A dataset provided by the European Space Agency

Name 14495
Title The gas-metallicity and the ISM of the brightest Lyman-alpha emitter at z=6.6: metal-free?
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=14495;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-46yde0p
Author Sobral, David
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=14495&mission=hst
Publication
  • ALMA Reveals Metals yet No Dust within Multiple Components in CR7
  • No evidence for Population III stars or a Direct Collapse Black Hole in the z = 6.6 Lyman-a emitter CR7
  • 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 2017-01-21T18:34:09Z/2017-03-17T18:43:22Z
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 2018-03-18T03:56:30Z
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, Sobral comma David, 2018, 'The gas-metallicity and the ISM of the brightest Lyman-alpha emitter at z=6.6: metal-free?', 1.0, European Space Agency, https://doi.org/10.5270/esa-46yde0p