Less and more IGM-transmitted galaxies from z similar to 2.7 to z similar to 6 from VANDELS and VUDS

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  • aa38438-20

    Final published version, 4.23 MB, PDF document

  • R. Thomas
  • L. Pentericci
  • O. Le Fevre
  • A. M. Koekemoer
  • M. Castellano
  • A. Cimatti
  • F. Fontanot
  • A. Gargiulo
  • B. Garilli
  • M. Talia
  • R. Amorin
  • S. Bardelli
  • S. Cristiani
  • G. Cresci
  • M. Franco
  • N. P. Hathi
  • P. Hibon
  • Y. Khusanova
  • Matthieu Le Brun
  • B. C. Lemaux
  • F. Mannucci
  • D. Schaerer
  • G. Zamorani
  • E. Zucca

Aims. Our aim is to analyze the variance of the intergalactic medium (IGM) transmission by studying this parameter in the rest-frame UV spectra of a large sample of high-redshift galaxies.Methods. We made use of the VIMOS Ultra Deep Survey and the VANDELS public survey to gain insight into the far UV spectrum of 2.7

Original languageEnglish
Article numberA63
JournalAstronomy & Astrophysics
Volume650
Number of pages7
ISSN0004-6361
DOIs
Publication statusPublished - 8 Jun 2021

    Research areas

  • intergalactic medium, galaxies: high-redshift, cosmology: miscellaneous, INTERGALACTIC MEDIUM TRANSMISSION, DATA-REDUCTION, EVOLUTION, REDSHIFTS, STELLAR

ID: 273012105