2017ApJ...842L..22Z

We present the first results from the ongoing Lyman Alpha Galaxies in the Epoch of Reionization (LAGER) project, which is the largest narrowband survey for z ∼ 7 galaxies to date. Using a specially built narrowband filter NB964 for the superb large-area Dark Energy Camera (DECam) on the NOAO/CTIO 4 m Blanco telescope, LAGER has collected 34 hr NB964 narrowband imaging data in the 3 deg² COSMOS field. We have identified 23 Lyα Emitter candidates at z = 6.9 in the central 2-deg² region, where DECam and public COSMOS multi-band images exist. The resulting luminosity function (LF) can be described as a Schechter function modified by a significant excess at the bright end (four galaxies with L_Lyα ∼ 10^43.4±0.2 erg s^–1). The number density at L_Lyα ∼ 10^43.4±0.2 erg s^–1 is little changed from z = 6.6, while at fainter L_Lyα it is substantially reduced. Overall, we see a fourfold reduction in Lyα luminosity density from z = 5.7 to z = 6.9. Combined with a more modest evolution of the continuum UV luminosity density, this suggests a factor of ∼3 suppression of Lyα by radiative transfer through the z ∼ 7 intergalactic medium (IGM). It indicates an IGM neutral fraction of x_H i_ ∼ 0.4-0.6 (assuming Lyα velocity offsets of 100-200 km s^–1). The changing shape of the Lyα LF between z <= 6.6 and z = 6.9 supports the hypothesis of ionized bubbles in a patchy reionization at z ∼ 7.