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Rossi, L.C.G. (author), Groot, Ashwyn (author), Fauchez, Thomas (author), Stam, D.M. (author)
Because clouds scatter and absorb incident radiation, they play crucial roles in the radiative balance, the atmospheric chemistry, climate, and thus the habitability
of a planet. Clouds usually affect the planet’s observables. We investigate here the effect of partial and variable cloud coverage on the light that is reflected by an
Earth...
abstract 2018
document
Mahapatra, G. (author), Stam, D.M. (author), Rossi, L.C.G. (author), Rodenhuis, M. (author), Snik, Frans (author), Keller, C.U. (author)
In this work, we analyse linear polarization data of the planet at a distance, obtained with the Extreme Polarimeter (ExPo) on the William Herschel Telescope
on La Palma. These spatially resolved, high-accuracy polarization observations of Venus show faint circular patterns centered on the sub-solar point that are absent in the flux...
abstract 2017
document
Rossi, L.C.G. (author), Stam, D.M. (author), Turbet, M. (author)
In this work, we analyse linear polarization data of the planet at a distance, obtained with the Extreme Polarimeter (ExPo) on the William Herschel Telescope
on La Palma. These spatially resolved, high-accuracy polarization observations of Venus show faint circular patterns centered on the sub-solar point that are absent in the flux...
abstract 2017
document
Berzosa Molina, Javier (author), Stam, D.M. (author), Rossi, L.C.G. (author)
The detection of moons around extrasolar planets is one of the main focuses of current and future observatories. These silent companions contribute to the planets' observed signals but are barely detectable with current methods. Numerous gaseous exoplanets are known to orbit in the habitable zones of stars, and the expected abundance of natural...
abstract 2017
document
Palmer, Chris (author), Rossi, L.C.G. (author), Stam, D.M. (author)
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....
abstract 2017
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