A Hubble Space Telescope Survey of the Disk Cluster Population of M31. II. Advanced Camera for Surveys Pointings
An ancient metal-poor population in M32, and halo satellite accretion in M31, identified by RR Lyrae stars
An updated survey of globular clusters in M 31. II. Newly discovered bright and remote clusters
Intermediate-Age Clusters in a Field Containing M31 and M32 Stars
The ancient stellar population of M 32: RR Lyrae variable stars confirmed
The Deepest Hubble Space Telescope Color-Magnitude Diagram of M32. Evidence for Intermediate-age Populations
The Extragalactic Distance Scale Without Cepheids. II. Surface Brightness Fluctuations
The Hubble Space Telescope Survey of M31 Satellite Galaxies. II. The Star Formation Histories of Ultrafaint Dwarf Galaxies
The Hubble Space Telescope Survey of M31 Satellite Galaxies. I. RR Lyrae-based Distances and Refined 3D Geometric Structure
The impact of satellite trails on Hubble Space Telescope observations
Variable Stars in (Not Only) Dwarf Galaxies: Key Tools to Constrain Distances and Stellar Content
Instrument
ACS, ACS/WFC, WFPC2, WFPC2/PC
Temporal Coverage
2004-11-24T07:04:16Z/2004-12-22T12:30:52Z
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.
