Absorption Troughs of Lyα Emitters in HETDEX
Schneider, Donald P.; Chisholm, John; Kollatschny, Wolfram; Gebhardt, Karl; Gronwall, Caryl; Ciardullo, Robin; Mentuch Cooper, Erin; Davis, Dustin; Bowman, William P.; Zeimann, Gregory R.; Weiss, Laurel H.; Hill, Gary J.; Jeong, Donghui; Saito, Shun; Fabricius, Maximilian; Farrow, Daniel; Byrohl, Chris; Berg, Danielle; Komatsu, Eiichiro; Gazagnes, Simon; Lujan Niemeyer, Maja; Mirza Khanlari, Mahan; House, Lindsay R.; Khoraminezhad, Hasti
United States, Germany, United Kingdom, Japan
Abstract
The Hobby–Eberly Telescope Dark Energy Experiment (HETDEX) is designed to detect and measure the redshifts of more than 1 million Lyα emitting galaxies (LAEs) 1.88 < z < 3.52. In addition to its cosmological measurements, these data enable studies of Lyα spectral profiles and the underlying radiative transfer. Using the roughly half a million LAEs in the HETDEX Data Release 3, we stack various subsets to obtain the typical Lyα profile for the z ∼ 2–3 epoch and to understand their physical properties. We find clear absorption wings around Lyα emission, which extend ∼2000 km s‑1 both redward and blueward of the central line. Using far-UV spectra of nearby (0.002 < z < 0.182) LAEs in the COS Legacy Archive Spectroscopic Survey treasury and optical/near-IR spectra of 2.8 < z < 6.7 LAEs in the Multi Unit Spectroscopic-Wide survey, we observe absorption profiles in both redshift regimes. Dividing the sample by volume density shows that the troughs increase in higher-density regions. This trend suggests that the depth of the absorption is dependent on the local density of objects near the LAE, a geometry that is similar to damped Lyα systems. Simple simulations of Lyα radiative transfer can produce similar troughs due to absorption of light from background sources by H I gas surrounding the LAEs.