A dataset provided by the European Space Agency

Name 15266
Title Imaging the Most Massive Galaxy Overdensities at z=2.2: The Morphology-Density Relation at High Redshift
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=15266;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-ebx7zsg
Author Cai, Zheng
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=15266&mission=hst
Publication
  • What boost galaxy mergers in two massive galaxy protoclusters at z = 2.24?
Instrument WFC3/IR
Temporal Coverage 2018-02-05T18:54:26Z/2019-03-27T09:09:22Z
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 2019-09-27T13:28:00Z
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, Cai comma Zheng, 2019, 'Imaging the Most Massive Galaxy Overdensities at z=2.2: The Morphology-Density Relation at High Redshift', 1.0, European Space Agency, https://doi.org/10.5270/esa-ebx7zsg