Supplementary material for 'Exploring H2O Prominence in Reflection Spectra of Cool Giant Planets ', ApJ, 2018. Contains 54600 model reflection spectra, along with animated visuals, from MacDonald et al. (2018). Please see the Readme for an explanation of the repository structure
We examine the spectra and infrared colors of the cool, methane-dominated atmospheres at TeA 1400 K...
Context. The nuclear obscurer of active galactic nuclei (AGN) is poorly understood in terms of its o...
Reflectance spectroscopy is a useful method for identifying an unknown mineral, if its spectrum can ...
<p>Supplementary material for 'Exploring H2O Prominence in Reflection Spectra of Cool Giant Planets ...
Interpreting the reflection spectra of cool giant planets will be a challenge. Spectra of such world...
Spectra of red giant stellar hosts and reflectance/emission planetary spectra as described in Kozaki...
Planned astronomical observatories of the 2020s will be capable of obtaining reflected light photome...
This dataset contains the reflected light models used in the analysis of Batalha et al. 2018 (Color ...
While the James Webb Space Telescope will detect and characterize extrasolar planets by transit and ...
This dataset contains the simulated high-resolution spectra and profiles of 360 different Earth-like...
Context. The extreme contrast ratios between stars and their planets at optical wavelengths make it ...
International audienceWe present the highest fidelity spectrum to date of a planetary-mass object. V...
This dataset contains opacities for atoms and molecules that are relevant to the sector of hot rocky...
README This file contains the model spectra presented in Morley et al. 2017, Observing the Atmosphe...
This dataset contains the geometric albedo, spectra, and colors of 19 different Solar System objects...
We examine the spectra and infrared colors of the cool, methane-dominated atmospheres at TeA 1400 K...
Context. The nuclear obscurer of active galactic nuclei (AGN) is poorly understood in terms of its o...
Reflectance spectroscopy is a useful method for identifying an unknown mineral, if its spectrum can ...
<p>Supplementary material for 'Exploring H2O Prominence in Reflection Spectra of Cool Giant Planets ...
Interpreting the reflection spectra of cool giant planets will be a challenge. Spectra of such world...
Spectra of red giant stellar hosts and reflectance/emission planetary spectra as described in Kozaki...
Planned astronomical observatories of the 2020s will be capable of obtaining reflected light photome...
This dataset contains the reflected light models used in the analysis of Batalha et al. 2018 (Color ...
While the James Webb Space Telescope will detect and characterize extrasolar planets by transit and ...
This dataset contains the simulated high-resolution spectra and profiles of 360 different Earth-like...
Context. The extreme contrast ratios between stars and their planets at optical wavelengths make it ...
International audienceWe present the highest fidelity spectrum to date of a planetary-mass object. V...
This dataset contains opacities for atoms and molecules that are relevant to the sector of hot rocky...
README This file contains the model spectra presented in Morley et al. 2017, Observing the Atmosphe...
This dataset contains the geometric albedo, spectra, and colors of 19 different Solar System objects...
We examine the spectra and infrared colors of the cool, methane-dominated atmospheres at TeA 1400 K...
Context. The nuclear obscurer of active galactic nuclei (AGN) is poorly understood in terms of its o...
Reflectance spectroscopy is a useful method for identifying an unknown mineral, if its spectrum can ...
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