Showing 1–20 of 32 results
/ Date/ Name
Jul 30, 2024TOI-757 b: an eccentric transiting mini-Neptune on a 17.5-d orbitJun 3, 2024CHEOPS in-flight performance: A comprehensive look at the first 3.5 years of operationsApr 25, 2024Tau Herculids 2022 from the McDonald Observatory, Texas -- a progress reportMar 25, 2024Precise characterisation of HD 15337 with CHEOPS: a laboratory for planet formation and evolutionNov 29, 2023A resonant sextuplet of sub-Neptunes transiting the bright star HD 110067Jun 7, 2023TOI-5678 b: A 48-day transiting Neptune-mass planet characterized with CHEOPS and HARPSFeb 21, 2023TOI-1055 b: Neptunian planet characterised with HARPS, TESS, and CHEOPSFeb 20, 2023GRBAlpha: the smallest astrophysical space observatory -- Part 1: Detector design, system description and satellite operationsFeb 20, 2023The peak-flux of GRB 221009A measured with GRBAlphaJul 28, 2022The HD 93963 A transiting system: A 1.04d super-Earth and a 3.65 d sub-Neptune discovered by TESS and CHEOPSFeb 9, 2022Rotation periods and shape asphericity in asteroid families based on TESS S1-S13 observationsJan 19, 2022Investigating the architecture and internal structure of the TOI-561 system planets with CHEOPS, HARPS-N and TESSFeb 18, 2021101 Trojans: a tale of period bimodality, binaries, and extremely slow rotators from K2 photometryJan 16, 2020Solar System objects observed with TESS -- First data release: bright main-belt and Trojan asteroids from the Southern SurveyJun 6, 2016Possibility for albedo estimation of exomoons: Why should we care about M dwarfs?Jul 18, 2012Testing SNe Ia distance measurement methods with SN 2011feJan 4, 2010The asteroseismic potential of Kepler: first results for solar-type starsDec 31, 2009Kepler Asteroseismology Program: Introduction and First ResultsMay 28, 2009The Science Case for PILOT III: the Nearby UniverseMay 27, 2009The Science Case for PILOT I: Summary and Overview