Analysis of a State Changing Supersoft X-Ray Source in M31
A Period Distribution of X-Ray Binaries Observed in the Central Region of M31 with Chandra and the Hubble Space Telescope
Discovery of a New Black Hole Transient within 100 (400 pc) of M31*
High-resolution mapping of dust via extinction in the M31 bulge
Mass-to-Light Ratios for M31 Globular Clusters: Age Dating and a Surprising Metallicity Trend
Observations of the recurrent M 31 transient XMMU J004215.8+411924 with Swift, Chandra, HST, and Einstein
On the Progenitors of Local Group Novae. II. The Red Giant Nova Rate of M31
On the Progenitors of Local Group Novae. I. The M31 Catalog
Optical Emission from Luminous and Very Soft X-Ray Sources in Nearby Galaxies: Testing the Scenario of Edge-on Supercritical Accretion Systems
Photometric evidence of an intermediate-age stellar population in the inner bulge of M31
The impact of satellite trails on Hubble Space Telescope observations
The Panchromatic Hubble Andromeda Treasury. VII. The Steep Mid-ultraviolet to Near-infrared Extinction Curve in the Central 200 pc of the M31 Bulge
Instrument
ACS, ACS/WFC, WFPC2, WFPC2/PC
Temporal Coverage
2006-02-10T03:58:08Z/2007-07-08T04:09:56Z
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.
