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Science (New York, N.Y.)|September 8, 2022
Density, not radius, separates rocky and water-rich small planets orbiting M dwarf starsRafael Luque, Enric PalléNature|June 12, 2009
Earth's transmission spectrum from lunar eclipse observationsEnric Pallé, María Rosa Zapatero Osorio, Rafael Barrena, et al.Astrobiology|June 26, 2018
Exoplanet Biosignatures: Observational ProspectsYuka Fujii, Daniel Angerhausen, Russell Deitrick, et al.Nature|February 18, 2025
Vertical structure of an exoplanet's atmospheric jet streamJulia V Seidel, Bibiana Prinoth, Lorenzo Pino, et al.Experimental Astronomy|March 14, 2023
Atmospheric characterization of terrestrial exoplanets in the mid-infrared: biosignatures, habitability, and diversitySascha P Quanz, Olivier Absil, Willy Benz, et al.Science (New York, N.Y.)|December 8, 2018
Ground-based detection of an extended helium atmosphere in the Saturn-mass exoplanet WASP-69bLisa Nortmann, Enric Pallé, Michael Salz, et al.Nature|January 7, 2026
A young progenitor for the most common planetary systems in the GalaxyJohn H Livingston, Erik A Petigura, Trevor J David, et al.Nature|May 17, 2023
A temperate Earth-sized planet with tidal heating transiting an M6 starMerrin S Peterson, Björn Benneke, Karen Collins, et al.Nature|March 13, 2020
Nightside condensation of iron in an ultrahot giant exoplanetDavid Ehrenreich, Christophe Lovis, Romain Allart, et al.Science (New York, N.Y.)|February 12, 2026
Gas-depleted planet formation occurred in the four-planet system around the red dwarf LHS 1903Thomas G Wilson, Anna M Simpson, Andrew Collier Cameron, et al.Pageof 1