Deep luminosity functions and colour-magnitude relations for cluster galaxies at 0.2 < z < 0.6
Internal kinematics of spiral galaxies in distant clusters. III. Velocity fields from FORS2/MXU spectroscopy
Kinematic and Structural Evolution of Field and Cluster Spiral Galaxies
RELICS: Reionization Lensing Cluster Survey
Strong-lensing analysis of a complete sample of 12 MACS clusters at z > 0.5: mass models and Einstein radii
The impact of satellite trails on Hubble Space Telescope observations
The ultraviolet continuum slopes of high-redshift galaxies: evidence for the emergence of dust-free stellar populations at z > 10
X-ray bright active galactic nuclei in massive galaxy clusters - III. New insights into the triggering mechanisms of cluster AGN
Instrument
ACS, ACS/WFC
Temporal Coverage
2005-10-31T19:11:52Z/2006-06-07T05:49:08Z
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, Ziegler comma Bodo, 2007, 'Galaxy Transformation as probed by Morphology and Velocity Fields of Distant Cluster Galaxies', 1.0, European Space Agency, https://doi.org/10.5270/esa-t4ciejl