A high occurrence of nuclear star clusters in faint Coma galaxies, and the roles of mass and environment
A Novel Approach to Constrain the Mass Ratio of Minor Mergers in Elliptical Galaxies: Application to NGC 4889, the Brightest Cluster Galaxy in Coma
A Photometric Survey of Globular Cluster Systems in Brightest Cluster Galaxies
A precise benchmark for cluster scaling relations: Fundamental Plane, Mass Plane, and IMF in the Coma cluster from dynamical models
A Wide-field Map of Intracluster Globular Clusters in Coma
Globular Cluster Systems in Brightest Cluster Galaxies. III: Beyond Bimodality
Infrared Surface Brightness Fluctuation Distances for MASSIVE and Type Ia Supernova Host Galaxies
Spectroscopic Constraints on the Buildup of Intracluster Light in the Coma Cluster
The Globular Cluster System of the Coma cD Galaxy NGC 4874 from Hubble Space Telescope ACS and WFC3/IR Imaging
The Hubble Constant from Infrared Surface Brightness Fluctuation Distances
The impact of satellite trails on Hubble Space Telescope observations
The X-ray coronae of the two brightest galaxies in the Coma cluster
Ultradiffuse Galaxies--A Distinct Population? Dwarf Galaxies in the Coma Cluster and A262 from Deep u-g-r Wendelstein Imaging Data
Instrument
ACS, ACS/WFC, WFC3, WFC3/IR, WFC3/UVIS
Temporal Coverage
2010-02-26T10:43:20Z/2010-03-01T18:50:01Z
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.
European Space Agency, Blakeslee et al., 2011, 'A Definitive Distance to the Coma Core Ellipticals', 1.0, European Space Agency, https://doi.org/10.5270/esa-7g7t8f8
