A Hubble Space Telescope Survey of the Disk Cluster Population of M31. I. WFPC2 Pointings
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
Initial mass function in the South-Western part of M 31
M31s Heavy-Element Distribution and Outer Disk
Photometry of Star Clusters in the M 31 Galaxy. Aperture Size Effects
The Opacity of Nearby Galaxies from Counts of Background Galaxies. II. Limits of the Synthetic Field Method
Instrument
NICMOS/NIC2, WFPC2, WFPC2/PC
Temporal Coverage
1997-08-14T08:25:36Z/1997-08-14T13:59:53Z
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, Trauger comma John, 1998, 'STELLAR POPULATIONS IN THE M31 DISK', 1.0, European Space Agency, https://doi.org/10.5270/esa-u4g7ylj