The less and the 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:

• Public survey
• QSOS
• Optical depth
• Astrophysics
• Spectral line
• Galaxy
• Line-of-sight
• Redshift
• Physics
• Dispersion (optics)

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