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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Dokumenter

  • aa38438-20

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  • 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

OriginalsprogEngelsk
ArtikelnummerA63
TidsskriftAstronomy & Astrophysics
Vol/bind650
Antal sider7
ISSN0004-6361
DOI
StatusUdgivet - 8 jun. 2021

ID: 273012105