A dataset provided by the European Space Agency

Name 14497
Title Identifying z>12 galaxies with JWST: What sources produce strong UV emission lines?
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=14497;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-0hkktnc
Author European Space Agency
Description This is a scientific proposal for HST mission. For specific information please visit https:\\archive.stsci.edu\proposal_search.php?id=14497&mission=hst
Publication A gravitationally boosted MUSE survey for emission-line galaxies at z ≳ 5 behind the massive cluster RCS 0224, Smit, Renske,Swinbank, A. M.,Massey, Richard, Monthly Notices of the Royal Astronomical Society, 467, 2017-05-01 00:00:00, 2017MNRAS.467.3306S||Assessing the sources of reionization: a spectroscopic case study of a 30× lensed galaxy at z 5 with Lyα, C IV, Mg II, and [Ne III], Witstok, Joris,Smit, Renske,Maiolino, Roberto, Monthly Notices of the Royal Astronomical Society, 508, 2021-12-01 00:00:00, 2021MNRAS.508.1686W
Instrument ACS, ACS/WFC, WFC3/IR
Temporal Coverage 2016-11-11T14:49:12Z/2016-11-17T14:39:22Z
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 2017-11-17T16:53:46Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2017, Identifying Z>12 Galaxies With Jwst: What Sources Produce Strong Uv Emission Lines?, 1.0, European Space Agency, https://doi.org/10.5270/esa-0hkktnc