The Magellan M2FS Spectroscopic Survey of High-$z$ Galaxies: Lyα Emitters at $z\approx 6.6$ and the Evolution of Lyα Luminosity Function over $z\approx 5.7-6.6$

Abstract

We present a sample of Lyα emitters (LAEs) at $z\approx 6.6$ from our spectroscopic survey of high-redshift galaxies using the multi-object spectrograph M2FS on the Magellan Clay telescope. The sample consists of 36 LAEs selected by the narrow-band (NB921) technique over nearly 2 deg${}^2$ in the sky. These galaxies generally have high Lyα luminosities spanning a range of $\sim 3\times 10^{42}-7\times 10^{43}$ erg s${}^{-1}$, and include some of the most Lyα-luminous galaxies known at this redshift. They show a positive correlation between the Lyα line width and Lyα luminosity, similar to the relation previously found in $z\approx 5.7$ LAEs. Based on the spectroscopic sample, we calculate a sophisticated sample completeness correction and derive the Lyα luminosity function (LF) at $z\approx 6.6$. We detect a density bump at the bright end of the Lyα LF that is significantly above the best-fit Schechter function, suggesting that very luminous galaxies tend to reside in overdense regions that have formed large ionized bubbles around them. By comparing with the $z\approx 5.7$ Lyα LF, we confirm that there is a rapid LF evolution at the faint end, but a lack of evolution at the bright end. The fraction of the neutral hydrogen in the intergalactic medium at $z\approx 6.6$ estimated from such a rapid evolution is about $\sim 0.3\pm 0.1$, supporting a rapid and rather late process of cosmic reionization.

arXiv commentAccepted for publication in ApJ

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