LAGER Lyα Luminosity Function at z ∼ 7: Implications for Reionization
Isak Wold, Sangeeta Malhotra, James E. Rhoads, Junxian Wang, Weida Hu, Lucia A. Perez, Zhen-Ya Zheng, Ali Ahmad Khostovan, A. R. Walker, L. Felipe Barrientos, Jorge González-López, Santosh Harish, L. Infante, Chunyan Jiang, John Pharo, C. Moya-Sierralta, F. E. Bauer, Gaspar Galaz, F. Valdés, Huan Yang
Abstract
Abstract We present a new measurement of the Ly α 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 ∼ 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 × 10 6 Mpc 3 is double that of the next largest z ∼ 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 α emitter (LAEs) candidates, characterize our survey’s completeness and reliability, and compute Ly α 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 α 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 ∼ 7 or with a volume-averaged neutral hydrogen fraction of x H I < 0.33 at 1 σ .