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A MUSE View of the HDFS: The Lyα Luminosity Function out to z~6

Published online by Cambridge University Press:  17 August 2016

Alyssa B. Drake
Affiliation:
Centre de Recherche Astrophysique de Lyon, Université Lyon 1, Lyon, France email: alyssa-bryony.drake@univ-lyon1.fr
Bruno Guiderdoni
Affiliation:
Centre de Recherche Astrophysique de Lyon, Université Lyon 1, Lyon, France email: alyssa-bryony.drake@univ-lyon1.fr
Jérémy Blaizot
Affiliation:
Centre de Recherche Astrophysique de Lyon, Université Lyon 1, Lyon, France email: alyssa-bryony.drake@univ-lyon1.fr
Johan Richard
Affiliation:
Centre de Recherche Astrophysique de Lyon, Université Lyon 1, Lyon, France email: alyssa-bryony.drake@univ-lyon1.fr
Roland Bacon
Affiliation:
Centre de Recherche Astrophysique de Lyon, Université Lyon 1, Lyon, France email: alyssa-bryony.drake@univ-lyon1.fr
Thibault Garel
Affiliation:
Centre de Recherche Astrophysique de Lyon, Université Lyon 1, Lyon, France email: alyssa-bryony.drake@univ-lyon1.fr
Takuya Hashimoto
Affiliation:
Centre de Recherche Astrophysique de Lyon, Université Lyon 1, Lyon, France email: alyssa-bryony.drake@univ-lyon1.fr
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Abstract

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We present preliminary results from MUSE on the Lyα luminosity function in the Hubble Deep Field South (HDFS). Using a large homogeneous sample of LAEs selected through blind spectroscopy, we utilise the unprecedented detection power of MUSE to study the progenitors of L* galaxies back to when the Universe was just ~2 Gyr old. We present these results in the context of the current literature, and highlight the importance of the forthcoming Hubble Ultra Deep Field (HUDF) study with MUSE, which will increase the size of our sample by a factor of ~ 10.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2016 

References

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