The direct detection of reflected starlight from exoplanets marks the beginning of a new era in the characterization of extrasolar planetary atmospheres. The flux and in particular the linear polarization signals from such planets are sensitive to atmospheric structure and composition, but other effects may also contribute to observed signals. We investigate the influence of an exoplanet’s shape and orbitorientation on its flux and polarization signature, and compare it against the influence of a variable cloud cover.Astrodynamics & Space Mission
We present results of numerical simulations of flux F and degree of polarization P of light that is...
Using numerical simulations of flux and polarization spectra of visible to near-infrared starlight ...
Context. Clouds have already been detected in exoplanetary atmospheres. They play crucial roles in a...
Polarimetry has already played an important role in the characterization of planets within the solar...
Aims. We present numerically calculated, disk-integrated, spectropolarimetric signals of starlight t...
Aims. We present numerically calculated, disk-integrated, spectropolarimetric signals of starlight t...
We present results of numerical simulations of flux F and degree of polarization P of light that is ...
The detection of moons around extrasolar planets is one of the main focuses of current and future ob...
Because clouds scatter and absorb incident radiation, they play crucial roles in the radiative balan...
Using numerical simulations of flux and polarization spectra of visible to near-infrared starlight r...
Context. Terrestrial-type exoplanets in or near stellar habitable zones appear to be ubiquitous. It ...
It is becoming clear that the atmospheres of the young, self-luminous extrasolar gi-ant planets imag...
It is less than 20 years since astronomers discovered the first exoplanet orbiting a Sun-like star. ...
It is becoming clear that the atmospheres of the young, self-luminous extrasolar gi-ant planets imag...
Aims. We present modeled flux and linear polarization signals of starlight that is reflected by spat...
We present results of numerical simulations of flux F and degree of polarization P of light that is...
Using numerical simulations of flux and polarization spectra of visible to near-infrared starlight ...
Context. Clouds have already been detected in exoplanetary atmospheres. They play crucial roles in a...
Polarimetry has already played an important role in the characterization of planets within the solar...
Aims. We present numerically calculated, disk-integrated, spectropolarimetric signals of starlight t...
Aims. We present numerically calculated, disk-integrated, spectropolarimetric signals of starlight t...
We present results of numerical simulations of flux F and degree of polarization P of light that is ...
The detection of moons around extrasolar planets is one of the main focuses of current and future ob...
Because clouds scatter and absorb incident radiation, they play crucial roles in the radiative balan...
Using numerical simulations of flux and polarization spectra of visible to near-infrared starlight r...
Context. Terrestrial-type exoplanets in or near stellar habitable zones appear to be ubiquitous. It ...
It is becoming clear that the atmospheres of the young, self-luminous extrasolar gi-ant planets imag...
It is less than 20 years since astronomers discovered the first exoplanet orbiting a Sun-like star. ...
It is becoming clear that the atmospheres of the young, self-luminous extrasolar gi-ant planets imag...
Aims. We present modeled flux and linear polarization signals of starlight that is reflected by spat...
We present results of numerical simulations of flux F and degree of polarization P of light that is...
Using numerical simulations of flux and polarization spectra of visible to near-infrared starlight ...
Context. Clouds have already been detected in exoplanetary atmospheres. They play crucial roles in a...