The HETDEX Survey: Probing Neutral Hydrogen in the Circumgalactic Medium of ∼88,000 Lyα Emitters

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 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 bac...

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Main Authors: Mahan Mirza Khanlari, Karl Gebhardt, Laurel H. Weiss, Dustin Davis, Erin Mentuch Cooper, Mahdi Qezlou, Maja Lujan Niemeyer, Robin Ciardullo, Donald P. Schneider, Shiro Mukae, Chenxu Liu, Daniel Farrow, Gary J. Hill, Gregory R. Zeimann, Wolfram Kollatschny
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
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Online Access:https://doi.org/10.3847/1538-4357/adf10e
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author Mahan Mirza Khanlari
Karl Gebhardt
Laurel H. Weiss
Dustin Davis
Erin Mentuch Cooper
Mahdi Qezlou
Maja Lujan Niemeyer
Robin Ciardullo
Donald P. Schneider
Shiro Mukae
Chenxu Liu
Daniel Farrow
Gary J. Hill
Gregory R. Zeimann
Wolfram Kollatschny
author_facet Mahan Mirza Khanlari
Karl Gebhardt
Laurel H. Weiss
Dustin Davis
Erin Mentuch Cooper
Mahdi Qezlou
Maja Lujan Niemeyer
Robin Ciardullo
Donald P. Schneider
Shiro Mukae
Chenxu Liu
Daniel Farrow
Gary J. Hill
Gregory R. Zeimann
Wolfram Kollatschny
author_sort Mahan Mirza Khanlari
collection DOAJ
description 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 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, in order to focus on the physics of the gas at large radii. The extensive number of fiber spectra contributing to the stacks ensures a sufficient signal-to-noise ratio 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.
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spelling doaj-art-a197963b1f9941c48c4120e6b597fea32025-08-22T15:16:39ZengIOP PublishingThe Astrophysical Journal1538-43572025-01-01989216910.3847/1538-4357/adf10eThe HETDEX Survey: Probing Neutral Hydrogen in the Circumgalactic Medium of ∼88,000 Lyα EmittersMahan Mirza Khanlari0https://orcid.org/0009-0003-1893-9526Karl Gebhardt1https://orcid.org/0000-0002-8433-8185Laurel H. Weiss2https://orcid.org/0000-0002-4974-1243Dustin Davis3https://orcid.org/0000-0002-8925-9769Erin Mentuch Cooper4https://orcid.org/0000-0002-2307-0146Mahdi Qezlou5https://orcid.org/0000-0001-7066-1240Maja Lujan Niemeyer6https://orcid.org/0000-0002-6907-8370Robin Ciardullo7https://orcid.org/0000-0002-1328-0211Donald P. Schneider8https://orcid.org/0000-0001-7240-7449Shiro Mukae9https://orcid.org/0000-0003-3823-8279Chenxu Liu10https://orcid.org/0000-0001-5561-2010Daniel Farrow11https://orcid.org/0000-0003-2575-0652Gary J. Hill12https://orcid.org/0000-0001-6717-7685Gregory R. Zeimann13https://orcid.org/0000-0003-2307-0629Wolfram Kollatschny14https://orcid.org/0000-0002-0417-1494Department of Astronomy, The University of Texas at Austin , 2515 Speedway Boulevard, Stop C1400, Austin, TX 78712, USADepartment of Astronomy, The University of Texas at Austin , 2515 Speedway Boulevard, Stop C1400, Austin, TX 78712, USADepartment of Astronomy, The University of Texas at Austin , 2515 Speedway Boulevard, Stop C1400, Austin, TX 78712, USADepartment of Astronomy, The University of Texas at Austin , 2515 Speedway Boulevard, Stop C1400, Austin, TX 78712, USADepartment of Astronomy, The University of Texas at Austin , 2515 Speedway Boulevard, Stop C1400, Austin, TX 78712, USA; McDonald Observatory, The University of Texas at Austin , 2515 Speedway Boulevard, Stop C1402, Austin, TX 78712, USADepartment of Astronomy, The University of Texas at Austin , 2515 Speedway Boulevard, Stop C1400, Austin, TX 78712, USAMax-Planck-Institut für Astrophysik , Karl-Schwarzschild-Str. 1, 85741 Garching, GermanyDepartment of Astronomy & Astrophysics, The Pennsylvania State University , University Park, PA 16802, USA; Institute for Gravitation and the Cosmos, The Pennsylvania State University , University Park, PA 16802, USADepartment of Astronomy & Astrophysics, The Pennsylvania State University , University Park, PA 16802, USA; Institute for Gravitation and the Cosmos, The Pennsylvania State University , University Park, PA 16802, USADepartment of Astronomy, The University of Texas at Austin , 2515 Speedway Boulevard, Stop C1400, Austin, TX 78712, USADepartment of Astronomy, The University of Texas at Austin , 2515 Speedway Boulevard, Stop C1400, Austin, TX 78712, USA; South-Western Institute for Astronomy Research, Yunnan University , Kunming, Yunnan, 650500, People’s Republic of ChinaCentre of Excellence for Data Science, Artificial Intelligence & Modeling (DAIM), University of Hull , Cottingham Road, Hull, HU6 7RX, UK; E. A. Milne Centre for Astrophysics University of Hull , Cottingham Road, Hull, HU6 7RX, UKDepartment of Astronomy, The University of Texas at Austin , 2515 Speedway Boulevard, Stop C1400, Austin, TX 78712, USA; McDonald Observatory, The University of Texas at Austin , 2515 Speedway Boulevard, Stop C1402, Austin, TX 78712, USAHobby Eberly Telescope, University of Texas , Austin, Austin, TX 78712, USAInstitut für Astrophysik and Geophysik, Universität Göttingen , Friedrich-Hund Platz 1, D-37077 Göttingen, GermanyWe 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 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, in order to focus on the physics of the gas at large radii. The extensive number of fiber spectra contributing to the stacks ensures a sufficient signal-to-noise ratio 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.https://doi.org/10.3847/1538-4357/adf10eCircumgalactic mediumGalaxy environmentsGalactic and extragalactic astronomyLarge-scale structure of the universeLyα galaxiesNeutral hydrogen clouds
spellingShingle Mahan Mirza Khanlari
Karl Gebhardt
Laurel H. Weiss
Dustin Davis
Erin Mentuch Cooper
Mahdi Qezlou
Maja Lujan Niemeyer
Robin Ciardullo
Donald P. Schneider
Shiro Mukae
Chenxu Liu
Daniel Farrow
Gary J. Hill
Gregory R. Zeimann
Wolfram Kollatschny
The HETDEX Survey: Probing Neutral Hydrogen in the Circumgalactic Medium of ∼88,000 Lyα Emitters
The Astrophysical Journal
Circumgalactic medium
Galaxy environments
Galactic and extragalactic astronomy
Large-scale structure of the universe
Lyα galaxies
Neutral hydrogen clouds
title The HETDEX Survey: Probing Neutral Hydrogen in the Circumgalactic Medium of ∼88,000 Lyα Emitters
title_full The HETDEX Survey: Probing Neutral Hydrogen in the Circumgalactic Medium of ∼88,000 Lyα Emitters
title_fullStr The HETDEX Survey: Probing Neutral Hydrogen in the Circumgalactic Medium of ∼88,000 Lyα Emitters
title_full_unstemmed The HETDEX Survey: Probing Neutral Hydrogen in the Circumgalactic Medium of ∼88,000 Lyα Emitters
title_short The HETDEX Survey: Probing Neutral Hydrogen in the Circumgalactic Medium of ∼88,000 Lyα Emitters
title_sort hetdex survey probing neutral hydrogen in the circumgalactic medium of ∼88 000 lyα emitters
topic Circumgalactic medium
Galaxy environments
Galactic and extragalactic astronomy
Large-scale structure of the universe
Lyα galaxies
Neutral hydrogen clouds
url https://doi.org/10.3847/1538-4357/adf10e
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