Abstract Short-wavelength exoplanet transit measurements have been used to probe mass loss in atmospheres. We present the Swift-UVOT light curves for five hot Jupiters orbiting UV-bright F-type stars: XO-3, KELT-3, WASP-3, WASP-62, and HAT-P-6. report one positive detection of XO-3b marginal KELT-3b. place upper limits on remaining three depths. The planetary radii derived from NUV depths both ...

Albedo, spectral slopes, and water ice band depths maps for the five midsized saturnian satellites Mimas, Enceladus, Tethys, Dione, Rhea have been derived from Cassini-Visual Infrared Mapping Spectrometer (VIMS) data. The are systematically built photometric corrected data by applying Kaasalainen-Shkuratov model (Kaasalainen et al., 2001; Shkuratov 2011). In this work a quadratic function is us...