The effect of stellar contamination on low-resolution transmission spectroscopy: needs identified by NASA's Exoplanet Exploration Program Study Analysis Group 21
BV Rackham, N Espinoza… - RAS Techniques …, 2023 - academic.oup.com
Abstract Study Analysis Group 21 (SAG21) of NASA's Exoplanet Exploration Program
Analysis Group was organized to study the effect of stellar contamination on space-based …
Analysis Group was organized to study the effect of stellar contamination on space-based …
Effects of a fully 3D atmospheric structure on exoplanet transmission spectra: retrieval biases due to day–night temperature gradients
A Caldas, J Leconte, F Selsis, IP Waldmann… - Astronomy & …, 2019 - aanda.org
Transmission spectroscopy provides us with information on the atmospheric properties at
the limb, which is often intuitively assumed to be a narrow annulus around the planet …
the limb, which is often intuitively assumed to be a narrow annulus around the planet …
Planetary candidates observed by Kepler. VIII. A fully automated catalog with measured completeness and reliability based on data release 25
SE Thompson, JL Coughlin, K Hoffman… - The Astrophysical …, 2018 - iopscience.iop.org
Abstract We present the Kepler Object of Interest (KOI) catalog of transiting exoplanets
based on searching 4 yr of Kepler time series photometry (Data Release 25, Q1–Q17). The …
based on searching 4 yr of Kepler time series photometry (Data Release 25, Q1–Q17). The …
The ExoTETHyS package: tools for exoplanetary transits around host stars
The ExoTETHyS Package: Tools for Exoplanetary Transits around Host Stars - IOPscience
This site uses cookies. By continuing to use this site you agree to our use of cookies. To find …
This site uses cookies. By continuing to use this site you agree to our use of cookies. To find …
High-precision stellar limb-darkening in exoplanetary transits
High-precision Stellar Limb-darkening in Exoplanetary Transits - IOPscience This site uses
cookies. By continuing to use this site you agree to our use of cookies. To find out more, see …
cookies. By continuing to use this site you agree to our use of cookies. To find out more, see …
The STAGGER-grid: A grid of 3D stellar atmosphere models-V. Synthetic stellar spectra and broad-band photometry
Context. The surface structures and dynamics of cool stars are characterised by the
presence of convective motions and turbulent flows which shape the emergent spectrum …
presence of convective motions and turbulent flows which shape the emergent spectrum …
Closeby Habitable Exoplanet Survey (CHES). I. Astrometric noise and planetary detection efficiency due to stellar spots and faculae
C Bao, J Ji, D Tan, G Chen, X Huang… - The Astronomical …, 2024 - iopscience.iop.org
Abstract The Closeby Habitable Exoplanet Survey (CHES) is dedicated to the astrometric
exploration for habitable-zone Earth-like planets orbiting solar-type stars in close proximity …
exploration for habitable-zone Earth-like planets orbiting solar-type stars in close proximity …
Stellar limb darkening-A new MPS-ATLAS library for Kepler, TESS, CHEOPS, and PLATO passbands
NM Kostogryz, V Witzke, AI Shapiro, SK Solanki… - Astronomy & …, 2022 - aanda.org
Context. The detection of the first exoplanet paved the way for the era of transit-photometry
space missions with revolutionary photometric precision, whose aim is to discover new …
space missions with revolutionary photometric precision, whose aim is to discover new …
Planet and star synergy at high-spectral resolution. A rationale for the characterization of exoplanet atmospheres-I. The infrared
A Chiavassa, M Brogi - Astronomy & Astrophysics, 2019 - aanda.org
Context. Spectroscopy of exoplanet atmospheres at high-resolving powers is rapidly gaining
popularity for measuring the presence of atomic and molecular species. While this technique …
popularity for measuring the presence of atomic and molecular species. While this technique …
Detectability of shape deformation in short-period exoplanets
B Akinsanmi, SCC Barros, NC Santos… - Astronomy & …, 2019 - aanda.org
Context. Short-period planets are influenced by the extreme tidal forces of their parent stars.
These forces deform the planets causing them to attain nonspherical shapes. The …
These forces deform the planets causing them to attain nonspherical shapes. The …