A dataset provided by the European Space Agency

Name 14596
Title Is Lyman Alpha Emitter CR7 Powered by a Direct Collapse Black Hole?
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=14596;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-feuaqni
Author Fan, Xiaohui
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=14596&mission=hst
Publication
  • On the nature and physical conditions of the luminous Ly a emitter CR7 and its rest-frame UV components
  • The nature of CR7 revealed with MUSE: a young starburst powering extended Ly a emission at z = 6.6
  • The Roles of Morphology and Environment on the Star Formation Rate-Stellar Mass Relation in COSMOS from 0 < z < 3.5
Instrument WFC3/IR
Temporal Coverage 2017-03-14T08:53:18Z/2017-11-21T19:59:39Z
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 2018-11-22T05:03:11Z
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, Fan comma Xiaohui, 2018, 'Is Lyman Alpha Emitter CR7 Powered by a Direct Collapse Black Hole?', 1.0, European Space Agency, https://doi.org/10.5270/esa-feuaqni