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Interstellar communication: The colors of optical SETI
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Forward modeling of spectroscopic galaxy surveys: application to SDSS
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Radial gradients in initial mass function sensitive absorption features in the Coma brightest cluster galaxies
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Measuring FeO variation using astronomical spectroscopic observations
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Atmospheric conditions at Cerro Armazones derived from astronomical data
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Robert J. De Rosa, Julien Rameau, Jenny Patience, James R. Graham, René Doyon, David Lafrenière, Bruce Macintosh, Laurent Pueyo, Abhijith Rajan, Jason J. Wang, Kimberly Ward-Duong, Li-Wei Hung, Jérôme Maire, Eric L. Nielsen, S. Mark Ammons, Joanna Bulger, Andrew Cardwell, Jeffrey K. Chilcote, Ramon L. Galvez, Benjamin L. Gerard, Stephen Goodsell, Markus Hartung, Pascale Hibon, Patrick Ingraham, Mara Johnson-Groh, et al. The Astrophysical Journal 824(2) 121 (2016) https://doi.org/10.3847/0004-637X/824/2/121
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Early-type stars observed in the ESO UVES Paranal Observatory Project - V. Time-variable interstellar absorption
C. M. McEvoy, J. V. Smoker, P. L. Dufton, et al. Monthly Notices of the Royal Astronomical Society 451(2) 1396 (2015) https://doi.org/10.1093/mnras/stv945
The Innsbruck/ESO sky models and telluric correction tools
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OH populations and temperatures from simultaneous spectroscopic observations of 25 bands
S. Noll, W. Kausch, S. Kimeswenger, S. Unterguggenberger and A. M. Jones Atmospheric Chemistry and Physics Discussions 14(23) 32979 (2014) https://doi.org/10.5194/acpd-14-32979-2014
An advanced scattered moonlight model for Cerro Paranal