This paper is available on arxiv under CC 4.0 license.
Authors:
(1) Eleonora Alei, ETH Zurich, Institute for Particle Physics & Astrophysics & National Center of Competence in Research PlanetS;
(2) Björn S. Konrad, ETH Zurich, Institute for Particle Physics & Astrophysics & National Center of Competence in Research PlanetS;
(3) Daniel Angerhausen, ETH Zurich, Institute for Particle Physics & Astrophysics, National Center of Competence in Research PlanetS & Blue Marble Space Institute of Science;
(4) John Lee Grenfell, Department of Extrasolar Planets and Atmospheres (EPA), Institute for Planetary Research (PF), German Aerospace Centre (DLR)
(5) Paul Mollière, Max-Planck-Institut für Astronomie;
(6) Sascha P. Quanz, ETH Zurich, Institute for Particle Physics & Astrophysics & National Center of Competence in Research PlanetS;
(7) Sarah Rugheimer, Department of Physics, University of Oxford;
(8) Fabian Wunderlich, Department of Extrasolar Planets and Atmospheres (EPA), Institute for Planetary Research (PF), German Aerospace Centre (DLR);
(9) LIFE collaboration, www.life-space-mission.com.
Appendix A: Scattering of terrestrial exoplanets
Appendix C: Bayes’ factor analysis: other epochs
Appendix D: Cloudy scenarios: additional figures
The Bayesian retrieval framework introduced in Paper III and extended here has delivered insightful answers to the questions introduced in Section 1. These can be summarized as follows:
This paper is available on arxiv under CC 4.0 license.