Article (Scientific journals)
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
Drake, A. B.; Garel, T.; Wisotzki, L. et al.
2017In Astronomy and Astrophysics, 608, p. 6
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Keywords :
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)
Marino, R. A.
Pello, R.
Schaye, J.
Verhamme, A.
Ventou, E.
Weilbacher, P. M.
More authors (12 more) Less
Language :
English
Title :
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
Publication date :
November 2017
Journal title :
Astronomy and Astrophysics
ISSN :
0004-6361
eISSN :
1432-0746
Volume :
608
Pages :
A6
Peer reviewed :
Peer Reviewed verified by ORBi
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