Sensitivity of biosignatures on Earth-like planets orbiting in the habitable zone of cool M-dwarf Stars to varying stellar UV radiation and surface biomass emissions-Reference-Cited by-同舟云学术

Sensitivity of biosignatures on Earth-like planets orbiting in the habitable zone of cool M-dwarf Stars to varying stellar UV radiation and surface biomass emissions

Published:2014-08 Issue: Volume:98 Page:66-76
ISSN:0032-0633
Container-title:Planetary and Space Science
language:en
Short-container-title:Planetary and Space Science

Author:

Grenfell J.L.,Gebauer S.,v. Paris P.,Godolt M.,Rauer H.

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

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4. The Ultraviolet radiation environment around M dwarf exoplanet host stars;France;Astrophys. J.,2013

5. Sensitivity of biomarkers to changes in chemical emissions in Earth's Proterozoic atmosphere;Grenfell;Icarus,2011

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