A Hubble Space Telescope Survey of the Disk Cluster Population of M31. I. WFPC2 Pointings
An HST/WFPC2 survey of bright young clusters in M 31. IV. Age and mass estimates
A Survey of Star Clusters in the M31 Southwest Field: UBVRI Photometry and Multiband Maps
Clues about the star formation history of the M31 disc from WFPC2 photometry
Constraints on Galaxy Formation from Stars in the Far Outer Disk of M31
Does the Oosterhoff Dichotomy Exist in the Andromeda Galaxy? I. The Case of G11
Hubble Space Telescope WFPC2 Color-Magnitude Diagrams for Globular Clusters in M31
Initial mass function in the South-Western part of M 31
M31 Globular Clusters in the Hubble Space Telescope Archive. I. Cluster Detection and Completeness
M31 Globular Clusters in the Hubble Space Telescope Archive. II. Structural Parameters
M31s Heavy-Element Distribution and Outer Disk
Photometry of Star Clusters in the M 31 Galaxy. Aperture Size Effects
RR Lyrae Variables in the Globular Clusters of M31: A First Detection of Likely Candidates
Supernova Remnant Progenitor Masses in M31
The Andromeda project. I. Deep HST-WFPC2 V, I photometry of 16 fields toward the disk and the halo of the M 31 galaxy. Probing the stellar content and metallicity distribution
The horizontal branch luminosity vs. metallicity in M 31 globular clusters
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
1999-01-10T07:19:13Z/2000-02-03T11:00:34Z
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, Rich comma R. Michael, 2001, 'Deep V, I Photometry for 20 M31 Globular Clusters', 1.0, European Space Agency, https://doi.org/10.5270/esa-gganf9j