Showing 1–20 of 28 results
/ Date/ Name
Mar 20, 2026Coma Physics of an Interstellar Object: JWST Spatial-Spectral Mapping of 3I/ATLASJan 13, 2026Anatomy of Empirical Transit Spectra of Mars based on TGO/NOMADOct 21, 2025Chemistry, Climate, and Transmission Spectra of TRAPPIST-1 e Explored with a Multimodel Sparse Sampled EnsembleAug 18, 2025A comprehensive spectroscopic reference of the solar system and its application to exoplanet direct imagingJul 11, 2025From Global Climate Models (GCMs) to Exoplanet Spectra with the Global Emission Spectra (GlobES)Jun 13, 2024The CUISINES Framework for Conducting Exoplanet Model Intercomparison Projects, Version 1.0Jun 4, 2024Abundances of trace constituents in Jupiter's atmosphere inferred from Herschel/PACS observationsApr 8, 2024ALMA Spectroscopy of Europa: A Search for Active PlumesJan 30, 2024Revealing Callisto's carbon-rich surface and CO2 atmosphere with JWSTAug 29, 2023Water Condensation Zones around Main Sequence StarsDec 9, 2022GCM Constraints on the Detectability of the CO$_2$-CH$_4$ Biosignature Pair on TRAPPIST-1e with JWSTOct 24, 2022Phosphine in the Venusian Atmosphere: A Strict Upper Limit from SOFIA GREAT ObservationsJun 30, 2021Simulating Reflected Light Exoplanet Spectra of the Promising Direct Imaging Target, $\upsilon$ Andromedae d, with a New, Fast Sampling Method Using the Planetary Spectrum GeneratorJan 18, 2021Probing the capability of future direct imaging missions to spectrally constrain the frequency of Earth-like planetsAug 10, 2020Non-detection of O$_2$/O$_3$ informs frequency of Earth-like planets with LUVOIR but not HabExJan 6, 2020Sensitive Probing of Exoplanetary Oxygen via Mid Infrared Collisional AbsorptionJan 3, 2020The First Habitable Zone Earth-sized Planet from TESS. III: Climate States and Characterization Prospects for TOI-700 dJan 3, 2020The First Habitable Zone Earth-sized Planet from TESS. I: Validation of the TOI-700 SystemDec 17, 2019Dim Prospects for Transmission Spectra of Ocean Earths Around M StarsOct 12, 2018Methane on Mars: New insights into the sensitivity of CH4 with the NOMAD/ExoMars spectrometer through its first in-flight calibration