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- W2106074368 abstract "Atmospheric temperature and mixing ratio profiles of terrestrial planets vary with the spectral energy flux distribution for different types of M-dwarf stars and the planetary gravity. We investigate the resulting effects on the spectral appearance of molecular absorption bands, which are relevant as indicators for potential planetary habitability during primary and secondary eclipse for transiting terrestrial planets with Earth-like biomass emissions. Atmospheric profiles are computed using a plane-parallel, 1D climate model coupled with a chemistry model. We then calculate simulated spectra using a line-by-line radiative transfer model." @default.
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- W2106074368 date "2011-03-21" @default.
- W2106074368 modified "2023-10-16" @default.
- W2106074368 title "Potential biosignatures in super-Earth atmospheres" @default.
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- W2106074368 doi "https://doi.org/10.1051/0004-6361/201014368" @default.
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