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| -\item[{\color{numcolor}\scriptsize12}] \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 |
| 1 | +\item[{\color{numcolor}\scriptsize}] \textbf{Luger, R.}, Foreman-Mackey, D., \& Hogg, D. W., 2017, \emph{Linear models for systematics and nuisances}, AAS Research Notes |
2 | 2 |
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| -\item[{\color{numcolor}\scriptsize5}] \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 |
| 3 | +\item[{\color{numcolor}\scriptsize13}] \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 |
| 4 | + |
| 5 | +\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 |
4 | 6 |
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5 | 7 | \item[{\color{numcolor}\scriptsize6}] \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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6 | 8 |
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| -\item[{\color{numcolor}\scriptsize29}] \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 |
| 9 | +\item[{\color{numcolor}\scriptsize31}] \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 |
8 | 10 |
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| -\item[{\color{numcolor}\scriptsize19}] 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 |
| 11 | +\item[{\color{numcolor}\scriptsize20}] 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 |
10 | 12 |
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| -\item[{\color{numcolor}\scriptsize19}] 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 |
| 13 | +\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 |
12 | 14 |
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13 | 15 | \item[{\color{numcolor}\scriptsize20}] 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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14 | 16 |
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