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

Aim. Our aim is to analyse the variance of the Inter-Galactic Medium transmission (IGM) by studying this parameter in the rest-frame UV spectra of a large sample of high redshift galaxies. Method. We make use of the VIMOS Ultra Deep Survey and the VANDELS public survey to have an insight into the far UV spectrum of $2.7

Keywords:

• Astrophysics
• Physics
• Galaxy

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