A Search for RR Lyrae Variables in the Central Region of M54
Central dynamics of globular clusters
Comparing the properties of local globular cluster systems: implications for the formation of the Galactic halo
Hubble Space Telescope Reveals Multiple Sub-giant Branch in Eight Globular Clusters
OGLE Study of the Sagittarius Dwarf Spheroidal Galaxy and its M54 Globular Cluster
On the Accuracy of the Signal-to-Noise Estimates Obtained with the Exposure-Time Calculator of the Wide Field Planetary Camera 2 on Board the Hubble Space Telescope
Proper Motion of the Sagittarius Dwarf Galaxy Based on Hubble Space Telescope Imaging
Surface brightness profiles and structural parameters for globular clusters in the Fornax and Sagittarius dwarf spheroidal galaxies
Surface Brightness Profiles of Galactic Globular Clusters from Hubble Space Telescope Images
Testing Photometric Diagnostics for the Dynamical State and Possible Intermediate-mass Black Hole Presence in Globular Clusters
The ACS survey of Galactic globular clusters. XII. Photometric binaries along the main sequence
Using binaries in globular clusters to catch sight of intermediate-mass black holes
Instrument
WFPC2, WFPC2/PC, WFPC2/WFC
Temporal Coverage
1997-03-18T19:55:14Z/1999-08-30T23:13:03Z
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, Ibata comma Rodrigo, 2000, 'Photometry of the globular cluster system of the Sagittarius dwarf galaxy', 1.0, European Space Agency, https://doi.org/10.5270/esa-fn84b7b