A dataset provided by the European Space Agency

Name 10327
Title ACS Imaging of a High-Redshift Cluster of Galaxies
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=10327;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-0z0dg41
Author Ford, Holland
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=10327&mission=hst
Publication
  • A SINFONI view of flies in the Spiderweb: a galaxy cluster in the making
  • CO(1-0) survey of high-z radio galaxies: alignment of molecular halo gas with distant radio sources
  • COALAS. I. ATCA CO(1-0) survey and luminosity function in the Spiderweb protocluster at z = 2.16
  • COALAS II. Extended molecular gas reservoirs are common in a distant, forming galaxy cluster
  • CO Survey of High-z Radio Galaxies, Revisited with the Atacama Large Millimeter/submillimeter Array: Jet-Cloud Alignments and Synchrotron Brightening by Molecular Gas in the Circumgalactic Environment
  • Diffuse UV light associated with the Spiderweb Galaxy: evidence for in situ star formation outside galaxies
  • Disentangling star formation and AGN activity in powerful infrared luminous radio galaxies at 1 < z < 4
  • Giant galaxy growing from recycled gas: ALMA maps the circumgalactic molecular medium of the Spiderweb in C I
  • Internal Structure of Protocluster Galaxies: Accelerated Structural Evolution in Overdense Environments?
  • MAHALO Deep Cluster Survey II. Characterizing massive forming galaxies in the Spiderweb protocluster at z = 2.2
  • Massive starburst galaxies in a z = 2.16 proto-cluster unveiled by panoramic Ha mapping
  • Molecular gas in the halo fuels the growth of a massive cluster galaxy at high redshift
  • New insights into the role of AGNs in forming the cluster red sequence
  • Signs of environmental effects on star-forming galaxies in the Spiderweb protocluster at z = 2.16
  • The 700 ks Chandra Spiderweb Field. I. Evidence for widespread nuclear activity in the protocluster
  • The environmental dependence of galaxy properties at z = 2
  • The growth and assembly of a massive galaxy at z ~ 2
  • The impact of satellite trails on Hubble Space Telescope observations
  • The implications of the surprising existence of a large, massive CO disk in a distant protocluster
  • The Nascent Red Sequence at z ~ 2
  • The realm of the galaxy protoclusters. A review
  • The Spiderweb Galaxy: A Forming Massive Cluster Galaxy at z ~ 2
Instrument ACS, ACS/WFC, NICMOS, NICMOS/NIC3
Temporal Coverage 2005-05-17T10:57:38Z/2005-05-22T16:02:05Z
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 2006-05-23T00:17:19Z
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, Ford comma Holland, 2006, 'ACS Imaging of a High-Redshift Cluster of Galaxies', 1.0, European Space Agency, https://doi.org/10.5270/esa-0z0dg41