The HETDEX Survey: Probing neutral hydrogen in the circumgalactic medium of ~88,000 Lyman Alpha Emitters

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Main Authors: Khanlari, Mahan Mirza, Gebhardt, Karl, Weiss, Laurel H., Davis, Dustin, Cooper, Erin Mentuch, Qezlou, Mahdi, Niemeyer, Maja Lujan, Ciardullo, Robin, Schneider, Donald P., Mukae, Shiro, Liu, Chenxu, Farrow, Daniel, Hill, Gary J., Zeimann, Gregory R., Kollatschny, Wolfram
Format: Preprint
Published: 2025
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author Khanlari, Mahan Mirza
Gebhardt, Karl
Weiss, Laurel H.
Davis, Dustin
Cooper, Erin Mentuch
Qezlou, Mahdi
Niemeyer, Maja Lujan
Ciardullo, Robin
Schneider, Donald P.
Mukae, Shiro
Liu, Chenxu
Farrow, Daniel
Hill, Gary J.
Zeimann, Gregory R.
Kollatschny, Wolfram
author_facet Khanlari, Mahan Mirza
Gebhardt, Karl
Weiss, Laurel H.
Davis, Dustin
Cooper, Erin Mentuch
Qezlou, Mahdi
Niemeyer, Maja Lujan
Ciardullo, Robin
Schneider, Donald P.
Mukae, Shiro
Liu, Chenxu
Farrow, Daniel
Hill, Gary J.
Zeimann, Gregory R.
Kollatschny, Wolfram
contents We explore the neutral hydrogen (H I) gas around 1.9 < z < 3.5 Lyman Alpha Emitters (LAEs) from the Hobby-Eberly Telescope Dark Energy Experiment (HETDEX) using faint Ly$α$ absorption. This absorption is the result of H I in the halo of the LAE scattering Ly$α$ photons from the integrated light of background galaxies along the line of sight. We stack millions of spectra from regions around ~88,000 LAEs to focus on the physics of the gas at large radii. The extensive number of fiber spectra contributing to the stacks ensures significant signal-to-noise ratio (S/N) to detect the faint Ly$α$ absorption which would otherwise be buried within the noise. We detect absorption out to a projected ~350 kpc around an average LAE at z~2.5. We use these results to create an empirical radial $W_λ$(Ly$α$) profile around LAEs. Comparison with numerical simulations reveals a profile similar to the empirical one within this region. Compared to previous studies, the profile is similar but modestly higher. We also outline a simple physical picture motivated by the observed trends in the data. We plan to quantify this radial profile as a function of redshift, local density, and Ly$α$ luminosity to explore the relationship between LAE environments and H I distribution.
format Preprint
id arxiv_https___arxiv_org_abs_2507_15942
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle The HETDEX Survey: Probing neutral hydrogen in the circumgalactic medium of ~88,000 Lyman Alpha Emitters
Khanlari, Mahan Mirza
Gebhardt, Karl
Weiss, Laurel H.
Davis, Dustin
Cooper, Erin Mentuch
Qezlou, Mahdi
Niemeyer, Maja Lujan
Ciardullo, Robin
Schneider, Donald P.
Mukae, Shiro
Liu, Chenxu
Farrow, Daniel
Hill, Gary J.
Zeimann, Gregory R.
Kollatschny, Wolfram
Astrophysics of Galaxies
We explore the neutral hydrogen (H I) gas around 1.9 < z < 3.5 Lyman Alpha Emitters (LAEs) from the Hobby-Eberly Telescope Dark Energy Experiment (HETDEX) using faint Ly$α$ absorption. This absorption is the result of H I in the halo of the LAE scattering Ly$α$ photons from the integrated light of background galaxies along the line of sight. We stack millions of spectra from regions around ~88,000 LAEs to focus on the physics of the gas at large radii. The extensive number of fiber spectra contributing to the stacks ensures significant signal-to-noise ratio (S/N) to detect the faint Ly$α$ absorption which would otherwise be buried within the noise. We detect absorption out to a projected ~350 kpc around an average LAE at z~2.5. We use these results to create an empirical radial $W_λ$(Ly$α$) profile around LAEs. Comparison with numerical simulations reveals a profile similar to the empirical one within this region. Compared to previous studies, the profile is similar but modestly higher. We also outline a simple physical picture motivated by the observed trends in the data. We plan to quantify this radial profile as a function of redshift, local density, and Ly$α$ luminosity to explore the relationship between LAE environments and H I distribution.
title The HETDEX Survey: Probing neutral hydrogen in the circumgalactic medium of ~88,000 Lyman Alpha Emitters
topic Astrophysics of Galaxies
url https://arxiv.org/abs/2507.15942