Showing 1–20 of 22 results
/ Date/ Name
Mar 30, 2012The Panchromatic Hubble Andromeda TreasuryMar 2, 2015A Comprehensive Archival Search for Counterparts to Ultra-Compact High Velocity Clouds: Five Local Volume Dwarf GalaxiesMar 1, 2026oMEGACat. IX. Chemical Tagging of Omega Centauri Populations with Machine-Learning-Inferred Abundances from the MUSE SpectrographSep 11, 2023The 50 Mpc Galaxy Catalog (50MGC): Consistent and Homogeneous Masses, Distances, Colors, and MorphologiesAug 10, 2012Three-integral multi-component dynamical models and simulations of the nuclear star cluster in NGC 4244May 29, 2014An optical--near-IR study of a triplet of super star clusters in the starburst core of M82Jan 20, 2021Hubble Space Telescope Imaging of Isolated Local Volume Dwarfs GALFA-Dw3 and Dw4Sep 5, 2023oMEGACat I: MUSE spectroscopy of 300,000 stars within the half-light radius of $ω$ CentauriJun 25, 2014Discovery of a new faint dwarf galaxy associated with NGC 253Feb 6, 2007GHOSTS: The Resolved Stellar Outskirts of Massive Disk GalaxiesAug 6, 2007Stellar populations across the NGC4244 truncated galactic diskApr 10, 2025X-ray Constraints on Wandering Black Holes in Stripped Galaxy Nuclei in the Halo of NGC 5128Apr 3, 2008Revised bolometric corrections and interstellar extinction coefficients for the ACS and WFPC2 photometric systemsMar 24, 2025Studying Binary Systems in Omega Centauri with MUSE: II. Observational constraints on the orbital period distributionSep 8, 2015Deep radio imaging of 47 Tuc identifies the peculiar X-ray source X9 as a new black hole candidateOct 30, 2025oMEGACat. VIII. A Subpopulation Census of ω CentauriSep 29, 2022X-ray and radio observations of central black holes in nearby low-mass early-type galaxies: Preliminary evidence for low Eddington fractionsFeb 24, 2017Hubble Space Telescope Imaging of the Ultra-Compact High Velocity Cloud AGC 226067: A stripped remnant in the Virgo ClusterSep 20, 2024oMEGACat IV: Constraining Ages of Omega Centauri sub-giant branch stars with HST and MUSEJun 3, 2024oMEGACat III. Multi-band photometry and metallicities reveal spatially well-mixed populations within $ω$ Centauri's half-light radius