DOIAbstract
Aims. We present an extension of our investigations on limb-darkening coefficients computed with spherical symmetrical Phoeni
Aims. We present an extension of our investigations on limb-darkening coefficients computed with spherical symmetrical Phoeni
Model stellar atmospheres are fundamental tools for understanding stellar observations from interfer...
Continuing our studies on stellar atmospheres (Claret [CITE], [CITE]), we present in this paper the ...
Limb darkening is a fundamental ingredient for interpreting observations of planetary transits, ecli...
Aims. We present an extension of our investigations on limb-darkening coefficients computed with sph...
Aims. The knowledge of how the specific intensity is distributed over the stellar disk is crucial fo...
Context. The phenomenon of limb-darkening is relevant to many topics in astrophysics, including the ...
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 ...
The detection of the first exoplanet paved the way into the era of transit photometry space missions...
Context. The detection of the first exoplanet paved the way for the era of transit-photometry space ...
Aims. We present new gravity and limb-darkening coefficients for a wide range of effective temperatu...
First official grid of stellar limb-darkening coefficients and intensity profiles computed by the co...
Aims. The numerical methods used to compute limb-darkening coefficients (LDCs) are still a matter of...
As an extension of our previous investigations on stellar atmospheres (Claret [CITE]), the limb-dar...
Model stellar atmospheres are fundamental tools for understanding stellar observations from interfer...
Continuing our studies on stellar atmospheres (Claret [CITE], [CITE]), we present in this paper the ...
Limb darkening is a fundamental ingredient for interpreting observations of planetary transits, ecli...
Aims. We present an extension of our investigations on limb-darkening coefficients computed with sph...
Aims. The knowledge of how the specific intensity is distributed over the stellar disk is crucial fo...
Context. The phenomenon of limb-darkening is relevant to many topics in astrophysics, including the ...
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 ...
The detection of the first exoplanet paved the way into the era of transit photometry space missions...
Context. The detection of the first exoplanet paved the way for the era of transit-photometry space ...
Aims. We present new gravity and limb-darkening coefficients for a wide range of effective temperatu...
First official grid of stellar limb-darkening coefficients and intensity profiles computed by the co...
Aims. The numerical methods used to compute limb-darkening coefficients (LDCs) are still a matter of...
As an extension of our previous investigations on stellar atmospheres (Claret [CITE]), the limb-dar...
Model stellar atmospheres are fundamental tools for understanding stellar observations from interfer...
Continuing our studies on stellar atmospheres (Claret [CITE], [CITE]), we present in this paper the ...
Limb darkening is a fundamental ingredient for interpreting observations of planetary transits, ecli...
Add to ORKG