High-Resolution Spectra of Habitable Zone Planets

This dataset contains the simulated high-resolution spectra and profiles of 360 different Earth-like exoplanets around 12 different host star types and 30 different surface types. <strong>Journal article for spectra:</strong> Madden &amp; Kaltenegger (2020) High-resolution Spectra for a Wide Range of Habitable Zone Planets around Sun-like Stars. ApJL (https://doi.org/10.3847/2041-8213/aba535) <strong>Journal article for profiles:</strong> Madden &amp; Kaltenegger (2020) How surfaces shape the climate of habitable exoplanets. MNRAS (https://doi.org/10.1093/mnras/staa387) <em><strong>Contents</strong></em> <em>ExampleSpectra_Total_HighRes.txt</em><strong> </strong>- This is a sample spectrum to get familiar with working with the data. All spectrum files are in \(W/m^2/\mu m\) and match with the included wavelength grid. <em>WavelengthGrid_Microns_HighRes.txt </em>- Wavelength grid is spaced at \(0.01cm^{-1}\) intervals and converted to microns from 0.4 to 20. <em>Spectra_Total_HighRes.zip</em> - Contains the combined emission and reflection spectra of all 360 simulations. All spectrum files are in \(W/m^2/\mu m\) and match with the included wavelength grid. <em>Spectra_ReflectanceOnly_HighRes.zip</em> - Contains just the reflection spectra of all 360 simulations. All spectrum files are in \(W/m^2/\mu m\) and match with the included wavelength grid. <em>Spectra_EmissionOnly_HighRes.zip</em> - Contains just the emission spectra of all 360 simulations. All spectrum files are in \(W/m^2/\mu m\) and match with the included wavelength grid. <em>Profiles.zip </em>- Contains the mixing ratios, temperature (K), and pressure (bar) profiles with altitude (cm) for each simulation.