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\documentclass[a4paper]{article} | ||
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\item[{\color{numcolor}\scriptsize}] \textbf{Luger, R.}, Foreman-Mackey, D., \& Hogg, D., 2017, \doi{10.3847/2515-5172/aa96b5}{Linear Models for Systematics and Nuisances}, Notes of the American Astronomical Society, \textbf{1}, 7 | ||
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\item[{\color{numcolor}\scriptsize}] \textbf{Luger, R.}, Lustig-Yaeger, J., \& Agol, E., 2017, \arxiv{1711.05739}{Planet-Planet Occultations in TRAPPIST-1 and Other Exoplanet Systems}, ArXiv:1711.05739 | ||
\item[{\color{numcolor}\scriptsize1}] \textbf{Luger, R.}, Lustig-Yaeger, J., \& Agol, E., 2017, \arxiv{1711.05739}{Planet-Planet Occultations in TRAPPIST-1 and Other Exoplanet Systems}, ArXiv:1711.05739 | ||
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\item[{\color{numcolor}\scriptsize15}] \textbf{Luger, R.}, Sestovic, M., Kruse, E., Grimm, S., \etal, 2017, \doi{10.1038/s41550-017-0129}{A Seven-Planet Resonant Chain in TRAPPIST-1}, Nature Astronomy, \textbf{1}, 129 | ||
\item[{\color{numcolor}\scriptsize18}] \textbf{Luger, R.}, Sestovic, M., Kruse, E., Grimm, S., \etal, 2017, \doi{10.1038/s41550-017-0129}{A Seven-Planet Resonant Chain in TRAPPIST-1}, Nature Astronomy, \textbf{1}, 129 | ||
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\item[{\color{numcolor}\scriptsize6}] \textbf{Luger, R.}, Lustig-Yaeger, J., Fleming, D., Tilley, M., \etal, 2017, \doi{10.3847/1538-4357/aa6040}{The Pale Green Dot: A Method to Characterize Proxima Centauri B Using Exo-Aurorae}, \apj, \textbf{837}, 63 | ||
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\item[{\color{numcolor}\scriptsize8}] \textbf{Luger, R.}, Kruse, E., Foreman-Mackey, D., Agol, E., \& Saunders, N., 2017, \arxiv{1702.05488}{An Update to the EVEREST K2 Pipeline: Short Cadence, Saturated Stars, and Kepler-Like Photometry Down to Kp = 15}, ArXiv:1702.05488 | ||
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\item[{\color{numcolor}\scriptsize35}] \textbf{Luger, R.}, Agol, E., Kruse, E., Barnes, R., \etal, 2016, \doi{10.3847/0004-6256/152/4/100}{EVEREST: Pixel Level Decorrelation of K2 Light Curves}, \aj, \textbf{152}, 100 | ||
\item[{\color{numcolor}\scriptsize37}] \textbf{Luger, R.}, Agol, E., Kruse, E., Barnes, R., \etal, 2016, \doi{10.3847/0004-6256/152/4/100}{EVEREST: Pixel Level Decorrelation of K2 Light Curves}, \aj, \textbf{152}, 100 | ||
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\item[{\color{numcolor}\scriptsize21}] Meadows, V., Arney, G., Schwieterman, E., Lustig-Yaeger, J., \etal\ (including\ \textbf{Luger, R.}), 2016, \arxiv{1608.08620}{The Habitability of Proxima Centauri B: II: Environmental States and Observational Discriminants}, ArXiv:1608.08620 | ||
\item[{\color{numcolor}\scriptsize23}] Meadows, V., Arney, G., Schwieterman, E., Lustig-Yaeger, J., \etal\ (including\ \textbf{Luger, R.}), 2016, \arxiv{1608.08620}{The Habitability of Proxima Centauri B: II: Environmental States and Observational Discriminants}, ArXiv:1608.08620 | ||
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\item[{\color{numcolor}\scriptsize21}] Barnes, R., Deitrick, R., \textbf{Luger, R.}, Driscoll, P., \etal, 2016, \arxiv{1608.06919}{The Habitability of Proxima Centauri B I: Evolutionary Scenarios}, ArXiv:1608.06919 | ||
\item[{\color{numcolor}\scriptsize23}] Barnes, R., Deitrick, R., \textbf{Luger, R.}, Driscoll, P., \etal, 2016, \arxiv{1608.06919}{The Habitability of Proxima Centauri B I: Evolutionary Scenarios}, ArXiv:1608.06919 | ||
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\item[{\color{numcolor}\scriptsize21}] Schwieterman, E., Meadows, V., Domagal-Goldman, S., Deming, D., \etal\ (including\ \textbf{Luger, R.}), 2016, \doi{10.3847/2041-8205/819/1/L13}{Identifying Planetary Biosignature Impostors: Spectral Features of CO and O$_4$ Resulting From Abiotic O$_2$/O$_3$ Production}, \apj, \textbf{819} | ||
\item[{\color{numcolor}\scriptsize22}] Schwieterman, E., Meadows, V., Domagal-Goldman, S., Deming, D., \etal\ (including\ \textbf{Luger, R.}), 2016, \doi{10.3847/2041-8205/819/1/L13}{Identifying Planetary Biosignature Impostors: Spectral Features of CO and O$_4$ Resulting From Abiotic O$_2$/O$_3$ Production}, \apj, \textbf{819} | ||
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\item[{\color{numcolor}\scriptsize72}] \textbf{Luger, R.}, \& Barnes, R., 2015, \doi{10.1089/ast.2014.1231}{Extreme Water Loss and Abiotic O$_2$ Buildup on Planets Throughout the Habitable Zones of M Dwarfs}, Astrobiology, \textbf{15}, 119 | ||
\item[{\color{numcolor}\scriptsize74}] \textbf{Luger, R.}, \& Barnes, R., 2015, \doi{10.1089/ast.2014.1231}{Extreme Water Loss and Abiotic O$_2$ Buildup on Planets Throughout the Habitable Zones of M Dwarfs}, Astrobiology, \textbf{15}, 119 | ||
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\item[{\color{numcolor}\scriptsize31}] \textbf{Luger, R.}, Barnes, R., Lopez, E., Fortney, J., \etal, 2015, \doi{10.1089/ast.2014.1215}{Habitable Evaporated Cores: Transforming Mini-Neptunes Into Super-Earths in the Habitable Zones of M Dwarfs}, Astrobiology, \textbf{15}, 57 | ||
\item[{\color{numcolor}\scriptsize32}] \textbf{Luger, R.}, Barnes, R., Lopez, E., Fortney, J., \etal, 2015, \doi{10.1089/ast.2014.1215}{Habitable Evaporated Cores: Transforming Mini-Neptunes Into Super-Earths in the Habitable Zones of M Dwarfs}, Astrobiology, \textbf{15}, 57 | ||
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\item[{\color{numcolor}\scriptsize8}] Deitrick, R., Barnes, R., McArthur, B., Quinn, T., \etal\ (including\ \textbf{Luger, R.}), 2015, \doi{10.1088/0004-637X/798/1/46}{The Three-Dimensional Architecture of the {\ensuremath{\upsilon}} Andromedae Planetary System}, \apj, \textbf{798}, 46 |
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\textbf{Total:} 12 $\smash{|}$ \textbf{Refereed:} 8 $\smash{|}$ \textbf{First Author:} 8 $\smash{|}$ \textbf{Citations:} 238 $\smash{|}$ \textbf{h-index:} 9 | ||
Total Pubs \textbf{12}\\Refereed \textbf{8}\\First Author \textbf{8}\\Citations \textbf{252}\\h-index \textbf{9}\\ |
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