A dataset provided by the European Space Agency

Name 15433
Title The first UV emission line spectrum of a strong low-z Lyman continuum leaker - a key to studying the sources of cosmic reionization
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=15433;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-f7q4g7e
Author Schaerer, Daniel
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=15433&mission=hst
Publication
  • Intense C III ll1907,1909 emission from a strong Lyman continuum emitting galaxy
Instrument STIS, STIS/CCD, STIS/NUV-MAMA
Temporal Coverage 2018-04-28T23:09:45Z/2019-01-02T23:10:20Z
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 2019-04-07T21:30:43Z
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, Schaerer comma Daniel, 2019, 'The first UV emission line spectrum of a strong low-z Lyman continuum leaker - a key to studying the sources of cosmic reionization', 1.0, European Space Agency, https://doi.org/10.5270/esa-f7q4g7e