A dataset provided by the European Space Agency

Name 15941
Title UV emission line spectra of z~0.3-0.4 Lyman continuum emitters a key reference to uncover the sources of cosmic reionization
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=15941;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-9d0jki6
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=15941&mission=hst
Publication
  • Abundances of CNO elements in z 0.3-0.4 Lyman continuum leaking galaxies
  • Strong Lyman continuum emitting galaxies show intense C IV l1550 emission
Instrument STIS, STIS/CCD, STIS/NUV-MAMA
Temporal Coverage 2020-06-18T10:29:36Z/2022-06-28T21:05:31Z
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 2022-12-29T03:44:47Z
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 et al., 2022, 'UV emission line spectra of z~0.3-0.4 Lyman continuum emitters a key reference to uncover the sources of cosmic reionization', 1.0, European Space Agency, https://doi.org/10.5270/esa-9d0jki6