Principal Component Analysis of the Time- and Position-dependent Point-Spread Function of the Advanced Camera for Surveys
Probing high-redshift clusters with HST/ACS gravitational weak-lensing and Chandra x-ray observations
RR Lyrae Variables in M33. I. Evidence for a Field Halo Population
The ACS Virgo Cluster Survey. VIII. The Nuclei of Early-Type Galaxies
The ACS Virgo Cluster Survey. XIII. SBF Distance Catalog and the Three-dimensional Structure of the Virgo Cluster
The impact of satellite trails on Hubble Space Telescope observations
Weak-Lensing Analysis of the z~=0.8 Cluster CL 0152-1357 with the Advanced Camera for Surveys
Instrument
ACS, ACS/HRC, ACS/WFC
Temporal Coverage
2002-09-13T14:51:56Z/2003-09-06T02:43:25Z
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, De Marchi comma Guido, 2003, 'Stability of the ACS CCD: geometry, flat fielding, photometry', 1.0, European Space Agency, https://doi.org/10.5270/esa-frqla57