Evolution of the observed Ly α luminosity function from z = 6.5 to z = 7.7: Evidence for the epoch of reionization?
| dc.contributor.author | Clément, B. | en |
| dc.contributor.author | Cuby, J. G. | en |
| dc.contributor.author | Courbin, F. | en |
| dc.contributor.author | Fontana, A. | en |
| dc.contributor.author | Freudling, W. | en |
| dc.contributor.author | Fynbo, J. | en |
| dc.contributor.author | Gallego, J. | en |
| dc.contributor.author | Hibon, P. | en |
| dc.contributor.author | Kneib, J. P. | en |
| dc.contributor.author | Le Fèvre, O. | en |
| dc.contributor.author | Lidman, C. | en |
| dc.contributor.author | McMahon, R. | en |
| dc.contributor.author | Milvang-Jensen, B. | en |
| dc.contributor.author | Moller, P. | en |
| dc.contributor.author | Moorwood, A. | en |
| dc.contributor.author | Nilsson, K. K. | en |
| dc.contributor.author | Pentericci, L. | en |
| dc.contributor.author | Venemans, B. | en |
| dc.contributor.author | Villar, V. | en |
| dc.contributor.author | Willis, J. | en |
| dc.date.accessioned | 2026-01-01T13:41:22Z | |
| dc.date.available | 2026-01-01T13:41:22Z | |
| dc.date.issued | 2012 | en |
| dc.description.abstract | Aims. Lyα emitters (LAEs) can be detected out to very high redshifts during the epoch of reionization. The evolution of the LAE luminosity function with redshift is a direct probe of the Lyα transmission of the intergalactic medium (IGM), and therefore of the IGM neutral-hydrogen fraction. Measuring the Lyα luminosity function (LF) of Lyα emitters at redshift z = 7.7 therefore allows us to constrain the ionizing state of the Universe at this redshift. Methods. We observed three 7′.5 × 7′.5 fields with the HAWK-I instrument at the VLT with a narrow band filter centred at 1.06 μm and targeting Lyα emitters at redshift z ∼ 7.7. The fields were chosen for the availability of multiwavelength data. One field is a galaxy cluster, the Bullet Cluster, which allowed us to use gravitational amplification to probe luminosities that are fainter than in the field. The two other fields are subareas of the GOODS Chandra Deep Field South and CFHTLS-D4 deep field. We selected z = 7.7 LAE candidates from a variety of colour criteria, in particular from the absence of detection in the optical bands. Results. We do not find any LAE candidates at z = 7.7 in ∼2.4 × 10 4 Mpc 3 down to a narrow band AB magnitude of ∼26, which allows us to infer robust constraints on the Lyα LAE luminosity function at this redshift. Conclusions. The predicted mean number of objects at z = 6.5, derived from somewhat different luminosity functions of Hu et al. (2010, ApJ, 725, 394), Ouchi et al. (2010, ApJ, 723, 869), and Kashikawa et al. (2011, ApJ, 734, 119) are 2.5, 13.7, and 11.6, respectively. Depending on which of these luminosity functions we refer to, we exclude a scenario with no evolution from z = 6.5 to z = 7.7 at 85% confidence without requiring a strong change in the IGM Lyα transmission, or at 99% confidence with a significant quenching of the IGM Lyα transmission, possibly from a strong increase in the high neutral-hydrogen fraction between these two redshifts. | en |
| dc.description.sponsorship | We acknowledge financial support from Agence Nationale de la Recherche (grant ANR-09-BLAN-0234-01). F.C. is supported by the Swiss National Science Foundation (SNSF). The Dark Cosmology Centre is funded by the Danish National Research Foundation. | en |
| dc.description.status | Peer-reviewed | en |
| dc.identifier.issn | 0004-6361 | en |
| dc.identifier.scopus | 84856754670 | en |
| dc.identifier.uri | https://hdl.handle.net/1885/733800674 | |
| dc.language.iso | en | en |
| dc.source | Astronomy and Astrophysics | en |
| dc.subject | dark ages, reionization, first stars | en |
| dc.subject | early Universe | en |
| dc.subject | galaxies: high-redshift | en |
| dc.subject | galaxies: luminosity function, mass function | en |
| dc.subject | methods: observational | en |
| dc.subject | techniques: image processing | en |
| dc.title | Evolution of the observed Ly α luminosity function from z = 6.5 to z = 7.7: Evidence for the epoch of reionization? | en |
| dc.type | Journal article | en |
| dspace.entity.type | Publication | en |
| local.contributor.affiliation | Clément, B.; Aix Marseille Université | en |
| local.contributor.affiliation | Cuby, J. G.; Aix Marseille Université | en |
| local.contributor.affiliation | Courbin, F.; Swiss Federal Institute of Technology Lausanne | en |
| local.contributor.affiliation | Fontana, A.; Osservatorio Astronomico Roma | en |
| local.contributor.affiliation | Freudling, W.; European Southern Observatory | en |
| local.contributor.affiliation | Fynbo, J.; University of Copenhagen | en |
| local.contributor.affiliation | Gallego, J.; Complutense University | en |
| local.contributor.affiliation | Hibon, P.; Arizona State University | en |
| local.contributor.affiliation | Kneib, J. P.; Aix Marseille Université | en |
| local.contributor.affiliation | Le Fèvre, O.; Aix Marseille Université | en |
| local.contributor.affiliation | Lidman, C.; Australian Astronomical Observatory | en |
| local.contributor.affiliation | McMahon, R.; University of Cambridge | en |
| local.contributor.affiliation | Milvang-Jensen, B.; University of Copenhagen | en |
| local.contributor.affiliation | Moller, P.; European Southern Observatory | en |
| local.contributor.affiliation | Moorwood, A.; European Southern Observatory | en |
| local.contributor.affiliation | Nilsson, K. K.; European Southern Observatory | en |
| local.contributor.affiliation | Pentericci, L.; Osservatorio Astronomico Roma | en |
| local.contributor.affiliation | Venemans, B.; European Southern Observatory | en |
| local.contributor.affiliation | Villar, V.; Complutense University | en |
| local.contributor.affiliation | Willis, J.; University of Victoria BC | en |
| local.identifier.citationvolume | 538 | en |
| local.identifier.doi | 10.1051/0004-6361/201117312 | en |
| local.identifier.pure | 04ed4686-6998-47f5-886d-1cf3ee5a622e | en |
| local.identifier.url | https://www.scopus.com/pages/publications/84856754670 | en |
| local.type.status | Published | en |