Showing 81–100 of 103 results
/ Date/ Name
Jul 22, 2024Time Allocation and Long-Term Scheduling of ESO Telescopes at La Silla Paranal ObservatorySep 24, 2001Stellar populations in NGC 5128 with the VLT: evidence for recent star formationSep 24, 2001The radio/optical alignment and the recent star formation associated with ionized filaments in the halo of NGC 5128 (Centaurus A)Mar 15, 2007Bright globular clusters in NGC 5128: the missing link between young massive clusters and evolved massive objectsSep 14, 2023Expanding on the Fundamental Metallicity Relation in Dwarf Galaxies with MUSEOct 14, 2009Integrated K-band spectra of old and intermediate-age globular clusters in the Large Magellanic CloudJun 15, 2022Galaxy populations in the Hydra I cluster from the VEGAS survey II. The ultra-diffuse galaxy populationAug 22, 2023Looking into the faintEst WIth MUSE (LEWIS): on the nature of ultra-diffuse galaxies in the Hydra-I cluster.I. Project description and preliminary resultsAug 22, 2023Ultra diffuse galaxies in the Hydra I cluster from the LEWIS Project: Phase-Space distribution and globular cluster richnessOct 31, 2023The ESO Science Archive Facility: Status, Impact, and ProspectsJun 15, 2011New Galactic Star Clusters Discovered in the VVV SurveyAug 2, 2024Galaxy populations in the Hydra I cluster from the VEGAS survey III. The realm of low surface brightness features and intra-cluster lightJun 3, 2017The difference in metallicity distribution functions of halo stars and globular clusters as a function of galaxy type: A tracer of globular cluster formation and evolutionJun 12, 2014VISTA Variables in the Vía Láctea (VVV): Halfway Status and ResultsDec 5, 2016Prolate rotation and metallicity gradient in the transforming dwarf galaxy PhoenixFeb 3, 2017Large Magellanic Cloud Near-Infrared Synoptic Survey. IV. Leavitt Laws for Type II Cepheid VariablesJul 14, 2025Absolute Calibration of Cluster Mira Variables to Provide a New Anchor for the Hubble Constant DeterminationDec 20, 2025Unlocking the physics of dwarf galaxies in the 2040s: The case for a next-generation wide-field spectroscopic facility with fibres and IFUsNov 18, 2010How old are the stars in the halo of NGC 5128 (Centaurus A)?Jan 18, 2012Globular cluster luminosity function as distance indicator