Stellar limb darkening. A new MPS-ATLAS library for Kepler, TESS, CHEOPS, and PLATO passbands
arXiv:2206.06641 · doi:10.1051/0004-6361/202243722
Abstract
The detection of the first exoplanet paved the way into the era of transit photometry space missions with a revolutionary photometric precision that aim at discovering new exoplanetary systems around different types of stars. With this high precision, it is possible to derive very accurately the radii of exoplanets which is crucial for constraining their type and composition. However, it requires an accurate description of host stars, especially their center-to-limb variation of intensities (so called limb darkening) as it affects the planet-to-star radius ratio determination. We aim at improving the accuracy of limb darkening calculations for stars with a wide range of fundamental parameters. We used the recently developed 1D MPS-ATLAS code to compute model atmosphere structures and to synthesize stellar limb darkening on a very fine grid of stellar parameters. For the computations we utilized the most accurate information on chemical element abundances and mixing length parameters including convective overshoot. The stellar limb darkening was fitted using the two most accurate limb darkening laws: the power-2 and 4-parameters non-linear laws. We present a new extensive library of stellar model atmospheric structures, the synthesized stellar limb darkening curves, and the coefficients of parameterized limb-darkening laws on a very fine grid of stellar parameters in the Kepler, TESS, CHEOPS, and PLATO passbands. The fine grid allows overcoming the sizable errors introduced by the need to interpolate. Our computations of solar limb darkening are in a good agreement with available solar measurements at different view angles and wavelengths. Our computations of stellar limb darkening agree well with available measurements of Kepler stars. A new grid of stellar model structures, limb darkening and their fitted coefficients in different broad filters is provided in CDS.
arXiv comment19 pages, 17 figures, accepted to Astronomy and Astrophysics. All tables are available in CDS
References in corpus (29)
- The chemical composition of the Sun
- The Transiting Exoplanet Survey Satellite
- A grid of MARCS model atmospheres for late-type stars I. Methods and general properties
- A new extensive library of PHOENIX stellar atmospheres and synthetic spectra
- Detection of Planetary Transits Across a Sun-like Star
- The PLATO 2.0 Mission
- The NextGen Model Atmosphere grid for $3000\le \Teff \le 10000\K$
- Theoretical Transmission Spectra During Extrasolar Giant Planet Transits
- Transmission Spectra as Diagnostics of Extrasolar Giant Planet Atmospheres
- Homogeneous studies of transiting extrasolar planets. I. Light curve analyses
- Limb and gravity-darkening coefficients for the TESS satellite at several metallicities, surface gravities, and microturbulent velocities
- Stellar Limb-Darkening Coefficients for CoRot and Kepler
- The Stagger-grid: A Grid of 3D Stellar Atmosphere Models - I. Methods and General Properties
- Limb darkening and exoplanets: testing stellar model atmospheres and identifying biases in transit parameters
- The Stagger-grid: A grid of 3D stellar atmosphere models - IV. Limb darkening coefficients
- The effect of stellar limb darkening values on the accuracy of the planet radii derived from photometric transit observations
- How realistic are solar model atmospheres?
- Limb-darkening and exoplanets II: Choosing the Best Law for Optimal Retrieval of Transit Parameters
- High-precision stellar limb-darkening in exoplanetary transits
- The ExoTETHyS package: Tools for Exoplanetary Transits around Host Stars
- Investigating the Metallicity-Mixing Length Relation
- Comparison of the power-2 limb-darkening law from the Stagger-grid to Kepler light curves of transiting exoplanets
- Measuring stellar granulation during planet transits
- Transiting exoplanets from the CoRoT space mission. XIII. CoRoT-13b: a dense hot Jupiter in transit around a star with solar metallicity and super-solar lithium content
- Transiting exoplanets from the CoRoT space mission. XII. CoRoT-12b: a short-period low-density planet transiting a solar analog star
- MPS-ATLAS: A fast all-in-one code for synthesising stellar spectra
- In-flight photometry extraction of PLATO targets: Optimal apertures for detecting extrasolar planets
- Center-to-limb polarization in continuum spectra of F, G, K stars
- Opacity distribution functions for stellar spectra synthesis
Cited by in corpus (11)
- ExoTiC-LD: thirty seconds to stellar limb-darkening coefficients
- New rotation period measurements of 67,163 Kepler stars
- Can 1D radiative equilibrium models of faculae be used for calculating contamination of transmission spectra?
- Insufficient evidence for DMS and DMDS in the atmosphere of K2-18 b. From a joint analysis of JWST NIRISS, NIRSpec, and MIRI observations
- JWST COMPASS: NIRSpec/G395H Transmission Observations of the Super-Earth TOI-776b
- Additional JWST/NIRSpec Transits of the Rocky M Dwarf Exoplanet GJ 1132 b Reveal a Featureless Spectrum
- Cloudy mornings and clear evenings on a gas giant exoplanet
- GEMS JWST: Transmission spectroscopy of TOI-5205b reveals significant stellar contamination and a metal-poor atmosphere
- The EBLM project -- XIV. TESS light curves for eclipsing binaries with very low mass companions
- First release of PLATO consortium stellar limb-darkening coefficients
- Modeling HMI observables for the study of solar oscillations