2025/06/16 by Anthony J. Taylor, A. J. Barger, Taylor, A. J. +7
Earth and Planetary Sciences · Physics and Astronomy · #Astrophysics of Galaxies (astro-ph.GA) #Atmospheric Ozone and Climate #Atomic and Subatomic Physics Research #FOS: Physical sciences #Ionosphere and magnetosphere dynamics
paper · pdf · doi:10.48550/arxiv.2506.13854
openalex publication_date 2025/06/16 · openalex created_date 2025/10/18 · openalex updated_date 2026/07/28
We present spectroscopic Lyα luminosity functions (LFs) at z = 5.7 and z = 6.6 based on a large 209 source sample of Lyα emitter (LAE) candidates identified in Subaru/Hyper Suprime-Cam narrowband imaging and confirmed with Keck II/DEIMOS spectroscopy over a multi-year observing campaign. After applying photometric and spectroscopic cuts to produce homogeneous samples, we use the resulting samples of 49 z = 5.7 and 56 z = 6.6 LAEs to compute spectroscopic LAE LFs at each redshift. We correct our LFs for incompleteness using a source-injection simulation. We find excellent agreement with current spectroscopic and photometric LAE LFs from the literature. We look for evolution over the redshift range z = 5.7-6.6. We find a strong convergence of the LFs at L(Lyα) > 1043.4 erg s-1. This convergence (noted in previous literature) provides strong evidence that the most luminous LAEs at z = 6.6 form ionized bubbles around themselves, allowing for greater Lyα transmission through the neutral intergalactic medium, which is measured as an increase in the bright end of the z = 6.6 LF over the expected evolution in the LF based on the faint end. We infer that ultraluminous LAEs may play a significant role in reionization.