Repositorio Institucional de la Universidad de Oviedo

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This research was supported by the following programs, grants, and fellowships: Spanish Ministry for Science, Innovation and Universities (MCIU) ESP2014-54062-R, ESP2014-54362P, AYA2015-69350-C3-2-P, BES-2015-074542, AYA2016-79425-C3-1/2/3-P, ESP2016-76076-R, ESP2016-80435-C2-1-R, ESP2016-80435-C2-2-R, ESP2017-87143-R, ESP2017-87676-C05-02-R, ESP2017-87676-2-2, RYC2012-09913 (“Ramón y Cajal” program), and FPU15/01476; Israel Science Foundation grant 848/16; CONICYT-FONDECYT/Chile Postdoctorado 3180405; Deutsches Zentrum für Luft- un Raumfahrt (DLR) 50OW0204 and 50OO1501; Italian Minister of Instruction, University and Research (MIUR), FFABR 2017; University of Rome Tor Vergata, “Mission: Sustainability 2016” fund; European Research Council under the European Union Horizon 2020 research and innovation program 694513; Mexican national council for science and technology CONACYT, CVU 448248; the “Center of Excellence Severo Ochoa” award for the Instituto de Astrofísica de Andalucía (SEV-2017-0709); Generalitat de Catalunya/CERCA program; Fondo Europeo de Desarrollo Regional (FEDER); German Science Foundation (DFG) Research Unit FOR2544 “Blue Planets around Red Stars” and Priority Programs SPP 1833, “Building a Habitable Earth,” and SPP 1992, “Exploring the Diversity of Extrasolar Planets”; NSF grants PHY17-48958 and PHY-1607761; Swiss National Science Foundation under grant BSGI0_155816 “PlanetsInTime” and within the framework of the NCCR PlanetS; Queen Mary University of London Scholarship and STFC Consolidated Grant ST/P000592/1; Spanish MCIU FPI-SO predoctoral contract BES-2017-082610; and the Knut and Alice Wallenberg Foundation