Results 91 to 100 of about 15,700 (208)
Radiative transfer (RT) models are critical in the interpretation of exoplanetary spectra, in simulating exoplanet climates, and when designing the specifications of future flagship observatories.
Geronimo L. Villanueva +17 more
doaj +1 more source
Theoretical frameworks for reflection and emission spectroscopy of exoplanet surfaces are becoming increasingly important for the characterization of rocky exoplanets, especially with the rapid growth of the detected exoplanet population and ...
Leonardos Gkouvelis
doaj +1 more source
Mapping out the time-evolution of exoplanet processes [PDF]
Jessie L. Christiansen +4 more
openalex +1 more source
Comprehensive Parameter Determination of Exoplanets through Asteroseismic Host Star Constraints
This study develops a robust framework for exoplanet characterization by leveraging asteroseismic constraints on host stars. Using precise photometric data from missions such as Kepler and TESS, we derive stellar parameters, including mass, radius, and ...
Wen-Xu Lin +7 more
doaj +1 more source
Pale Orange Dots: The Impact of Organic Haze on the Habitability and Detectability of Earthlike Exoplanets [PDF]
Giada N. Arney +7 more
openalex +1 more source
The CUISINES Framework for Conducting Exoplanet Model Intercomparison Projects, Version 1.0
As JWST begins to return observations, it is more important than ever that exoplanet climate models can consistently and correctly predict the observability of exoplanets, retrieval of their data, and interpretation of planetary environments from that ...
Linda E. Sohl +12 more
doaj +1 more source
The present-day bulk elemental composition of an exoplanet can provide insight into a planet’s formation and evolutionary history. Such information is now being measured for dozens of planets with state-of-the-art facilities using Bayesian atmosphere ...
Joshua D. Lothringer +2 more
doaj +1 more source

