Showing 121–140 of 157 results
/ Date/ Name
May 30, 2016Fast-slow bursters in the unfolding of a high codimension singularity and the ultra-slow transitions of classesFeb 25, 2016State of the Field: Extreme Precision Radial VelocitiesAug 18, 2015The SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Overview and Early DataJul 17, 2015Origin of optical losses in gallium arsenide disk whispering gallery resonatorsJun 22, 2015Euro-VO - Coordination of Virtual Observatory activities in EuropeMar 6, 2015Kuiper belt structure around nearby super-Earth host starsFeb 19, 2015The EChO science caseJan 5, 2015The Eleventh and Twelfth Data Releases of the Sloan Digital Sky Survey: Final Data from SDSS-IIIDec 2, 2014The VLTI / PIONIER near-infrared interferometric survey of southern T Tauri stars. I. First resultsNov 24, 2014Macroscopic Polarization Rotation Induced by a Single SpinMay 30, 2014The Kepler-10 planetary system revisited by HARPS-N: A hot rocky world and a solid Neptune-mass planetMay 5, 2014IGM Constraints from the SDSS-III/BOSS DR9 Ly-alpha Forest Flux Probability Distribution FunctionOct 6, 2013PRISM (Polarized Radiation Imaging and Spectroscopy Mission): An Extended White PaperSep 19, 2013Gas lines from the 5-Myr old optically thin disk around HD141569A. Herschel observations and modelingJul 29, 2013The Tenth Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the SDSS-III Apache Point Observatory Galactic Evolution ExperimentJul 15, 2013The Subaru Coronagraphic Extreme Adaptive Optics Imager: First Results and On-Sky PerformanceJun 10, 2013The Hot and Energetic Universe: A White Paper presenting the science theme motivating the Athena+ missionJul 31, 2012The Baryon Oscillation Spectroscopic Survey of SDSS-IIIJul 30, 2012The Ninth Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the SDSS-III Baryon Oscillation Spectroscopic SurveyJul 30, 2012Intricate visibility effects from resolved emission of young stellar objects: the case of MWC158 observed with the VLTI