Aims. The knowledge of how the specific intensity is distributed over the stellar disk is crucial for interpreting the light curves of extrasolar transiting planets, double-lined eclipsing binaries, and other astrophysical phenomena. To provide theoretical inputs for light curve modelling codes, we present new calculations of limb-darkening coefficients for the spherically symmetric phoeni
The ability to observe extrasolar planets transiting their stars has profoundly changed our understa...
Aims. There are very few comparisons between theoretical and empirical limb-darkening coefficients (...
This paper examines how to compare stellar limb-darkening coefficients evaluated from model atmosphe...
Aims. The knowledge of how the specific intensity is distributed over the stellar disk is crucial fo...
Aims. We present an extension of our investigations on limb-darkening coefficients computed with sph...
Context. The phenomenon of limb-darkening is relevant to many topics in astrophysics, including the ...
Context. The detection of the first exoplanet paved the way for the era of transit-photometry space ...
Aims. One of the biggest problems we can encounter while dealing with the limb-darkening coefficient...
Aims. One of the biggest problems we can encounter while dealing with the limb-darkening coefficient...
Aims. We present new calculations of limb and gravity-darkening coefficients to be used as input in ...
Aims. The numerical methods used to compute limb-darkening coefficients (LDCs) are still a matter of...
The detection of the first exoplanet paved the way into the era of transit photometry space missions...
International audienceTransiting exoplanets provide unparalleled access to the fundamental parameter...
Aims. We present new gravity and limb-darkening coefficients for a wide range of effective temperatu...
Aims. The complex physics of close binary stars is made even more challenging by the proximity effec...
The ability to observe extrasolar planets transiting their stars has profoundly changed our understa...
Aims. There are very few comparisons between theoretical and empirical limb-darkening coefficients (...
This paper examines how to compare stellar limb-darkening coefficients evaluated from model atmosphe...
Aims. The knowledge of how the specific intensity is distributed over the stellar disk is crucial fo...
Aims. We present an extension of our investigations on limb-darkening coefficients computed with sph...
Context. The phenomenon of limb-darkening is relevant to many topics in astrophysics, including the ...
Context. The detection of the first exoplanet paved the way for the era of transit-photometry space ...
Aims. One of the biggest problems we can encounter while dealing with the limb-darkening coefficient...
Aims. One of the biggest problems we can encounter while dealing with the limb-darkening coefficient...
Aims. We present new calculations of limb and gravity-darkening coefficients to be used as input in ...
Aims. The numerical methods used to compute limb-darkening coefficients (LDCs) are still a matter of...
The detection of the first exoplanet paved the way into the era of transit photometry space missions...
International audienceTransiting exoplanets provide unparalleled access to the fundamental parameter...
Aims. We present new gravity and limb-darkening coefficients for a wide range of effective temperatu...
Aims. The complex physics of close binary stars is made even more challenging by the proximity effec...
The ability to observe extrasolar planets transiting their stars has profoundly changed our understa...
Aims. There are very few comparisons between theoretical and empirical limb-darkening coefficients (...
This paper examines how to compare stellar limb-darkening coefficients evaluated from model atmosphe...
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