, namely, foreground contamination, thermal noise, and sample variance, in detecting the H I power spectrum from the epoch of reionization (EoR). We derive limits on the sensitivity of a Fourier synthesis telescope to detect EoR based on its array configuration and a statistical representation of images made by the instrument. We use the Murchison Widefield Array (MWA) configuration for our studies. Using a unified framework for estimating signal and noise components in the H I power spectrum, we derive an expression for and estimate the contamination from extragalactic point-like sources in three-dimensional k -space. Sensitivity for EoR H I power spectrum detection is estimated for different observing modes with MWA. With 1000 hr of observing on a single field using the 128 tile MWA, EoR detection is feasible (S/N >1 for k ##IMG## [http://ej.iop.org/icons/Entities/lsim.gif] {lsim} 0.8 Mpc --1 ). Bandpass shaping and refinements to the EoR window are found to be effective in containing foreground contamination, which makes the instrument tolerant to imaging errors. We find that for a given observing time, observing many independent fields of view does not offer an advantage over a single field observation when thermal noise dominates over other uncertainties in the derived power spectrum.},
	Author = {Nithyanandan Thyagarajan and N. Udaya Shankar and Ravi Subrahmanyan and Wayne Arcus and Gianni Bernardi and Judd D. Bowman and Frank Briggs and John D. Bunton and Roger J. Cappallo and Brian E. Corey and Ludi deSouza and David Emrich and Bryan M. Gaensler and Robert F. Goeke and Lincoln J. Greenhill and Bryna J. Hazelton and David Herne and Jacqueline N. Hewitt and Melanie Johnston-Hollitt and David L. Kaplan and Justin C. Kasper and Barton B. Kincaid and Ronald Koenig and Eric Kratzenberg and Colin J. Lonsdale and Mervyn J. Lynch and S. Russell McWhirter and Daniel A. Mitchell and Miguel F. Morales and Edward H. Morgan and Divya Oberoi and Stephen M. Ord and Joseph Pathikulangara and Ronald A. Remillard and Alan E. E. Rogers and D. Anish Roshi and Joseph E. Salah and Robert J. Sault and K. S. Srivani and Jamie B. Stevens and Prabu Thiagaraj and Steven J. Tingay and Randall B. Wayth and Mark Waterson and Rachel L. Webster and Alan R. Whitney and Andrew J. Williams and Christopher L. Williams and J. Stuart B. Wyithe},
	Date-Added = {2014-02-04 22:04:48 +0000},
	Date-Modified = {2014-08-31 18:50:01 +0000},
	Journal = {The Astrophysical Journal},
	Keywords = {wedge},
	Number = {1},
	Pages = {6},
	Title = {A Study of Fundamental Limitations to Statistical Detection of Redshifted H I from the Epoch of Reionization},
	Url = {http://stacks.iop.org/0004-637X/776/i=1/a=6},
	Volume = {776},
	Year = {2013},
	Bdsk-Url-1 = {http://stacks.iop.org/0004-637X/776/i=1/a=6}}

@article{Sullivan:2012,
	Abstract = {We introduce the Fast Holographic Deconvolution method for analyzing interferometric radio data. Our new method is an extension of A-projection/software-holography/forward modeling analysis techniques and shares their precision deconvolution and wide-field polarimetry, while being significantly faster than current implementations that use full direction-dependent antenna gains. Using data from the MWA 32 antenna prototype, we demonstrate the effectiveness and precision of our new algorithm. Fast Holographic Deconvolution may be particularly important for upcoming 21 cm cosmology observations of the Epoch of Reionization and Dark Energy where foreground subtraction is intimately related to the precision of the data reduction.},
	Author = {I. S. Sullivan and M. F. Morales and B. J. Hazelton and W. Arcus and D. Barnes and G. Bernardi and F. H. Briggs and J. D. Bowman and J. D. Bunton and R. J. Cappallo and B. E. Corey and A. Deshpande and L. deSouza and D. Emrich and B. M. Gaensler and R. Goeke and L. J. Greenhill and D. Herne and J. N. Hewitt and M. Johnston-Hollitt and D. L. Kaplan and J. C. Kasper and B. B. Kincaid and R. Koenig and E. Kratzenberg and C. J. Lonsdale and M. J. Lynch and S. R. McWhirter and D. A. Mitchell and E. Morgan and D. Oberoi and S. M. Ord and J. Pathikulangara and T. Prabu and R. A. Remillard and A. E. E. Rogers and A. Roshi and J. E. Salah and R. J. Sault and N. Udaya Shankar and K. S. Srivani and J. Stevens and R. Subrahmanyan and S. J. Tingay and R. B. Wayth and M. Waterson and R. L. Webster and A. R. Whitney and A. Williams and C. L. Williams and J. S. B. Wyithe},
	Date-Added = {2014-01-28 20:46:31 +0000},
	Date-Modified = {2014-01-28 20:46:41 +0000},
	Journal = {The Astrophysical Journal},
	Number = {1},
	Pages = {17},
	Title = {Fast Holographic Deconvolution: A New Technique for Precision Radio Interferometry},
	Url = {http://stacks.iop.org/0004-637X/759/i=1/a=17},
	Volume = {759},
	Year = {2012},
	Bdsk-Url-1 = {http://stacks.iop.org/0004-637X/759/i=1/a=17}}

@article{Parsons:2012b,
	Author = {Parsons, Aaron R and Pober, Jonathan C and Aguirre, James E and Carilli, Christopher L and Jacobs, Daniel C and Moore, David F},
	Date-Added = {2014-01-16 20:13:23 +0000},
	Date-Modified = {2015-02-18 17:36:01 +0000},
	Journal = {The Astrophysical Journal},
	Number = {2},
	Pages = {165},
	Publisher = {IOP Publishing},
	Title = {A per-baseline, delay-spectrum technique for accessing the 21 cm cosmic reionization signature},
	Volume = {756},
	Year = {2012}}

@article{Hazelton:2013,
	Abstract = {The primary challenge for experiments measuring the neutral hydrogen power spectrum from the epoch of reionization (EoR) is mode-mixing effects, where foregrounds from very bright astrophysical sources interact with the instrument to contaminate the EoR signal. In this paper, we identify a new type of mode mixing that occurs when measurements from non-identical baselines are combined for increased power spectrum sensitivity. This multi-baseline effect dominates the mode-mixing power in our simulations and can contaminate the EoR window, an area in Fourier space previously identified to be relatively free of foreground power.},
	Author = {Bryna J. Hazelton and Miguel F. Morales and Ian S. Sullivan},
	Date-Added = {2014-01-16 19:23:41 +0000},
	Date-Modified = {2014-08-31 18:45:43 +0000},
	Journal = {The Astrophysical Journal},
	Keywords = {wedge},
	Number = {2},
	Pages = {156},
	Title = {The Fundamental Multi-baseline Mode-mixing Foreground in 21 cm Epoch of Reionization Observations},
	Url = {http://stacks.iop.org/0004-637X/770/i=2/a=156},
	Volume = {770},
	Year = {2013},
	Bdsk-Url-1 = {http://stacks.iop.org/0004-637X/770/i=2/a=156}}

@article{Bowman:2013,
	Author = {Bowman,Judd D. and Cairns,Iver and Kaplan,David L. and Murphy,Tara and Oberoi,Divya and Staveley-Smith,Lister and Arcus,Wayne and Barnes,David G. and Bernardi,Gianni and Briggs,Frank H. and Brown,Shea and Bunton,John D. and Burgasser,Adam J. and Cappallo,Roger J. and Chatterjee,Shami and Corey,Brian E. and Coster,Anthea and Deshpande,Avinash and deSouza,Ludi and Emrich,David and Erickson,Philip and Goeke,Robert F. and Gaensler,B. M. and Greenhill,Lincoln J. and Harvey-Smith,Lisa and Hazelton,Bryna J. and Herne,David and Hewitt,Jacqueline N. and Johnston-Hollitt,Melanie and Kasper,Justin C. and Kincaid,Barton B. and Koenig,Ronald and Kratzenberg,Eric and Lonsdale,Colin J. and Lynch,Mervyn J. and Matthews,Lynn D. and McWhirter,S. Russell and Mitchell,Daniel A. and Morales,Miguel F. and Morgan,Edward H. and Ord,Stephen M. and Pathikulangara,Joseph and Prabu,Thiagaraj and Remillard,Ronald A. and Robishaw,Timothy and Rogers,Alan E. E. and Roshi,Anish A. and Salah,Joseph E. and Sault,Robert J. and Shankar,N. Udaya and Srivani,K. S. and Stevens,Jamie B. and Subrahmanyan,Ravi and Tingay,Steven J. and Wayth,Randall B. and Waterson,Mark and Webster,Rachel L. and Whitney,Alan R. and Williams,Andrew J. and Williams,Christopher L. and Wyithe,J. Stuart B.},
	Date-Added = {2014-01-15 20:42:24 +0000},
	Date-Modified = {2014-01-15 20:42:32 +0000},
	Doi = {10.1017/pas.2013.009},
	Issn = {1448-6083},
	Journal = {PASA - Publications of the Astronomical Society of Australia},
	Month = {1},
	Title = {Science with the Murchison Widefield Array},
	Url = {http://journals.cambridge.org/article_S132335801300009X},
	Volume = {30},
	Year = {2013},
	Bdsk-Url-1 = {http://journals.cambridge.org/article_S132335801300009X},
	Bdsk-Url-2 = {http://dx.doi.org/10.1017/pas.2013.009}}

@article{Hoffman:2013,
	Author = {Hoffman, Matthew R. and Noel, Thomas W. and Auchter, Carolyn and Jayakumar, Anupriya and Williams, Spencer R. and Blinov, Boris B. and Fortson, E. N.},
	Date-Added = {2013-11-20 17:26:09 +0000},
	Date-Modified = {2013-11-20 17:26:19 +0000},
	Doi = {10.1103/PhysRevA.88.025401},
	Issue = {2},
	Journal = {Phys. Rev. A},
	Month = {Aug},
	Numpages = {4},
	Pages = {025401},
	Publisher = {American Physical Society},
	Title = {Radio-frequency-spectroscopy measurement of the Land\'e ${g}_{J}$ factor of the $5{D}_{5/2}$ state of Ba${}^{+}$ with a single trapped ion},
	Url = {http://link.aps.org/doi/10.1103/PhysRevA.88.025401},
	Volume = {88},
	Year = {2013},
	Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevA.88.025401},
	Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevA.88.025401}}

@inproceedings{Cornwell:2005,
	Author = {Cornwell, T.J. and Golap, K. and Bhatnagar, S.},
	Booktitle = {Acoustics, Speech, and Signal Processing, 2005. Proceedings. (ICASSP '05). IEEE International Conference on},
	Date-Added = {2013-07-29 19:21:53 +0000},
	Date-Modified = {2013-07-29 19:22:15 +0000},
	Doi = {10.1109/ICASSP.2005.1416440},
	Issn = {1520-6149},
	Keywords = {antenna arrays;array signal processing;astronomy computing;image processing;radioastronomical techniques;radioastronomy;radiotelescopes;sensitivity;Square Kilometre Array;W projection;international consortium;noncoplanar baselines aberration;radio astronomy;reconfigurable computing;synthesis radio telescopes;wide field imaging;Costs;Equations;Fourier transforms;Observatories;Optical distortion;Optical interferometry;Phased arrays;RF signals;Radio astronomy;Virtual manufacturing},
	Pages = {v/861-v/864 Vol. 5},
	Title = {Wide field imaging problems in radio astronomy},
	Volume = {5},
	Year = {2005},
	Bdsk-Url-1 = {http://dx.doi.org/10.1109/ICASSP.2005.1416440}}

@article{Wyithe:2007,
	Abstract = {Spatial dependence in the statistics of redshifted 21-cm fluctuations promises to provide the most powerful probe of the reionization epoch. In this paper we consider the second and third moments of the redshifted 21-cm intensity distribution using a simple model that accounts for galaxy bias during the reionization process. We demonstrate that skewness in redshifted 21-cm maps should be substantial throughout the reionization epoch and on all angular scales, owing to the effects of galaxy bias which leads to early reionization in overdense regions of the intergalactic medium (IGM). The variance (or power spectrum) of 21-cm fluctuations will exhibit a minimum in redshift part way through the reionization process, when the global ionization fraction is around 50 per cent. This minimum is generic, and is due to the transition from 21-cm intensity being dominated by overdense to underdense regions as reionization progresses. We show that the details of the reionization history, including the presence of radiative feedback are encoded in the evolution of the autocorrelation and skewness functions with redshift and mean IGM neutral fraction. The amplitudes of fluctuations are particularly sensitive to the masses of ionizing sources, and vary by an order of magnitude for astrophysically plausible models. We discuss the detection of skewness by first-generation instruments, and conclude that the Mileura Wide-field Array--Low-Frequency Demonstrator will have sufficient sensitivity to detect skewness on a range of angular scales at redshifts near the end of reionization, while a subsequent instrument of 10 times the collecting area could map out the evolution of skewness in detail. The observation of a minimum in variance during the reionization history, and the detection of skewness would both provide important confirmation of the cosmological origin of redshifted 21-cm intensity fluctuations.},
	Author = {Wyithe, J. Stuart B. and Morales, Miguel F.},
	Date-Added = {2013-05-31 18:40:13 +0000},
	Date-Modified = {2013-05-31 18:40:25 +0000},
	Doi = {10.1111/j.1365-2966.2007.12048.x},
	Eprint = {http://mnras.oxfordjournals.org/content/379/4/1647.full.pdf+html},
	Journal = {Monthly Notices of the Royal Astronomical Society},
	Number = {4},
	Pages = {1647-1657},
	Title = {Biased reionization and non-Gaussianity in redshifted 21-cm intensity maps of the reionization epoch},
	Url = {http://mnras.oxfordjournals.org/content/379/4/1647.abstract},
	Volume = {379},
	Year = {2007},
	Bdsk-Url-1 = {http://mnras.oxfordjournals.org/content/379/4/1647.abstract},
	Bdsk-Url-2 = {http://dx.doi.org/10.1111/j.1365-2966.2007.12048.x}}

@article{Zahn:2007,
	Abstract = {We present results from a large volume simulation of hydrogen reionization. We combine 3D radiative transfer calculations and an N -body simulation, describing structure formation in the intergalactic medium, to detail the growth of H II regions around high-redshift galaxies. Our simulation tracks 1024 3 dark matter particles, in a box of comoving side length 65.6 Mpc h -1 . This large volume allows us to accurately characterize the size distribution of H II regions throughout most of the reionization process. At the same time, our simulation resolves many of the small galaxies likely responsible for reionization. It confirms a picture anticipated by analytic models: H II regions grow collectively around highly clustered sources and have a well-defined characteristic size, which evolves from a sub-Mpc scale at the beginning of reionization to R > 10 Mpc toward the end. We present a detailed statistical description of our results and compare them with a numerical scheme based on the analytic model by Furlanetto and coworkers. We find that the analytic calculation reproduces the size distribution of H II regions and the 21 cm power spectrum of the radiative transfer simulation remarkably well. The ionization field from the simulation, however, has more small-scale structure than the analytic calculation, owing to Poisson scatter in the simulated abundance of galaxies on small scales. We propose and validate a simple scheme to incorporate this scatter into our calculations. Our results suggest that analytic calculations are sufficiently accurate to aid in predicting and interpreting the results of future 21 cm surveys. In particular, our fast numerical scheme is useful for forecasting constraints from future 21 cm surveys and in constructing mock surveys to test data analysis procedures.},
	Author = {Oliver Zahn and Adam Lidz and Matthew McQuinn and Suvendra Dutta and Lars Hernquist and Matias Zaldarriaga and Steven R. Furlanetto},
	Date-Added = {2013-05-06 16:44:39 +0000},
	Date-Modified = {2013-05-06 16:44:39 +0000},
	Journal = {The Astrophysical Journal},
	Number = {1},
	Pages = {12},
	Title = {Simulations and Analytic Calculations of Bubble Growth during Hydrogen Reionization},
	Url = {http://stacks.iop.org/0004-637X/654/i=1/a=12},
	Volume = {654},
	Year = {2007},
	Bdsk-Url-1 = {http://stacks.iop.org/0004-637X/654/i=1/a=12}}

@article{Malloy:2013,
	Abstract = {One of the most promising approaches for studying reionization is to use the redshifted 21 cm line. Early generations of redshifted 21 cm surveys will not, however, have the sensitivity to make detailed maps of the reionization process, and will instead focus on statistical measurements. Here, we show that it may nonetheless be possible to directly identify ionized regions in upcoming data sets by applying suitable filters to the noisy data. The locations of prominent minima in the filtered data correspond well with the positions of ionized regions. In particular, we corrupt semi-numeric simulations of the redshifted 21 cm signal during reionization with thermal noise at the level expected for a 500 antenna tile version of the Murchison Widefield Array (MWA), and mimic the degrading effects of foreground cleaning. Using a matched filter technique, we find that the MWA should be able to directly identify ionized regions despite the large thermal noise. In a plausible fiducial model in which ~20% of the volume of the universe is neutral at z ~ 7, we find that a 500-tile MWA may directly identify as many as ~150 ionized regions in a 6 MHz portion of its survey volume and roughly determine the size of each of these regions. This may, in turn, allow interesting multi-wavelength follow-up observations, comparing galaxy properties inside and outside of ionized regions. We discuss how the optimal configuration of radio antenna tiles for detecting ionized regions with a matched filter technique differs from the optimal design for measuring power spectra. These considerations have potentially important implications for the design of future redshifted 21 cm surveys.},
	Author = {Matthew Malloy and Adam Lidz},
	Date-Added = {2013-04-29 19:37:02 +0000},
	Date-Modified = {2013-05-02 14:16:12 +0000},
	Journal = {The Astrophysical Journal},
	Number = {1},
	Pages = {68},
	Title = {Identifying Ionized Regions in Noisy Redshifted 21 cm Data Sets},
	Url = {http://stacks.iop.org/0004-637X/767/i=1/a=68},
	Volume = {767},
	Year = {2013},
	Bdsk-Url-1 = {http://stacks.iop.org/0004-637X/767/i=1/a=68}}

@article{Dillon:2013,
	Author = {Dillon, Joshua S. and Liu, Adrian and Tegmark, Max},
	Date-Added = {2013-04-26 16:44:18 +0000},
	Date-Modified = {2013-04-26 16:44:18 +0000},
	Doi = {10.1103/PhysRevD.87.043005},
	Issue = {4},
	Journal = {Phys. Rev. D},
	Month = {Feb},
	Numpages = {30},
	Pages = {043005},
	Publisher = {American Physical Society},
	Title = {A fast method for power spectrum and foreground analysis for 21~cm cosmology},
	Url = {http://link.aps.org/doi/10.1103/PhysRevD.87.043005},
	Volume = {87},
	Year = {2013},
	Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevD.87.043005},
	Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevD.87.043005}}

@article{Vedantham:2012,
	Abstract = {Tomography of redshifted 21 cm transition from neutral hydrogen using Fourier synthesis telescopes is a promising tool to study the Epoch of Reionization (EoR). Limiting the confusion from Galactic and extragalactic foregrounds is critical to the success of these telescopes. The instrumental response or the point-spread function (PSF) of such telescopes is inherently three dimensional with frequency mapping to the line-of-sight (LOS) distance. EoR signals will necessarily have to be detected in data where continuum confusion persists; therefore, it is important that the PSF has acceptable frequency structure so that the residual foreground does not confuse the EoR signature. This paper aims to understand the three-dimensional PSF and foreground contamination in the same framework. We develop a formalism to estimate the foreground contamination along frequency, or equivalently LOS dimension, and establish a relationship between foreground contamination in the image plane and visibility weights on the Fourier plane. We identify two dominant sources of LOS foreground contamination{\^O}{\o}Ω"PSF contamination" and "gridding contamination." We show that PSF contamination is localized in LOS wavenumber space, beyond which there potentially exists an "EoR window" with negligible foreground contamination where we may focus our efforts to detect EoR. PSF contamination in this window may be substantially reduced by judicious choice of a frequency window function. Gridding and imaging algorithms create additional gridding contamination and we propose a new imaging algorithm using the Chirp Z Transform that significantly reduces this contamination. Finally, we demonstrate the analytical relationships and the merit of the new imaging algorithm for the case of imaging with the Murchison Widefield Array.},
	Author = {Harish Vedantham and N. Udaya Shankar and Ravi Subrahmanyan},
	Date-Added = {2013-04-05 21:06:44 +0000},
	Date-Modified = {2014-08-31 18:47:28 +0000},
	Journal = {The Astrophysical Journal},
	Keywords = {window},
	Number = {2},
	Pages = {176},
	Title = {Imaging the Epoch of Reionization: Limitations from Foreground Confusion and Imaging Algorithms},
	Url = {http://stacks.iop.org/0004-637X/745/i=2/a=176},
	Volume = {745},
	Year = {2012},
	Bdsk-Url-1 = {http://stacks.iop.org/0004-637X/745/i=2/a=176}}

@article{Trott:2012,
	Abstract = {Precise subtraction of foreground sources is crucial for detecting and estimating 21 cm H I signals from the Epoch of Reionization (EoR). We quantify how imperfect point-source subtraction due to limitations of the measurement data set yields structured residual signal in the data set. We use the Cramer-Rao lower bound, as a metric for quantifying the precision with which a parameter may be measured, to estimate the residual signal in a visibility data set due to imperfect point-source subtraction. We then propagate these residuals into two metrics of interest for 21 cm EoR experiments‚{\"A}{\^\i}the angular power spectrum and two-dimensional power spectrum‚{\"A}{\^\i}using a combination of full analytic covariant derivation, analytic variant derivation, and covariant Monte Carlo simulations. This methodology differs from previous work in two ways: (1) it uses information theory to set the point-source position error, rather than assuming a global rms error, and (2) it describes a method for propagating the errors analytically, thereby obtaining the full correlation structure of the power spectra. The methods are applied to two upcoming low-frequency instruments that are proposing to perform statistical EoR experiments: the Murchison Widefield Array and the Precision Array for Probing the Epoch of Reionization. In addition to the actual antenna configurations, we apply the methods to minimally redundant and maximally redundant configurations. We find that for peeling sources above 1 Jy, the amplitude of the residual signal, and its variance, will be smaller than the contribution from thermal noise for the observing parameters proposed for upcoming EoR experiments, and that optimal subtraction of bright point sources will not be a limiting factor for EoR parameter estimation. We then use the formalism to provide an ab initio analytic derivation motivating the "wedge" feature in the two-dimensional power spectrum, complementing previous discussion in the literature.},
	Author = {Cathryn M. Trott and Randall B. Wayth and Steven J. Tingay},
	Date-Added = {2013-04-05 21:06:23 +0000},
	Date-Modified = {2014-08-31 18:47:17 +0000},
	Journal = {The Astrophysical Journal},
	Keywords = {wedge},
	Number = {1},
	Pages = {101},
	Title = {The Impact of Point-source Subtraction Residuals on 21 cm Epoch of Reionization Estimation},
	Url = {http://stacks.iop.org/0004-637X/757/i=1/a=101},
	Volume = {757},
	Year = {2012},
	Bdsk-Url-1 = {http://stacks.iop.org/0004-637X/757/i=1/a=101}}

@article{Trac:2007,
	Abstract = {We present a new hybrid code for large-volume, high-resolution simulations of cosmic reionization, which utilizes an N -body algorithm for dark matter, physically motivated prescriptions for baryons and star formation, and an adaptive ray-tracing algorithm for radiative transfer of ionizing photons. Two test simulations, each with 3 billion particles and 400 million rays in a 50 Mpc h -1 box, have been run to give initial results. Halos are resolved down to virial temperatures of 10 4 K for the redshift range of interest in order to robustly model star formation and clumping factors. This is essential to correctly account for ionization and recombination processes. We find that the halos and sources are strongly biased with respect to the underlying dark matter, re-enforcing the requirement of large simulation boxes to minimize cosmic variance and to obtain a qualitatively correct picture of reionization. We model the stellar initial mass function (IMF) by following the spatially dependent gas metallicity evolution, and distinguish between the first generation, Population III (PopIII) stars and the second generation, Population II (PopII) stars. The PopIII stars with a top-heavy IMF produce an order of magnitude more ionizing photons at high redshifts z ##IMG## [http://ej.iop.org/icons/Entities/gtrsim.gif] {gtrsim} 10, resulting in a more extended reionization. In our simulations, complete overlap of H II regions occurs at z ≈ 6.5, and the computed mass- and volume-weighted residual H I fractions at 5 ##IMG## [http://ej.iop.org/icons/Entities/lesssim.gif] {lesssim} z ##IMG## [http://ej.iop.org/icons/Entities/lesssim.gif] {lesssim} 6.5 are both in good agreement with high-redshift quasar absorption measurements from the Sloan Digital Sky Survey (SDSS). The values for the Thomson optical depth are consistent within 1 - ? of the current best-fit value from third-year Wilkinson Microwave Anisotropy Probe ( WMAP ) results.},
	Author = {Hy Trac and Renyue Cen},
	Date-Added = {2013-04-05 21:06:07 +0000},
	Date-Modified = {2013-04-05 21:06:07 +0000},
	Journal = {The Astrophysical Journal},
	Number = {1},
	Pages = {1},
	Title = {Radiative Transfer Simulations of Cosmic Reionization. I. Methodology and Initial Results},
	Url = {http://stacks.iop.org/0004-637X/671/i=1/a=1},
	Volume = {671},
	Year = {2007},
	Bdsk-Url-1 = {http://stacks.iop.org/0004-637X/671/i=1/a=1}}

@article{Morales:2005b,
	Abstract = {Recent theoretical developments concerning the plasma physics near the GRB blast wave have renewed interest in the properties of impulsive low frequency radio emission from GRBs. Prompt coherent low frequency radio emission would provide a unique probe of the plasma conditions near the blast wave during the period of peak particle acceleration and gamma ray emission. In this paper we introduce the GRB All-sky Spectrometer Experiment (GASE). This experiment will make use of advances in digital technology to record 4 MHz of bandwidth in eight 30 MHz dipole antennas for two hours after a Swift or HETE-2 trigger is received. Due to the long dispersion delay at low frequencies, this allows contemporaneous measurements of the gamma ray and radio emission. The high spectral resolution of GASE will allow the predicted prompt 30 MHz signal from GRBs to be fully de-dispersed and identified. The combination of high spectral resolution, full-sky imaging, and (if required) geographically separated detectors will also provide stringent rejection of radio interference.},
	Author = {Miguel F Morales and Jacqueline N Hewitt and Justin C Kasper and B Lane and Judd D Bowman and P. S Ray and Roger J Cappallo},
	Date-Added = {2013-04-05 21:03:08 +0000},
	Date-Modified = {2013-04-05 21:03:08 +0000},
	Journal = {From Clark Lake to the Long Wavelength Array: Bill Erickson's Radio Science ASP Conference Series},
	Local-Url = {file://localhost/Volumes/miguel.f.morales/Documents/Papers/2005/Morales/From%20Clark%20Lake%20to%20the%20Long%20Wavelength%20Array%20Bill%20Erickson's%20Radio%20Science%20ASP%20Conference%20Series%202005%20Morales.pdf},
	Month = {Nov},
	Pages = {512},
	Pmid = {2005ASPC..345..512M},
	Rating = {0},
	Read = {Yes},
	Title = {The GRB All-sky Spectrometer Experiment (GASE)},
	Uri = {papers://DFE1617F-A133-478C-B28B-7AFF8D228C27/Paper/p168},
	Url = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005ASPC..345..512M&link_type=ABSTRACT},
	Volume = {345},
	Year = {2005},
	Bdsk-Url-1 = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005ASPC..345..512M&link_type=ABSTRACT}}

@article{Morales:2008,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2011PASP..123.1265M},
	Archiveprefix = {arXiv},
	Author = {{Morales}, M.~F.},
	Date-Added = {2013-04-05 21:02:17 +0000},
	Date-Modified = {2013-05-14 16:39:46 +0000},
	Eprint = {0812.3669},
	Journal = {ArXiv e-prints},
	Keywords = {Astrophysics},
	Month = dec,
	Title = {{Enabling Next Generation Dark Energy and Epoch of Reionization Radio Observatories with the MOFF Correlator}},
	Year = 2008,
	Bdsk-Url-1 = {http://adsabs.harvard.edu/abs/2011PASP..123.1265M}}

@article{Wyithe:2008b,
	Author = {Wyithe, J. Stuart B. and Loeb, Abraham and Geil, Paul M.},
	Date-Added = {2013-04-05 21:01:54 +0000},
	Date-Modified = {2013-04-05 21:01:54 +0000},
	Doi = {10.1111/j.1365-2966.2007.12631.x},
	Issn = {1365-2966},
	Journal = {Monthly Notices of the Royal Astronomical Society},
	Keywords = {galaxies: high-redshift, intergalactic medium, cosmology: theory, diffuse radiation, large-scale structure of Universe},
	Number = {3},
	Pages = {1195--1209},
	Publisher = {Blackwell Publishing Ltd},
	Title = {Baryonic acoustic oscillations in 21-cm emission: a probe of dark energy out to high redshifts},
	Url = {http://dx.doi.org/10.1111/j.1365-2966.2007.12631.x},
	Volume = {383},
	Year = {2008},
	Bdsk-Url-1 = {http://dx.doi.org/10.1111/j.1365-2966.2007.12631.x}}

@article{Wyithe:2008,
	Author = {Wyithe, J. Stuart B. and Loeb, Abraham},
	Date-Added = {2013-04-05 21:01:22 +0000},
	Date-Modified = {2013-04-05 21:01:22 +0000},
	Doi = {10.1111/j.1365-2966.2007.12568.x},
	Issn = {1365-2966},
	Journal = {Monthly Notices of the Royal Astronomical Society},
	Keywords = {galaxies: high-redshift, intergalactic medium, cosmology: theory, diffuse radiation, large-scale structure of Universe},
	Number = {2},
	Pages = {606--614},
	Publisher = {Blackwell Publishing Ltd},
	Title = {Fluctuations in 21-cm emission after reionization},
	Url = {http://dx.doi.org/10.1111/j.1365-2966.2007.12568.x},
	Volume = {383},
	Year = {2008},
	Bdsk-Url-1 = {http://dx.doi.org/10.1111/j.1365-2966.2007.12568.x}}

@article{Tegmark:1997b,
	Author = {Tegmark, M.},
	Date-Added = {2013-04-05 21:00:51 +0000},
	Date-Modified = {2013-04-05 21:00:51 +0000},
	Doi = {10.1103/PhysRevD.55.5895},
	Journal = {Phys. Rev. D},
	Month = {May},
	Number = {10},
	Numpages = {12},
	Pages = {5895--5907},
	Publisher = {American Physical Society},
	Title = {How to measure CMB power spectra without losing information},
	Volume = {55},
	Year = {1997},
	Bdsk-Url-1 = {http://dx.doi.org/10.1103/PhysRevD.55.5895}}

@article{Tegmark:1997,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/1997ApJ...480L..87T},
	Author = {{Tegmark}, M.},
	Date-Added = {2013-04-05 21:00:25 +0000},
	Date-Modified = {2013-04-05 21:00:25 +0000},
	Doi = {10.1086/310631},
	Eprint = {arXiv:astro-ph/9611130},
	Journal = {ApJ},
	Keywords = {COSMOLOGY: COSMIC MICROWAVE BACKGROUND, METHODS: DATA ANALYSIS},
	Month = may,
	Pages = {L87},
	Title = {{How to Make Maps from Cosmic Microwave Background Data without Losing Information}},
	Volume = 480,
	Year = 1997,
	Bdsk-Url-1 = {http://dx.doi.org/10.1086/310631}}

@inproceedings{Romney:1999,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/1999ASPC..180...57R},
	Author = {{Romney}, J.~D.},
	Booktitle = {Synthesis Imaging in Radio Astronomy II},
	Date-Added = {2013-04-05 21:00:02 +0000},
	Date-Modified = {2013-04-05 21:00:02 +0000},
	Editor = {{G.~B.~Taylor, C.~L.~Carilli, \& R.~A.~Perley}},
	Page = {57},
	Series = {Astronomical Society of the Pacific Conference Series},
	Title = {{Cross Correlators}},
	Volume = 180,
	Year = 1999}

@article{Parsons:2008,
	Author = {Parsons, A. and others},
	Copyright = {Copyright ¬{\copyright} 2008 The University of Chicago Press},
	Date-Added = {2013-04-05 20:59:20 +0000},
	Date-Modified = {2013-04-05 20:59:20 +0000},
	Issn = {00046280},
	Journal = {Publications of the Astronomical Society of the Pacific},
	Jstor_Articletype = {research-article},
	Jstor_Formatteddate = {November 2008},
	Language = {English},
	Number = {873},
	Pages = {pp. 1207-1221},
	Publisher = {The University of Chicago Press on behalf of the Astronomical Society of the Pacific},
	Title = {A Scalable Correlator Architecture Based on Modular FPGA Hardware, Reuseable Gateware, and Data Packetization},
	Url = {http://www.jstor.org/stable/10.1086/593053},
	Volume = {120},
	Year = {2008},
	Bdsk-Url-1 = {http://www.jstor.org/stable/10.1086/593053}}

@article{Morales_Wyithe:2010,
	Author = {Morales, M. F. and Wyithe, J. S. B.},
	Date-Added = {2013-04-05 20:58:56 +0000},
	Date-Modified = {2015-02-05 18:48:01 +0000},
	Doi = {10.1146/annurev-astro-081309-130936},
	Eprint = {http://www.annualreviews.org/doi/pdf/10.1146/annurev-astro-081309-130936},
	Journal = {Annual Review of Astronomy and Astrophysics},
	Keywords = {review,observational},
	Number = {1},
	Pages = {127-171},
	Title = {Reionization and Cosmology with 21-cm Fluctuations},
	Url = {http://www.annualreviews.org/doi/abs/10.1146/annurev-astro-081309-130936},
	Volume = {48},
	Year = {2010},
	Bdsk-Url-1 = {http://www.annualreviews.org/doi/abs/10.1146/annurev-astro-081309-130936},
	Bdsk-Url-2 = {http://dx.doi.org/10.1146/annurev-astro-081309-130936}}

@article{Morales:2009,
	Author = {Morales, M. F. and Matejek, M.},
	Date-Added = {2013-04-05 20:58:25 +0000},
	Date-Modified = {2013-04-05 20:58:25 +0000},
	Doi = {10.1111/j.1365-2966.2009.15537.x},
	Issn = {1365-2966},
	Journal = {Monthly Notices of the Royal Astronomical Society},
	Keywords = {instrumentation: interferometers, techniques: interferometric, cosmology: miscellaneous},
	Number = {4},
	Pages = {1814--1820},
	Publisher = {Blackwell Publishing Ltd},
	Title = {Software holography: interferometric data analysis for the challenges of next generation observatories},
	Url = {http://dx.doi.org/10.1111/j.1365-2966.2009.15537.x},
	Volume = {400},
	Year = {2009},
	Bdsk-Url-1 = {http://dx.doi.org/10.1111/j.1365-2966.2009.15537.x}}

@article{Mao:2008,
	Author = {Mao, Y. and Tegmark, M. and McQuinn, M. and Zaldarriaga, M. and Zahn, O.},
	Date-Added = {2013-04-05 20:57:46 +0000},
	Date-Modified = {2013-04-05 20:57:46 +0000},
	Doi = {10.1103/PhysRevD.78.023529},
	Journal = {Phys. Rev. D},
	Month = {Jul},
	Number = {2},
	Numpages = {22},
	Pages = {023529},
	Publisher = {American Physical Society},
	Title = {How accurately can 21 cm tomography constrain cosmology?},
	Volume = {78},
	Year = {2008},
	Bdsk-Url-1 = {http://dx.doi.org/10.1103/PhysRevD.78.023529}}

@article{Loeb:2008,
	Author = {Loeb, A. and Wyithe, J. S. B.},
	Date-Added = {2013-04-05 20:57:10 +0000},
	Date-Modified = {2013-04-05 20:57:10 +0000},
	Doi = {10.1103/PhysRevLett.100.161301},
	Journal = {Phys. Rev. Lett.},
	Month = {Apr},
	Number = {16},
	Numpages = {4},
	Pages = {161301},
	Publisher = {American Physical Society},
	Title = {Possibility of Precise Measurement of the Cosmological Power Spectrum with a Dedicated Survey of 21 cm Emission after Reionization},
	Volume = {100},
	Year = {2008},
	Bdsk-Url-1 = {http://dx.doi.org/10.1103/PhysRevLett.100.161301}}

@article{Carlson:2000,
	Author = {Carlson, B. R. and Dewdney, P. E.},
	Date-Added = {2013-04-05 20:56:53 +0000},
	Date-Modified = {2013-04-05 20:56:53 +0000},
	Doi = {10.1049/el:20000699},
	Issn = {0013-5194},
	Journal = {Electronics Letters},
	Keywords = {WIDAR method; cross-correlation; maximum spectral resolution; minimum cost; radio interferometer; very wideband signals; wideband digital correlation; wideband interferometric digital architecture; wideband spectrum; correlation methods;},
	Month = may,
	Number = {11},
	Pages = {987 - 988},
	Title = {Efficient wideband digital correlation},
	Volume = {36},
	Year = {2000},
	Bdsk-Url-1 = {http://dx.doi.org/10.1049/el:20000699}}

@article{Chang:2008,
	Author = {Chang, T.-C. and Pen, U.-L. and Peterson, J. B. and McDonald, P.},
	Date-Added = {2013-04-05 20:56:32 +0000},
	Date-Modified = {2013-04-05 20:56:32 +0000},
	Doi = {10.1103/PhysRevLett.100.091303},
	Journal = {Phys. Rev. Lett.},
	Month = {Mar},
	Number = {9},
	Numpages = {4},
	Pages = {091303},
	Publisher = {American Physical Society},
	Title = {Baryon Acoustic Oscillation Intensity Mapping of Dark Energy},
	Volume = {100},
	Year = {2008},
	Bdsk-Url-1 = {http://dx.doi.org/10.1103/PhysRevLett.100.091303}}

@book{FFT_book,
	Author = {Brigham, E. O.},
	Date-Added = {2013-04-05 20:56:10 +0000},
	Date-Modified = {2013-04-05 20:56:10 +0000},
	Encoding = {tex},
	Publisher = {Prentice-Hall, Inc},
	Title = {The Fast Fourier Transform},
	Year = 1974}

@article{Bhatnagar:2008,
	Author = {{Bhatnagar}, S. and {Cornwell, T. J.} and {Golap, K.} and {Uson, J. M.}},
	Date-Added = {2013-04-05 20:55:28 +0000},
	Date-Modified = {2016-06-03 23:46:43 +0000},
	Doi = {10.1051/0004-6361:20079284},
	Encoding = {tex},
	Journal = {A\&A},
	Number = 1,
	Pages = {419-429},
	Title = {Correcting direction-dependent gains in the deconvolution of radio interferometric images},
	Url = {http://dx.doi.org/10.1051/0004-6361:20079284},
	Volume = 487,
	Year = 2008,
	Bdsk-Url-1 = {http://dx.doi.org/10.1051/0004-6361:20079284}}

@article{Morales:2006,
	Abstract = {Statistical observations of the epoch of reionization using the 21 cm line of neutral hydrogen have the potential to revolutionize our understanding of structure formation and the first luminous objects. However, these observations are complicated by a host of strong foreground sources. Several foreground-removal techniques have been proposed in the literature, and it has been assumed that these would be used in combination to reveal the epoch of reionization (EOR) signal. By studying the characteristic subtraction errors of the proposed foreground-removal techniques, we identify an additional subtraction stage that can further reduce the EOR foreground contamination, and study the interactions between the foreground-removal algorithms. This enables us to outline a comprehensive foreground-removal strategy that incorporates all previously proposed subtraction techniques. Using this foreground-removal framework and the characteristic subtraction errors, we discuss the complementarity of different foreground-removal techniques and the implications for array design and the analysis of EOR data.},
	Affiliation = {AA(Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, MS-51 P-225, Cambridge, MA 02138-1516.), AB(MIT Kavli Institute for Astrophysics and Space Research, 77 Massachusetts Avenue, Cambridge, MA 02139.), AC(MIT Kavli Institute for Astrophysics and Space Research, 77 Massachusetts Avenue, Cambridge, MA 02139.)},
	Author = {Miguel F Morales and Judd D Bowman and Jacqueline N Hewitt},
	Date-Added = {2013-04-05 20:53:17 +0000},
	Date-Modified = {2014-08-31 18:46:26 +0000},
	Doi = {10.1086/506135},
	Journal = {The Astrophysical Journal},
	Keywords = {Cosmology: Observations, Radio Lines: Galaxies, foregrounds},
	Local-Url = {file://localhost/Volumes/miguel.f.morales/Documents/Papers/2006/Morales/The%20Astrophysical%20Journal%202006%20Morales.pdf},
	Month = {Aug},
	Note = {(c) 2006: The American Astronomical Society},
	Pages = {767},
	Pmid = {2006ApJ...648..767M},
	Rating = {0},
	Read = {Yes},
	Title = {Improving Foreground Subtraction in Statistical Observations of 21 cm Emission from the Epoch of Reionization},
	Uri = {papers://DFE1617F-A133-478C-B28B-7AFF8D228C27/Paper/p147},
	Url = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006ApJ...648..767M&link_type=ABSTRACT},
	Volume = {648},
	Year = {2006},
	Bdsk-Url-1 = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006ApJ...648..767M&link_type=ABSTRACT},
	Bdsk-Url-2 = {http://dx.doi.org/10.1086/506135}}

@article{Liu:2011,
	Author = {Adrian Liu and Max Tegmark},
	Date-Added = {2013-04-05 20:52:12 +0000},
	Date-Modified = {2013-04-05 20:52:12 +0000},
	Doi = {doi:10.1103/PhysRevD.83.103006},
	Journal = {Physical Review D},
	Language = {en},
	Month = {Jan},
	Number = {10},
	Pages = {103006--103006},
	Rating = {0},
	Title = {A method for 21 cm power spectrum estimation in the presence of foregrounds},
	Uri = {papers://DFE1617F-A133-478C-B28B-7AFF8D228C27/Paper/p4789},
	Url = {http://adsabs.harvard.edu/abs/2011PhRvD..83j3006L},
	Volume = {83},
	Year = {2011},
	Bdsk-Url-1 = {http://adsabs.harvard.edu/abs/2011PhRvD..83j3006L},
	Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevD.83.103006}}

@article{Kogan:2000,
	Author = {Leonid Kogan},
	Date-Added = {2013-04-05 20:51:38 +0000},
	Date-Modified = {2013-04-05 20:51:38 +0000},
	Journal = {IEEE Transactions on Antennas and Propagation},
	Local-Url = {file://localhost/Volumes/miguel.f.morales/Documents/Papers/IEEE%20Transactions%20on%20Antennas%20and%20Propagation%202000%20Kogan.pdf},
	Number = {7},
	Pages = {1075},
	Rating = {0},
	Title = {Optimizing a Large Array Configuration to Minimize the Sidelobes},
	Uri = {papers://DFE1617F-A133-478C-B28B-7AFF8D228C27/Paper/p4790},
	Url = {http://ieeexplore.ieee.org/stamp/stamp.jsp?tp=&arnumber=876326},
	Volume = {48},
	Year = {2000},
	Bdsk-Url-1 = {http://ieeexplore.ieee.org/stamp/stamp.jsp?tp=&arnumber=876326}}

@article{Cornwell:1988,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/1988ITAP...36.1165C},
	Author = {{Cornwell}, T.~J.},
	Date-Added = {2013-04-05 20:50:52 +0000},
	Date-Modified = {2013-04-05 20:50:52 +0000},
	Doi = {10.1109/8.7233},
	Journal = {IEEE Transactions on Antennas and Propagation},
	Keywords = {ANTENNA ARRAYS, ANTENNA DESIGN, RADIO INTERFEROMETERS, CORRELATION, FOURIER TRANSFORMATION, OPTIMIZATION},
	Month = aug,
	Pages = {1165-1167},
	Title = {{A novel principle for optimization of the instantaneous Fourier plane coverage of correlation arrays}},
	Volume = 36,
	Year = 1988,
	Bdsk-Url-1 = {http://dx.doi.org/10.1109/8.7233}}

@article{Cohanim:2010,
	Author = {Babak Cohanim and Jacqueline Hewitt and Olivier De Weck},
	Date-Added = {2013-04-05 20:49:51 +0000},
	Date-Modified = {2013-04-05 20:49:51 +0000},
	Doi = {doi:10.1086/422356},
	Journal = {The Astrophysical Journal Supplement Series},
	Language = {en},
	Local-Url = {file://localhost/Volumes/miguel.f.morales/Documents/Papers/The%20Astrophysical%20Journal%20Supplement%20Series%202010%20Cohanim.pdf},
	Month = {Jan},
	Pages = {705-705-719--719},
	Rating = {0},
	Title = {The Design of Radio Telescope Array Configurations using Multiobjective Optimization: Imaging Performance versus Cable Length},
	Uri = {papers://DFE1617F-A133-478C-B28B-7AFF8D228C27/Paper/p4842},
	Url = {http://adsabs.harvard.edu/abs/2004ApJS..154..705C},
	Volume = {154},
	Year = {2010},
	Bdsk-Url-1 = {http://adsabs.harvard.edu/abs/2004ApJS..154..705C},
	Bdsk-Url-2 = {http://dx.doi.org/10.1086/422356}}

@article{Bernardi:2011,
	Abstract = {ABSTRACT
We present a method for subtracting point sources from interferometric radio images via forward modelling of the instrument response and involving an algebraic non-linear minimization. The method is applied to simulated maps of the Murchison Wide-field Array but is generally useful in cases where only image data are available. After source subtraction, the residual maps have no statistical difference to the expected thermal noise distribution at all angular scales, indicating high effectiveness in the subtraction. Simulations indicate that the errors in recovering the source parameters decrease with increasing signal-to-noise ratio, which is consistent with the theoretical measurement errors. In applying the technique to simulated snapshot observations with the Murchison Wide-field Array, we found that all 101 sources present in the simulation were recovered with an average position error of 10 arcsec and an average flux density error of 0.15 per cent. This led to a dynamic range increase of approximately 3 orders of magnitude. Since all the sources were deconvolved jointly, the subtraction was not limited by source sidelobes but by thermal noise. This technique is a promising deconvolution method for upcoming radio arrays with a huge number of elements and a candidate for the difficult task of subtracting foreground sources from observations of the 21-cm neutral hydrogen signal from the epoch of reionization.},
	Author = {Bernardi, G. and Mitchell, D. A. and Ord, S. M. and Greenhill, L. J. and Pindor, B. and Wayth, R. B. and Wyithe, J. S. B.},
	Date-Added = {2013-04-05 20:48:19 +0000},
	Date-Modified = {2013-04-05 20:48:19 +0000},
	Doi = {10.1111/j.1365-2966.2010.18145.x},
	Issn = {1365-2966},
	Journal = {Monthly Notices of the Royal Astronomical Society},
	Keywords = {methods: data analysis, methods: numerical, techniques: interferometric, cosmology: observations, dark ages, reionization, first stars, diffuse radiation},
	Number = {1},
	Pages = {411--422},
	Publisher = {Blackwell Publishing Ltd},
	Title = {Subtraction of point sources from interferometric radio images through an algebraic forward modelling scheme},
	Url = {http://dx.doi.org/10.1111/j.1365-2966.2010.18145.x},
	Volume = {413},
	Year = {2011},
	Bdsk-Url-1 = {http://dx.doi.org/10.1111/j.1365-2966.2010.18145.x}}

@article{Boone:2002,
	Author = {F. Boone},
	Date-Added = {2013-04-05 20:40:37 +0000},
	Date-Modified = {2013-04-05 20:41:43 +0000},
	Journal = {Astronomy and Astrophysics},
	Number = {3},
	Pages = {1160-1171},
	Title = {Interferometric array design: Interferometric array design: Distributions of Fourier samples for imaging},
	Volume = {386},
	Year = {2002},
	Bdsk-Url-1 = {http://dx.doi.org/10.1051/0004-6361:20020297}}

@article{Barkana:2005,
	Abstract = {Fluctuations in the 21 cm brightness from cosmic hydrogen at redshifts z ##IMG## [http://ej.iop.org/icons/Entities/gtrsim.gif] {gtrsim} 6 have their source in the primordial density perturbations from inflation, as well as the radiation from galaxies. We propose a method to separate these components based on the angular dependence of the 21 cm fluctuation power spectrum. Peculiar velocities increase the power spectrum by a factor of ~2 compared with density fluctuations alone and introduce an angular dependence in Fourier space. The resulting angular structure relative to the line of sight facilitates a simple separation of the power spectrum into several components, permitting an unambiguous determination of the primordial power spectrum of density fluctuations, and of the detailed properties of all astrophysical sources of 21 cm fluctuations. We also demonstrate that angular multipoles are not useful for measuring large-scale power, and thus, theoretical predictions should focus on the three-dimensional power spectrum of 21 cm fluctuations.},
	Author = {Rennan Barkana and Abraham Loeb},
	Journal = {The Astrophysical Journal Letters},
	Number = {2},
	Pages = {L65},
	Title = {A Method for Separating the Physics from the Astrophysics of High-Redshift 21 Centimeter Fluctuations},
	Url = {http://stacks.iop.org/1538-4357/624/i=2/a=L65},
	Volume = {624},
	Year = {2005},
	Bdsk-Url-1 = {http://stacks.iop.org/1538-4357/624/i=2/a=L65}}

@article{Beardsley:2012,
	Abstract = {Antenna layout is an important design consideration for radio interferometers because it determines the quality of the snapshot point spread function (PSF, or array beam). This is particularly true for experiments targeting the 21-cm Epoch of Reionization signal as the quality of the foreground subtraction depends directly on the spatial dynamic range and thus the smoothness of the baseline distribution. Nearly all sites have constraints on where antennas can be placed -- even at the remote Australian location of the Murchison Widefield Array (MWA) there are rock outcrops, flood zones, heritages areas, emergency runways and trees. These exclusion areas can introduce spatial structure into the baseline distribution that enhances the PSF sidelobes and reduces the angular dynamic range. In this paper we present a new method of constrained antenna placement that reduces the spatial structure in the baseline distribution. This method not only outperforms random placement algorithms that avoid exclusion zones, but surprisingly outperforms random placement algorithms without constraints to provide what we believe are the smoothest constrained baseline distributions developed to date. We use our new algorithm to determine antenna placements for the originally planned MWA, and present the antenna locations, baseline distribution and snapshot PSF for this array choice.},
	Author = {Beardsley, A. P. and Hazelton, B. J. and Morales, M. F. and Capallo, R. J. and Goeke, R. and Emrich, D. and Lonsdale, C. J. and Arcus, W. and Barnes, D. and Bernardi, G. and Bowman, J. D. and Bunton, J. D. and Corey, B. E. and Deshpande, A. and deSouza, L. and Gaensler, B. M. and Greenhill, L. J. and Herne, D. and Hewitt, J. N. and Kaplan, D. L. and Kasper, J. C. and Kincaid, B. B. and Koenig, R. and Kratzenberg, E. and Lynch, M. J. and McWhirter, S. R. and Mitchell, D. A. and Morgan, E. and Oberoi, D. and Ord, S. M. and Pathikulangara, J. and Prabu, T. and Remillard, R. A. and Rogers, A. E. E. and Roshi, A. and Salah, J. E. and Sault, R. J. and Shankar, N. Udaya and Srivani, K. S. and Stevens, J. and Subrahmanyan, R. and Tingay, S. J. and Wayth, R. B. and Waterson, M. and Webster, R. L. and Whitney, A. R. and Williams, A. and Williams, C. L. and Wyithe, J. S. B.},
	Date-Modified = {2014-10-27 15:45:37 +0000},
	Doi = {10.1111/j.1365-2966.2012.20878.x},
	Issn = {1365-2966},
	Journal = {Monthly Notices of the Royal Astronomical Society},
	Keywords = {instrumentation: interferometers, cosmology: miscellaneous},
	Number = {3},
	Pages = {1781--1788},
	Title = {A new layout optimization technique for interferometric arrays, applied to the Murchison Widefield Array},
	Url = {http://dx.doi.org/10.1111/j.1365-2966.2012.20878.x},
	Volume = {425},
	Year = {2012},
	Bdsk-Url-1 = {http://dx.doi.org/10.1111/j.1365-2966.2012.20878.x}}

@article{Bowman:2006,
	Abstract = {Statistical observations of the epoch of reionization (EOR) power spectrum provide a rich data set for understanding the transition from the cosmic ``dark ages'' to the ionized universe we see today. EOR observations have become an active area of experimental cosmology, and three first-generation observatories-MWA, PAST, and LOFAR-are currently under development. In this paper we provide the first quantitative calculation of the three-dimensional power spectrum sensitivity, incorporating the design parameters of a planned array. This calculation is then used to explore the constraints these first-generation observations can place on the EOR power spectrum. The results demonstrate the potential for upcoming power spectrum observations to constrain theories of structure formation and reionization.},
	Affiliation = {AA(Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, 77 Massachusetts Ave., Cambridge, MA 02139; jdbowman@mit.edu, mmorales@space.mit.edu, jhewitt@space.mit.edu.; Department of Physics, Massachusetts Institute of Technology.), AB(Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, 77 Massachusetts Ave., Cambridge, MA 02139; jdbowman@mit.edu, mmorales@space.mit.edu, jhewitt@space.mit.edu.), AC(Kavli Institute for Astrophysics a...},
	Author = {Judd D Bowman and Miguel F Morales and Jacqueline N Hewitt},
	Date-Added = {2008-04-05 05:39:41 -0700},
	Date-Modified = {2011-05-19 19:58:49 -0700},
	Doi = {10.1086/498703},
	Journal = {The Astrophysical Journal},
	Keywords = {Cosmology: Early Universe, Galaxies: Intergalactic Medium- Radio Lines: General, Techniques: Interferometric},
	Month = {Jan},
	Note = {(c) 2006: The American Astronomical Society},
	Pages = {20},
	Pmid = {2006ApJ...638...20B},
	Rating = {0},
	Read = {Yes},
	Title = {The Sensitivity of First-Generation Epoch of Reionization Observatories and Their Potential for Differentiating Theoretical Power Spectra},
	Uri = {papers://DFE1617F-A133-478C-B28B-7AFF8D228C27/Paper/p163},
	Url = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006ApJ...638...20B&link_type=ABSTRACT},
	Volume = {638},
	Year = {2006},
	Bdsk-Url-1 = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006ApJ...638...20B&link_type=ABSTRACT},
	Bdsk-Url-2 = {http://dx.doi.org/10.1086/498703}}

@article{Bowman:2009,
	Abstract = {Subtraction of astrophysical foreground contamination from "dirty" sky maps produced by simulated measurements of the Murchison Widefield Array (MWA) has been performed by fitting a third-order polynomial along the spectral dimension of each pixel in the data cubes. The simulations are the first to include the unavoidable instrumental effects of the frequency-dependent primary antenna beams and synthesized array beams. They recover the one-dimensional spherically binned input redshifted 21 cm power spectrum within ~1% over the scales probed most sensitively by the MWA (0.01 ##IMG## [http://ej.iop.org/icons/Entities/lsim.gif] {lsim} k ##IMG## [http://ej.iop.org/icons/Entities/lsim.gif] {lsim} 1 Mpc �1 ) and demonstrate that realistic instrumental effects will not mask the epoch of reionization signal. We find that the weighting function used to produce the dirty sky maps from the gridded visibility measurements is important to the success of the technique. Uniform weighting of the visibility measurements produces the best results, whereas natural weighting significantly worsens the foreground subtraction by coupling structure in the density of the visibility measurements to spectral structure in the dirty sky map data cube. The extremely dense uv -coverage of the MWA was found to be advantageous for this technique and produced very good results on scales corresponding to | u | ##IMG## [http://ej.iop.org/icons/Entities/lsim.gif] {lsim} 500? in the uv -plane without any selective editing of the uv -coverage.},
	Author = {Judd D. Bowman and Miguel F. Morales and Jacqueline N. Hewitt},
	Journal = {The Astrophysical Journal},
	Number = {1},
	Pages = {183},
	Title = {Foreground Contamination in Interferometric Measurements of the Redshifted 21 cm Power Spectrum},
	Url = {http://stacks.iop.org/0004-637X/695/i=1/a=183},
	Volume = {695},
	Year = {2009},
	Bdsk-Url-1 = {http://stacks.iop.org/0004-637X/695/i=1/a=183}}

@article{Furlanetto:2006,
	Abstract = {Electronic Article Available from Elsevier Science.},
	Affiliation = {AA(Department of Physics, Yale University, PO Box 208121, New Haven, CT 06520, USA), AB(Department of Physics, University of California, Santa Barbara, CA 93106, USA), AC(Research School of Astronomy and Astrophysics, The Australian National University, Mount Stromlo Observatory, Cotter Road, Weston, ACT 2611, Australia)},
	Author = {Steven R Furlanetto and S. Peng Oh and Frank H Briggs},
	Date-Added = {2008-04-05 05:55:43 -0700},
	Date-Modified = {2015-02-05 18:46:10 +0000},
	Doi = {10.1016/j.physrep.2006.08.002},
	Journal = {Physics Reports},
	Keywords = {review,theory},
	Local-Url = {file://localhost/Volumes/miguel.f.morales/Documents/Papers/2006/Furlanetto/Physics%20Reports%202006%20Furlanetto.pdf},
	Month = {Sep},
	Note = {Elsevier B.V.},
	Pages = {181},
	Pmid = {2006PhR...433..181F},
	Rating = {0},
	Read = {Yes},
	Title = {Cosmology at low frequencies: The 21 cm transition and the high-redshift Universe},
	Uri = {papers://DFE1617F-A133-478C-B28B-7AFF8D228C27/Paper/p341},
	Url = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006PhR...433..181F&link_type=ABSTRACT},
	Volume = {433},
	Year = {2006},
	Bdsk-Url-1 = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006PhR...433..181F&link_type=ABSTRACT},
	Bdsk-Url-2 = {http://dx.doi.org/10.1016/j.physrep.2006.08.002}}

@article{Komatsu:2011,
	Abstract = {The combination of seven-year data from WMAP and improved astrophysical data rigorously tests the standard cosmological model and places new constraints on its basic parameters and extensions. By combining the WMAP data with the latest distance measurements from the baryon acoustic oscillations (BAO) in the distribution of galaxies and the Hubble constant ( H 0 ) measurement, we determine the parameters of the simplest six-parameter ?CDM model. The power-law index of the primordial power spectrum is n s = 0.968 � 0.012 (68% CL) for this data combination, a measurement that excludes the Harrison-Zel'dovich-Peebles spectrum by 99.5% CL. The other parameters, including those beyond the minimal set, are also consistent with, and improved from, the five-year results. We find no convincing deviations from the minimal model. The seven-year temperature power spectrum gives a better determination of the third acoustic peak, which results in a better determination of the redshift of the matter-radiation equality epoch. Notable examples of improved parameters are the total mass of neutrinos, � m ? < 0.58 eV(95%CL), and the effective number of neutrino species, N eff = 4.34 +0.86 �0.88 (68% CL), which benefit from better determinations of the third peak and H 0 . The limit on a constant dark energy equation of state parameter from WMAP +BAO+ H 0 , without high-redshift Type Ia supernovae, is w = �1.10 � 0.14 (68% CL). We detect the effect of primordial helium on the temperature power spectrum and provide a new test of big bang nucleosynthesis by measuring Y p = 0.326 � 0.075 (68% CL). We detect, and show on the map for the first time, the tangential and radial polarization patterns around hot and cold spots of temperature fluctuations, an important test of physical processes at z = 1090 and the dominance of adiabatic scalar fluctuations. The seven-year polarization data have significantly improved: we now detect the temperature- E -mode polarization cross power spectrum at 21?, compared with 13? from the five-year data. With the seven-year temperature- B -mode cross power spectrum, the limit on a rotation of the polarization plane due to potential parity-violating effects has improved by 38% to ##IMG## [http://ej.iop.org/images/0067-0049/192/2/18/apjs374858ieqn1.gif] {$\Delta \alpha =-1\mbox{$.\!\!^\circ $}1\pm 1\mbox{$.\!\!^\circ $}4 (\rm statistical)\pm 1\mbox{$.\!\!^\circ $}5 (\rm systematic)$} (68% CL). We report significant detections of the Sunyaev-Zel'dovich (SZ) effect at the locations of known clusters of galaxies. The measured SZ signal agrees well with the expected signal from the X-ray data on a cluster-by-cluster basis. However, it is a factor of 0.5-0.7 times the predictions from "universal profile" of Arnaud et al., analytical models, and hydrodynamical simulations. We find, for the first time in the SZ effect, a significant difference between the cooling-flow and non-cooling-flow clusters (or relaxed and non-relaxed clusters), which can explain some of the discrepancy. This lower amplitude is consistent with the lower-than-theoretically expected SZ power spectrum recently measured by the South Pole Telescope Collaboration.},
	Author = {E. Komatsu and K. M. Smith and J. Dunkley and C. L. Bennett and B. Gold and G. Hinshaw and N. Jarosik and D. Larson and M. R. Nolta and L. Page and D. N. Spergel and M. Halpern and R. S. Hill and A. Kogut and M. Limon and S. S. Meyer and N. Odegard and G. S. Tucker and J. L. Weiland and E. Wollack and E. L. Wright},
	Journal = {The Astrophysical Journal Supplement Series},
	Number = {2},
	Pages = {18},
	Title = {Seven-year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation},
	Url = {http://stacks.iop.org/0067-0049/192/i=2/a=18},
	Volume = {192},
	Year = {2011},
	Bdsk-Url-1 = {http://stacks.iop.org/0067-0049/192/i=2/a=18}}

@article{Lidz:2008,
	Abstract = {We forecast the sensitivity with which the Murchison Widefield Array (MWA) can measure the 21 cm power spectrum of cosmic hydrogen. The MWA is sensitive to roughly a decade in scale (wavenumbers of k~0.1-1 h Mpc-1). This amounts primarily to constraints on two numbers: the amplitude and the slope of the 21 cm power spectrum on the scales probed. We find, however, that the redshift evolution in these quantities can yield important information about reionization. We examine a range of theoretical models, spanning uncertainties in the nature of the ionizing sources and the abundance of minihalos during reionization. Although the power spectrum differs substantially among these models, a generic prediction is that the amplitude of the 21 cm power spectrum on MWA scales (k~0.4 h Mpc-1) peaks near the epoch when the intergalactic medium (IGM) is ~50% ionized. Moreover, the slope of the 21 cm power spectrum flattens as the ionization fraction increases and the sizes of the H II regions grow. With regards to detection sensitivity, we show that the optimal MWA antenna configuration for power spectrum measurements would pack all 500 antenna tiles as closely as possible in a compact core. Detecting the characteristic redshift evolution of our models will help to confirm that observed 21 cm fluctuations originate from the IGM, and not from foregrounds, and will provide an indirect constraint on the evolution of the volume-filling factor of H II regions during reionization. After two years of observations, the MWA can constrain the filling factor at an epoch when i>~0.5 to within roughly +/-δi>~0.1 at 2 σ confidence.},
	Affiliation = {AA(Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138.), AB(Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138.; Berkeley Center for Cosmological Physics, Department of Physics, University of California; and Lawrence Berkeley National Labs, 1 Cyclotron Road, Berkeley, CA 94720.), AC(Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138.), AD(Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, M...},
	Author = {Adam Lidz and Oliver Zahn and Matthew McQuinn and Matias Zaldarriaga and Lars Hernquist},
	Date-Added = {2008-10-31 11:07:28 -0700},
	Date-Modified = {2011-05-19 19:58:34 -0700},
	Doi = {10.1086/587618},
	Journal = {The Astrophysical Journal},
	Keywords = {Cosmology: Theory, Galaxies: Intergalactic Medium, Cosmology: Large-Scale Structure of Universe},
	Month = {Jun},
	Note = {(c) 2008: The American Astronomical Society},
	Pages = {962},
	Pmid = {2008ApJ...680..962L},
	Rating = {0},
	Read = {Yes},
	Title = {Detecting the Rise and Fall of 21 cm Fluctuations with the Murchison Widefield Array},
	Uri = {papers://DFE1617F-A133-478C-B28B-7AFF8D228C27/Paper/p3647},
	Url = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008ApJ...680..962L&link_type=ABSTRACT},
	Volume = {680},
	Year = {2008},
	Bdsk-Url-1 = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008ApJ...680..962L&link_type=ABSTRACT},
	Bdsk-Url-2 = {http://dx.doi.org/10.1086/587618}}

@article{Lonsdale:2009,
	Abstract = {The Murchison Widefield Array: Design Overview},
	Author = {C Lonsdale and R Cappallo and M Morales and F Briggs and L Benkevitch and J Bowman and J Bunton and S Burns and B Corey and L deSouza and S Doeleman and M Derome and A Deshpande and M Gopala and L Greenhill and D Herne and J Hewitt and P Kamini and J Kasper and B Kincaid and J Kocz and E Kowald and E Kratzenberg and D Kumar and M Lynch and S Madhavi and M Matejek and D Mitchell and E Morgan and D Oberoi and S Ord and J Pathikulangara and T Prabu and A Rogers and A Roshi and J Salah and R Sault and N Shankar and K Srivani and J Stevens and S Tingay and A Vaccarella and M Waterson and R Wayth and R Webster and A Whitney and A Williams and C Williams},
	Date-Added = {2009-08-27 13:12:19 -0700},
	Date-Modified = {2011-05-19 19:58:32 -0700},
	Doi = {10.1109/JPROC.2009.2017564},
	Journal = {Proceedings of the IEEE},
	Month = {Aug},
	Number = {8},
	Pages = {1497 -- 1506},
	Pmid = {5164979@ieeejrns},
	Rating = {0},
	Read = {Yes},
	Title = {The Murchison Widefield Array: Design Overview},
	Uri = {papers://DFE1617F-A133-478C-B28B-7AFF8D228C27/Paper/p3966},
	Url = {http://ieeexplore.ieee.org/search/srchabstract.jsp?arnumber=5164979&isnumber=5165124&punumber=5&k2dockey=5164979@ieeejrns},
	Volume = {97},
	Year = {2009},
	Bdsk-Url-1 = {http://ieeexplore.ieee.org/search/srchabstract.jsp?arnumber=5164979&isnumber=5165124&punumber=5&k2dockey=5164979@ieeejrns},
	Bdsk-Url-2 = {http://dx.doi.org/10.1109/JPROC.2009.2017564}}

@article{McQuinn:2006,
	Abstract = {A number of radio interferometers are currently being planned or constructed to observe 21 cm emission from reionization. Not only will such measurements provide a detailed view of that epoch, but, since the 21 cm emission also traces the distribution of matter in the universe, this signal can be used to constrain cosmological parameters. The sensitivity of an interferometer to the cosmological information in the signal may depend on how precisely the angular dependence of the 21 cm three-dimensional power spectrum can be measured. Using an analytic model for reionization, we quantify all the effects that break the spherical symmetry of the three-dimensional 21 cm power spectrum. We find that upcoming observatories will be sensitive to the 21 cm signal over a wide range of scales, from larger than 100 to as small as 1 comoving Mpc. Next, we consider three methods to measure cosmological parameters from the signal: (1) direct fitting of the density power spectrum to the signal, (2) using only the velocity field fluctuations in the signal, and (3) looking at the signal at large enough scales that all fluctuations trace the density field. With the foremost method, the first generation of 21 cm observations should moderately improve existing constraints on cosmological parameters for certain low-redshift reionization scenarios, and a 2 yr observation with the second-generation interferometer MWA5000 in combination with the CMB telescope Planck could improve constraints on Ωw, Ωmh2, Ωbh2, Ων, ns, and αs. If the universe is substantially ionized by z~12 or if spin temperature fluctuations are important, we show that it will be difficult to place competitive constraints on cosmological parameters with any of the considered methods.},
	Affiliation = {AA(Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138; mmcquinn@cfa.harvard.edu.), AB(Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138; mmcquinn@cfa.harvard.edu.), AC(Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138; mmcquinn@cfa.harvard.edu.; Jefferson Laboratory of Physics, Harvard University, Cambridge, MA 02138.), AD(Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138; mmcqu...},
	Author = {Matthew McQuinn and Oliver Zahn and Matias Zaldarriaga and Lars Hernquist and Steven R Furlanetto},
	Date-Added = {2008-04-05 05:44:44 -0700},
	Date-Modified = {2011-05-19 19:59:02 -0700},
	Doi = {10.1086/505167},
	Journal = {The Astrophysical Journal},
	Keywords = {Galaxies: Intergalactic Medium, Radio Lines: General, Cosmology: Theory},
	Month = {Nov},
	Note = {(c) 2006: The American Astronomical Society},
	Pages = {815},
	Pmid = {2006ApJ...653..815M},
	Rating = {0},
	Read = {Yes},
	Title = {Cosmological Parameter Estimation Using 21 cm Radiation from the Epoch of Reionization},
	Uri = {papers://DFE1617F-A133-478C-B28B-7AFF8D228C27/Paper/p222},
	Url = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006ApJ...653..815M&link_type=ABSTRACT},
	Volume = {653},
	Year = {2006},
	Bdsk-Url-1 = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006ApJ...653..815M&link_type=ABSTRACT},
	Bdsk-Url-2 = {http://dx.doi.org/10.1086/505167}}

@article{Morales:2004,
	Abstract = {This paper explores the potential for statistical epoch of reionization (EOR) measurements using wide-field radio observations. New developments in low-frequency radio instrumentation and signal processing allow very sensitive EOR measurements, and the analysis techniques enabled by these advances offer natural ways of separating the EOR signal from the residual foreground emission. This paper introduces the enabling technologies and proposes an analysis technique designed to make optimal use of the capabilities of next-generation low-frequency radio arrays. The observations we propose can directly observe the power spectrum of the EOR using relatively short observations and are significantly more sensitive than other techniques that have been discussed in the literature. For example, in the absence of foreground contamination the measurements we propose would produce five 3 σ power spectrum points in 100 hr of observation with only 4 MHz bandwidth with LOFAR for simple models of the high-redshift 21 cm emission. The challenge of residual foreground removal may be addressed by the symmetries in the three-dimensional (two spatial frequencies and radio frequency) radio interferometric data. These symmetries naturally separate the EOR signal from most classes of residual unsubtracted foreground contamination, including all foreground continuum sources and radio line emission from the Milky Way.},
	Affiliation = {AA(Center for Space Research, 37-664H, Massachusetts Institute of Technology, 77 Massachusetts Avenue, Cambridge, MA 02139; mmorales@space.mit.edu), AB(Center for Space Research, 37-241, Massachusetts Institute of Technology, 77 Massachusetts Avenue, Cambridge, MA 02139; jhewitt@space.mit.edu)},
	Author = {Miguel F Morales and Jacqueline N Hewitt},
	Date-Added = {2008-04-05 07:45:43 -0700},
	Date-Modified = {2011-05-19 19:59:03 -0700},
	Doi = {10.1086/424437},
	Journal = {The Astrophysical Journal},
	Keywords = {Radio Lines: General, Cosmology: Observations, Cosmology: Early Universe},
	Month = {Oct},
	Note = {(c) 2004: The American Astronomical Society},
	Pages = {7},
	Pmid = {2004ApJ...615....7M},
	Rating = {0},
	Read = {Yes},
	Title = {Toward Epoch of Reionization Measurements with Wide-Field Radio Observations},
	Uri = {papers://DFE1617F-A133-478C-B28B-7AFF8D228C27/Paper/p803},
	Url = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004ApJ...615....7M&link_type=ABSTRACT},
	Volume = {615},
	Year = {2004},
	Bdsk-Url-1 = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004ApJ...615....7M&link_type=ABSTRACT},
	Bdsk-Url-2 = {http://dx.doi.org/10.1086/424437}}

@article{Morales:2005,
	Abstract = {Recent theoretical developments for observing the epoch of reionization (EOR) have concentrated on the power spectrum signature of redshifted 21 cm emission. These studies have demonstrated the great potential of statistical EOR observations; however, the sensitivity calculations for proposed low-frequency radio arrays have been highly approximate. The formalism developed for interferometric measurements of the cosmic microwave background can be extended to three dimensions to naturally incorporate the line-of-sight information inherent in the EOR signal. In this paper we demonstrate how to accurately calculate the EOR power spectrum sensitivity of an array and develop scaling relationships that can be used to guide the design of EOR observatories. The implications for antenna distribution, antenna size, and correlator requirements on the EOR sensitivity are detailed.},
	Affiliation = {AA(Center for Space Research, Massachusetts Institute of Technology, 77 Massachusetts Avenue, Cambridge, MA 02139; mmorales@space.mit.edu)},
	Author = {Miguel F Morales},
	Date-Added = {2008-04-05 07:45:20 -0700},
	Date-Modified = {2011-05-19 19:58:49 -0700},
	Doi = {10.1086/426730},
	Journal = {The Astrophysical Journal},
	Keywords = {Cosmology: Observations, Radio Lines: General},
	Month = {Jan},
	Note = {(c) 2005: The American Astronomical Society},
	Pages = {678},
	Pmid = {2005ApJ...619..678M},
	Rating = {0},
	Read = {Yes},
	Title = {Power Spectrum Sensitivity and the Design of Epoch of Reionization Observatories},
	Url = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005ApJ...619..678M&link_type=ABSTRACT},
	Volume = {619},
	Year = {2005},
	Bdsk-Url-1 = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005ApJ...619..678M&link_type=ABSTRACT},
	Bdsk-Url-2 = {http://dx.doi.org/10.1086/426730}}

@article{Morales:2010,
	Author = {Miguel Morales and J Wyithe},
	Date-Added = {2011-06-02 11:59:14 -0700},
	Date-Modified = {2011-06-02 17:43:03 -0700},
	Doi = {doi:10.1146/annurev-astro-081309-130936},
	Journal = {Annual Review of Astronomy and Astrophysics},
	Language = {en},
	Month = {Sep},
	Pages = {127--171},
	Rating = {0},
	Title = {Reionization and Cosmology with 21-cm Fluctuations},
	Uri = {papers://DFE1617F-A133-478C-B28B-7AFF8D228C27/Paper/p4786},
	Url = {http://adsabs.harvard.edu/abs/2010ARA%2526A..48..127M},
	Volume = {48},
	Year = {2010},
	Bdsk-Url-1 = {http://adsabs.harvard.edu/abs/2010ARA%2526A..48..127M},
	Bdsk-Url-2 = {http://dx.doi.org/10.1146/annurev-astro-081309-130936}}

@article{Morales:2012,
	Abstract = {Contamination from instrumental effects interacting with bright astrophysical sources is the primary impediment to measuring Epoch of Reionization (EoR) and Baryon Acoustic Oscillations (BAO) 21 cm power spectra�an effect called mode mixing. In this paper, we identify four fundamental power spectrum shapes produced by mode mixing that will affect all upcoming observations. We are able, for the first time, to explain the wedge-like structure seen in advanced simulations and to forecast the shape of an "EoR window" that is mostly free of contamination. Understanding the origins of these contaminations also enables us to identify calibration and foreground subtraction errors below the imaging limit, providing a powerful new tool for precision observations.},
	Author = {Miguel F. Morales and Bryna Hazelton and Ian Sullivan and Adam Beardsley},
	Date-Modified = {2014-10-18 23:03:37 +0000},
	Journal = {ApJ},
	Keywords = {wedge},
	Number = {2},
	Pages = {137},
	Title = {Four Fundamental Foreground Power Spectrum Shapes for 21 cm Cosmology Observations},
	Url = {http://stacks.iop.org/0004-637X/752/i=2/a=137},
	Volume = {752},
	Year = {2012},
	Bdsk-Url-1 = {http://stacks.iop.org/0004-637X/752/i=2/a=137}}