Results 71 to 80 of about 68,799 (245)

Analysis of Habitability and Stellar Habitable Zones from Observed Exoplanets

open access: yesGalaxies
The investigation of exoplanetary habitability is integral to advancing our knowledge of extraterrestrial life potential and detailing the environmental conditions of distant worlds. In this analysis, we explore the properties of exoplanets situated with
Jonathan H. Jiang   +4 more
doaj   +1 more source

A Revised Exoplanet Yield from the Transiting Exoplanet Survey Satellite (TESS) [PDF]

open access: yesAstrophysical Journal Supplement Series, 2018
The Transiting Exoplanet Survey Satellite (TESS) has a goal of detecting small planets orbiting stars bright enough for mass determination via ground-based radial velocity observations.
T. Barclay, J. Pepper, E. Quintana
semanticscholar   +1 more source

Why Is it So Cold in Here? Explaining the Cold Temperatures Retrieved from Transmission Spectra of Exoplanet Atmospheres [PDF]

open access: yesAstrophysical Journal, 2020
Transmission spectroscopy is a powerful technique widely used to probe exoplanet terminators. Atmospheric retrievals of transmission spectra are enabling comparative studies of exoplanet atmospheres.
R. MacDonald, J. Goyal, N. Lewis
semanticscholar   +1 more source

Gliese 581g as a scaled-up version of Earth: atmospheric circulation simulations

open access: yes, 2011
We use three-dimensional simulations to study the atmospheric circulation on the first Earth-sized exoplanet discovered in the habitable zone of an M star.
Anderson   +48 more
core   +1 more source

The Ultraviolet Radiation Environment Around M dwarf Exoplanet Host Stars [PDF]

open access: yes, 2012
The spectral and temporal behavior of exoplanet host stars is a critical input to models of the chemistry and evolution of planetary atmospheres. At present, little observational or theoretical basis exists for understanding the ultraviolet spectra of M ...
Bushinsky, Rachel   +10 more
core   +4 more sources

The MUSCLES Extension for Atmospheric Transmission Spectroscopy: UV and X-Ray Host-star Observations for JWST ERS & GTO Targets

open access: yesThe Astronomical Journal, 2023
X-ray through infrared spectral energy distributions (SEDs) are essential for understanding a star’s effect on exoplanet atmospheric composition and evolution. We present a catalog of panchromatic SEDs, hosted on the Barbara A. Mikulski Archive for Space
Patrick R. Behr   +10 more
doaj   +1 more source

PERICLES: A Set of Empirical Rotational Isochrones Modeled on Cool Dwarfs in Open Clusters and Wide Binaries

open access: yesAstronomische Nachrichten, EarlyView.
ABSTRACT Isochrones, equal‐age curves, are widely used in astrophysics to estimate stellar ages. Classical stellar parameters are, however, very limited in their usability for main sequence stars because of their weak age‐dependence. Here, rotation period measurements provide complementary information.
David Gruner, Sydney A. Barnes
wiley   +1 more source

Investigation of Kepler Objects of Interest Stellar Parameters from Observed Transit Durations [PDF]

open access: yes, 2013
The Kepler mission discovery of candidate transiting exoplanets (KOIs) enables a plethora of ensemble analysis of the architecture and properties of exoplanetary systems.
Bilinski, Christopher   +2 more
core   +2 more sources

The single beacon: progresses in understanding Earth as an exoplanet using DSCOVR/EPIC observations

open access: yesFrontiers in Remote Sensing
Almost 6000 exoplanets have thus far been confirmed, revolutionizing our understanding of planetary habitability. Yet, despite the identification of Earth-like exoplanets, definitive evidence of extraterrestrial life remains elusive.
Xun Jian   +9 more
doaj   +1 more source

Kepler Observations of the Three Pre-Launch Exoplanet Candidates: Discover of Two Eclipsing Binaries and a New Exoplanet [PDF]

open access: yes, 2010
Three transiting exoplanet candidate stars were discovered in a ground-based photometric survey prior to the launch of NASA's Kepler mission. Kepler observations of them were obtained during Quarter 1 of the Kepler mission.
Bryson, Stephen T.   +8 more
core  

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