UC Berkeley - eScholarship.org
We present the Polarization of Hot Exoplanets (PolHEx) code for modelling the total flux (F) and degree of linear Polarization (P).
The Radio & Plasma Wave Investigation (RPWI) for the JUpiter ICy ...ABSTRACT. We explore the occurrence and detectability of planet-planet occultations (PPOs) in exoplanet systems. These are events during which a planet ... Insights into the 10-100 GeV gamma-ray emission of pulsars from ...Depuis le lancement du premier satellite, Spoutnik, en 1957, les acti- vités spatiales en orbite terrestre produisent des débris spatiaux qui me-. Variability of white dwarf debris disks - Lund University PublicationsHigh contrast imaging (HCI) is one of the most challenging techniques for exoplanet detection, but also one of the most promising.
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