A dataset provided by the European Space Agency

Name 10531
Title The most distant X-ray cluster at z = 1.4: morphologies, color-magnitude relation and Fundamental Plane
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=10531;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-wogmflj
Author Mullis, Christopher
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=10531&mission=hst
Publication
  • Cluster galaxies in XMMU J2235-2557: galaxy population properties in most massive environments at z ~ 1.4
  • Dust-obscured star formation in the outskirts of XMMU J2235.3-2557, a massive galaxy cluster at z = 1.4
  • Morphological evolution in situ: disc-dominated cluster red sequences at z ~ 1.25
  • The impact of satellite trails on Hubble Space Telescope observations
Instrument ACS, ACS/WFC, NICMOS, NICMOS/NIC3, WFPC2, WFPC2/PC
Temporal Coverage 2005-08-09T04:17:05Z/2005-08-14T08:49:47Z
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.
Creator Contact https://support.cosmos.esa.int/esdc/index.php?/Tickets/Submit
Date Published 2006-08-14T16:14:37Z
Last Update 2025-01-25
Keywords Hubble, HST, HLA, HCV, ACS, COS, STIS, WFC3, FOC, FOS, HRS, NICMOS, WFPC, WFPC2
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Mullis et al., 2006, 'The most distant X-ray cluster at z = 1.4: morphologies, color-magnitude relation and Fundamental Plane', 1.0, European Space Agency, https://doi.org/10.5270/esa-wogmflj