A dataset provided by the European Space Agency

Name 10260
Title The Most Massive Star Clusters: Supermassive Globular Clusters or Dwarf Galaxy Nuclei?
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=10260;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-lg40f0w
Author Harris, William Edgar
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=10260&mission=hst
Publication
  • 037-B327 in M31: Luminous Globular Cluster or Core of a Former Dwarf Spheroidal Companion to M31?
  • A Hubble Space Telescope Survey of the Disk Cluster Population of M31. II. Advanced Camera for Surveys Pointings
  • A near-ultraviolet view of the inner region of M 31 with the large binocular telescope
  • An HST/WFPC2 survey of bright young clusters in M 31. IV. Age and mass estimates
  • An updated survey of globular clusters in M 31. I. Classification and radial velocity for 76 candidate clusters
  • An updated survey of globular clusters in M 31. II. Newly discovered bright and remote clusters
  • A Population of Luminous Globular Clusters and Stripped Nuclei with Elevated Mass to Light Ratios around NGC 5128
  • A Transient Black Hole Low-Mass X-Ray Binary Candidate in Centaurus A
  • Cosmic-CoNN: A Cosmic-Ray Detection Deep-learning Framework, Data Set, and Toolkit
  • deepCR: Cosmic Ray Rejection with Deep Learning
  • Detailed study of B037 based on HST images
  • Globular Clusters and X-Ray Point Sources in Centaurus A (NGC 5128)
  • HST/ACS colour-magnitude diagrams of M 31 globular clusters
  • Low-Mass X-Ray Binaries and Globular Clusters in Centaurus A
  • On the Progenitors of Local Group Novae. I. The M31 Catalog
  • Optical Counterparts of the Nearest Ultraluminous X-Ray Sources
  • Probing cool giants in unresolved galaxies using fluctuation eigenspectra: A demonstration using high-resolution MUSE observations of NGC 5128
  • Sizes of Confirmed Globular Clusters in NGC 5128: A Wide-Field High-Resolution Study
  • Structural Parameters for Globular Clusters in M31 and Generalizations for the Fundamental Plane
  • Structural Parameters for Globular Clusters in NGC 5128. II. Hubble Space Telescope ACS Imaging and New Clusters
  • Structural parameters for globular clusters in NGC 5128 - III. ACS surface brightness profiles and model fits
  • Supernova Remnant Progenitor Masses in M31
  • The impact of satellite trails on Hubble Space Telescope observations
  • TRGB Distances to Galaxies Based on Hubble Space Telescope (HST) Images in One F814W Filter1
  • Triggered star formation in the inner filament of Centaurus A
Instrument ACS, ACS/WFC
Temporal Coverage 2004-07-04T21:02:54Z/2004-10-01T09:15:18Z
Version 1.0
Mission Description Launched in 1990, the NASA/ESA Hubble Space Telescope remains the premier UV and visible light telescope in orbit. With well over 1.6 million observations from 10 different scientific instruments, the ESA Hubble Science Archive is a treasure trove of astronomical data to be exploited.
Creator Contact https://support.cosmos.esa.int/esdc/index.php?/Tickets/Submit
Date Published 2005-10-01T15:44:16Z
Last Update 2025-01-25
Keywords Hubble, HST, HLA, HCV, ACS, COS, STIS, WFC3, FOC, FOS, HRS, NICMOS, WFPC, WFPC2
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Harris et al., 2005, 'The Most Massive Star Clusters: Supermassive Globular Clusters or Dwarf Galaxy Nuclei?', 1.0, European Space Agency, https://doi.org/10.5270/esa-lg40f0w