LAGER Lyα Luminosity Function at z ∼ 7: Implications for Reionization
dc.contributor.author | Wold, Isak G. B. | |
dc.contributor.author | Malhotra, Sangeeta | |
dc.contributor.author | Rhoads, James | |
dc.contributor.author | Wang, Junxian | |
dc.contributor.author | Hu, Weida | |
dc.contributor.author | Perez, Lucia A. | |
dc.contributor.author | Zheng, Zhen-Ya | |
dc.contributor.author | Khostovan, Ali Ahmad | |
dc.contributor.author | Walker, Alistair R. | |
dc.contributor.author | Barrientos, L. Felipe | |
dc.contributor.author | González-López, Jorge | |
dc.contributor.author | Harish, Santosh | |
dc.contributor.author | Infante, Leopoldo | |
dc.contributor.author | Jiang, Chunyan | |
dc.contributor.author | Pharo, John | |
dc.contributor.author | Moya-Sierralta, Cristóbal | |
dc.contributor.author | Bauer, Franz E. | |
dc.contributor.author | Galaz, Gaspar | |
dc.contributor.author | Valdes, Francisco | |
dc.contributor.author | Yang, Huan | |
dc.date.accessioned | 2023-05-19T20:50:08Z | |
dc.date.available | 2023-05-19T20:50:08Z | |
dc.date.issued | 2022 | |
dc.description.abstract | We present a new measurement of the Ly alpha luminosity function (LF) at redshift z = 6.9, finding moderate evolution from z = 5.7 that is consistent with a fully or largely ionized z similar to 7 intergalactic medium. Our result is based on four fields of the LAGER (Lyman Alpha Galaxies in the Epoch of Reionization) project. Our survey volume of 6.1 x 10(6) Mpc(3) is double that of the next largest z similar to 7 survey. We combine two new LAGER fields (WIDE12 and GAMA15A) with two previously reported LAGER fields (COSMOS and CDFS). In the new fields, we identify N = 95 new z = 6.9 Ly alpha emitter (LAEs) candidates, characterize our survey's completeness and reliability, and compute Ly alpha LFs. The best-fit Schechter LF parameters for all four LAGER fields are in good general agreement. Two fields (COSMOS and WIDE12) show evidence for a bright-end excess above the Schechter function fit. We find that the Ly alpha luminosity density declines at the same rate as the UV continuum LF from z = 5.7 to 6.9. This is consistent with an intergalactic medium that was fully ionized as early as redshift z similar to 7 or with a volume-averaged neutral hydrogen fraction of x (H I) < 0.33 at 1 sigma. | |
dc.fechaingreso.objetodigital | 2024-10-17 | |
dc.fuente.origen | ORCID-mayo23 | |
dc.identifier.doi | 10.3847/1538-4357/ac4997 | |
dc.identifier.uri | https://repositorio.uc.cl/handle/11534/70168 | |
dc.identifier.wosid | WOS:000763683300001 | |
dc.issue.numero | No. 1 | |
dc.language.iso | en | |
dc.nota.acceso | contenido completo | |
dc.pagina.final | 15 | |
dc.pagina.inicio | 1 | |
dc.revista | Astrophysical Journal | |
dc.rights | acceso abierto | |
dc.title | LAGER Lyα Luminosity Function at z ∼ 7: Implications for Reionization | es_ES |
dc.type | artículo | |
dc.volumen | Vol. 927 | |
sipa.codpersvinculados | 1000955 | |
sipa.index | WOS |
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