The MUSE Hubble Ultra Deep Field Survey. VI. The faint-end of the Ly{\ensuremath{\alpha}} luminosity function at 2.91 < z < 6.64 and implications for reionisation
galaxies: luminosity function; mass function; galaxies: evolution; early Universe; dark ages; reionization; first stars; galaxies: formation; Astrophysics - Cosmology and Nongalactic Astrophysics
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Drake, A. B.
Garel, T.
Wisotzki, L.
Leclercq, F.
Hashimoto, T.
Richard, J.
Bacon, R.
Blaizot, J.
Caruana, J.
Conseil, S.
Contini, T.
Guiderdoni, B.
Herenz, E. C.
Inami, H.
Lewis, J.
Mahler, Guillaume ; Université de Liège - ULiège > Département d'astrophysique, géophysique et océanographie (AGO) > Multi-wavelength Extragalactic and Galactic Astrophysics (MEGA)
The MUSE Hubble Ultra Deep Field Survey. VI. The faint-end of the Ly{\ensuremath{\alpha}} luminosity function at 2.91 < z < 6.64 and implications for reionisation