We characterize the atmosphere of the iconic giant planet HD209458 b based on a joint modeling effort of the available observations. HD 209458 b is the first...
Revised Parameter Estimates For The Most Metal-Poor Candidates In SDSS-I And SEGUE
There are several hundred thousand R = 2000 stellar spectra reported in the final public release of the Sloan Digital Sky Survey (SDSS-I) and the continuing...
Revised Parameter Estimates For The Most Metal-poor Candidates In SDSS-I And SEGUE
There are several hundred thousand R = 2000 stellar spectra reported in the final public release of the Sloan Digital Sky Survey (SDSS-I) and the continuation...
Revised parameters for OGLE-TR-10 from UVES spectra: updated planetary physical properties
We have obtained high-resolution UVES spectra with S/N>100 to accurately characterize the stellar parameters for the transiting planet-hosting star OGLE-TR-10...
Revisiting NGC 3109: A Systematic Blue Massive Stars Analysis
In the last years thoughtful quantitative analyses of extragalactic blue massive stars have shown not only that these studies are doable even at large distances...
Revisiting the (V/sigma,epsilon) anisotropy diagram of early-type galaxies using integral-field kinematics
We use integral-field observation of the stellar kinematics obtained with SAURON in combination with Schwarzschild dynamical models to revisit our understanding...
Revisiting the atmosphere of HD 209458b with HARPS-N, CARMENES and ESPRESSO
HD 209458b was the first transiting planet discovered, and the first for which its atmosphere, in particular Na I, was detected. With time, it has become one of...