Joint Analysis of Cluster Observations. I. Mass Profile of Abell 478 from Combined X-Ray, Sunyaev-Zeldovich, and Weak-Lensing Data
LoCuSS: connecting the dominance and shape of brightest cluster galaxies with the assembly history of massive clusters
LoCuSS: first results from strong-lensing analysis of 20 massive galaxy clusters at z = 0.2
Measuring the matter distribution within z = 0.2 cluster lenses with XMM-Newton
Molecular accretion in the core of the galaxy cluster 2A 0335+096
Molecular Gas Along a Bright Ha Filament in 2A 0335+096 Revealed by ALMA
Offset between dark matter and ordinary matter: evidence from a sample of 38 lensing clusters of galaxies
On the distribution of dark matter in clusters of galaxies
On the frequency of star-forming galaxies in the vicinity of powerful AGNs: The case of SMM J04135+10277
Riding the wake of a merging galaxy cluster
Star Formation, Radio Sources, Cooling X-Ray Gas, and Galaxy Interactions in the Brightest Cluster Galaxy in 2A0335+096
The peculiar cooling flow cluster RX J0820.9+0752
X-ray-optical classification of cluster mergers and the evolution of the cluster merger fraction
Instrument
WFPC2, WFPC2/PC, WFPC2/WFC
Temporal Coverage
1999-08-18T08:10:13Z/2000-06-28T23:53:54Z
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, Edge comma Alastair C., 2000, 'A SNAPSHOT SURVEY OF X-RAY SELECTED CENTRAL CLUSTER GALAXIES', 1.0, European Space Agency, https://doi.org/10.5270/esa-bn5kzw2