PREPRINT
3A4EE62E-C1FC-47F6-B03E-606E79185719

The Evolution of Lyman Alpha Emitter Line Widths from z=5.7 to z=6.6

A. Songaila, A. J. Barger, L. L. Cowie, E. M. Hu, A. J. Taylor
arXiv:2207.05758

Submitted on 12 July 2022

Abstract

Recent evidence suggests that high-redshift Ly-alpha emitting galaxies (LAEs) with logL(Ly-alpha) > 43.5 erg/s, referred to as ultraluminous LAEs (ULLAEs), may show less evolution than lower-luminosity LAEs in the redshift range z=5.7-6.6. Here we explore the redshift evolution of the velocity widths of the Ly-alpha emission lines in LAEs over this redshift interval. We use new wide-field, narrowband observations from Subaru/Hyper Suprime-Cam to provide a sample of 24 z=6.6 and 12 z=5.7 LAEs with log L(Ly-alpha) > 43 erg/s, all of which have follow-up spectroscopy from Keck/DEIMOS. Combining with archival lower-luminosity data, we find a significant narrowing of the Ly-alpha lines in LAEs at logL(Ly-alpha) < 43.25 erg/s -- somewhat lower than the usual ULLAE definition -- at z = 6.6 relative to those at z = 5.7, but we do not see this in higher-luminosity LAEs. As we move to higher redshifts, the increasing neutrality of the intergalactic medium should increase the scattering of the Ly-alpha lines, making them narrower. The absence of this effect in the higher-luminosity LAEs suggests they may lie in more highly ionized regions, self-shielding from the scattering effects of the intergalactic medium.

Preprint

Comment: 11 pages, 8 figures, 3 tables, accepted for publication in ApJ

Subject: Astrophysics - Astrophysics of Galaxies

URL: https://arxiv.org/abs/2207.05758