A SLUGGS and Gemini/GMOS combined study of the elliptical galaxy M60: wide-field photometry and kinematics of the globular cluster system
A Variable Ultraluminous X-Ray Source in a Globular Cluster in NGC 4649
Deep Chandra Monitoring Observations of NGC 4649. I. Catalog of Source Properties
Deep Chandra Monitoring Observations of NGC 4649. II. Wide-field Hubble Space Telescope Imaging of the Globular Clusters
Spatial Structures in the Globular Cluster Distribution of the 10 Brightest Virgo Galaxies
The impact of satellite trails on Hubble Space Telescope observations
The Radial Distribution of X-Ray Binaries and Globular Clusters in NGC 4649 and their Relation with the Local Stellar Mass Density
The Two-dimensional Spatial Distributions of the Globular Clusters and Low-mass X-Ray Binaries of NGC 4649
Instrument
ACS, ACS/WFC, WFC3, WFC3/IR
Temporal Coverage
2011-05-17T02:57:21Z/2011-05-17T10:06:49Z
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, Fabbiano et al., 2012, 'Constraining the Transient Black Hole {Bh} Low-Mass X-Ray Binary {Lmxb} Population', 1.0, European Space Agency, https://doi.org/10.5270/esa-tpec22u