A differential RR Lyrae line-of-sight distance between M31 and M33
An HST/WFPC2 survey of bright young clusters in M 31. IV. Age and mass estimates
An updated survey of globular clusters in M 31. I. Classification and radial velocity for 76 candidate clusters
An updated survey of globular clusters in M 31. II. Newly discovered bright and remote clusters
A Synoptic X-Ray Study of M31 with the Chandra High Resolution Camera
Chandra and HST Study of a New Transient X-Ray Source in M31
Discovery of an X-Ray Nova in M31
Optical Constraints on an X-ray Transient Source in M31
RR Lyrae variables in M31 and its satellites: an analysisof the galaxys population
The impact of satellite trails on Hubble Space Telescope observations
Variable Star Candidates in an Advanced Camera for Surveys Field of M31
Instrument
ACS, ACS/HRC, ACS/WFC, WFPC2, WFPC2/PC
Temporal Coverage
2001-07-07T06:14:14Z/2002-12-01T16:25:31Z
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, Garcia comma Michael R., 2003, 'Black Hole X-ray Transients and X-ray Binaries in M31', 1.0, European Space Agency, https://doi.org/10.5270/esa-1n15954