Evaluating the Plausible Range of N2O Biosignatures on ExoEarths: Flux-Abundance Relationships and Simulated Spectra for FGKM Main Sequence Stars
Edward Schwieterman1, Stephanie L. Olson2, Daria Pidhorodetska3, Christopher T. Reinhard4, Ainsley Ganti5, Thomas Fauchez6, Sandra Bastelberger7, Jaime Crouse3, Andy Ridgwell8 and Timothy Lyons1, (1)University of California Riverside, Department of Earth and Planetary Sciences, Riverside, CA, United States, (2)Purdue University, Department of Earth, Atmospheric, and Planetary Science, West Lafayette, IN, United States, (3)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (4)California Institute of Technology, Pasadena, United States, (5)The Potomac School, McLean, United States, (6)NASA GSFC, American University, Washington, United States, (7)ETH Swiss Federal Institute of Technology Zurich, Institute for Atmosphere and Climate Science, Zurich, Switzerland, (8)University of Bristol, School of Earth Sciences, Bristol, United Kingdom
