Spectra of red giant stellar hosts and reflectance/emission planetary spectra as described in Kozakis & Kaltenegger (2020). File names and content are explained in 0readme.txt. Please email theakozakis@gmail.com with any questions
We model the atmospheres and spectra of Earth-like planets orbiting the entire grid of M dwarfs for...
We present model atmospheres for an Earth-like planet orbiting the entire grid of main sequence FGK...
International audienceA broad effort is ongoing with large spectroscopic surveys such as APOGEE, ESO...
This dataset contains the simulated high-resolution spectra and profiles of 360 different Earth-like...
Context. It remains difficult to interpret the near-IR emission of young stellar populations. One ma...
Supplementary material for 'Exploring H2O Prominence in Reflection Spectra of Cool Giant Planets ', ...
Atmospheres of transiting extrasolar giant planets (EGPs) such as HD 209458b must impose features on...
Interpreting the reflection spectra of cool giant planets will be a challenge. Spectra of such world...
Planets larger than Earth and smaller than Neptune are some of the most numerous in the galaxy, but ...
Spectroscopy is a tool for determining the composition and physical properties of a material. Becau...
Context. The atmosphere of Earth-like extrasolar planets orbiting different types of stars is influe...
This dataset contains the geometric albedo, spectra, and colors of 19 different Solar System objects...
An essential reference for researchers and students of planetary remote sensing on the interaction o...
Aims. A spectroscopic analysis of stellar spectra can be carried out using multiple approaches such ...
Planets larger than Earth and smaller than Neptune are some of the most numerous in the galaxy, but ...
We model the atmospheres and spectra of Earth-like planets orbiting the entire grid of M dwarfs for...
We present model atmospheres for an Earth-like planet orbiting the entire grid of main sequence FGK...
International audienceA broad effort is ongoing with large spectroscopic surveys such as APOGEE, ESO...
This dataset contains the simulated high-resolution spectra and profiles of 360 different Earth-like...
Context. It remains difficult to interpret the near-IR emission of young stellar populations. One ma...
Supplementary material for 'Exploring H2O Prominence in Reflection Spectra of Cool Giant Planets ', ...
Atmospheres of transiting extrasolar giant planets (EGPs) such as HD 209458b must impose features on...
Interpreting the reflection spectra of cool giant planets will be a challenge. Spectra of such world...
Planets larger than Earth and smaller than Neptune are some of the most numerous in the galaxy, but ...
Spectroscopy is a tool for determining the composition and physical properties of a material. Becau...
Context. The atmosphere of Earth-like extrasolar planets orbiting different types of stars is influe...
This dataset contains the geometric albedo, spectra, and colors of 19 different Solar System objects...
An essential reference for researchers and students of planetary remote sensing on the interaction o...
Aims. A spectroscopic analysis of stellar spectra can be carried out using multiple approaches such ...
Planets larger than Earth and smaller than Neptune are some of the most numerous in the galaxy, but ...
We model the atmospheres and spectra of Earth-like planets orbiting the entire grid of M dwarfs for...
We present model atmospheres for an Earth-like planet orbiting the entire grid of main sequence FGK...
International audienceA broad effort is ongoing with large spectroscopic surveys such as APOGEE, ESO...
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