LAGER Ly$\hat{I}\pm$ Luminosity Function at $z\sim 7$, Implications for Reionization

Abstract

We present a new measurement of the Ly$\hat{I}\pm$ luminosity function at redshift $z=6.9$, finding moderate evolution from $z=5.7$ that is consistent with a fully or largely ionized $z\sim 7$ 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 $6.1\times 10^6$ Mpc${}^3$ is double that of the next largest $z\sim 7$ 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$\hat{I}\pm$ emitters (LAEs); characterize our survey's completeness and reliability; and compute Ly$\hat{I}\pm$ luminosity functions. The best-fit Schechter luminosity function 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$\hat{I}\pm$ luminosity density declines at the same rate as the UV continuum LF from $z=5.7$ to $z=6.9$. This is consistent with an intergalactic medium that was fully ionized as early as redshift $z\sim 7$, or with a volume-averaged neutral hydrogen fraction of $x_{HI}<0.33$ at $1\ddot{I}ƒ$.

19 pages, 11 figures; accepted by ApJ