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Using Lyα Absorption to Measure the Intensity and Variability of z ∼ 2.4 Ultraviolet Background Light

Weiss, Laurel H.; Gebhardt, Karl; Davis, Dustin; Mentuch Cooper, Erin; Lujan Niemeyer, Maja; Qezlou, Mahdi; Mirza Khanlari, Mahan; Ciardullo, Robin; Farrow, Daniel; Gawiser, Eric; Gazagnes, Simon; Gronwall, Caryl; Hill, Gary J.; Schneider, Donald P.

Authors

Laurel H. Weiss

Karl Gebhardt

Dustin Davis

Erin Mentuch Cooper

Maja Lujan Niemeyer

Mahdi Qezlou

Mahan Mirza Khanlari

Robin Ciardullo

Eric Gawiser

Simon Gazagnes

Caryl Gronwall

Gary J. Hill

Donald P. Schneider



Abstract

We present measurements of z ∼ 2.4 ultraviolet (UV) background light using Lyα absorption from galaxies at z ∼ 2–3 in the Hobby–Eberly Telescope Dark Energy Experiment (HETDEX) database. Thanks to the wide area of this survey, we also measure the variability of this light across the sky. The data suggest an asymmetric geometry where integrated UV light from background galaxies is absorbed by H i within the halo of a foreground galaxy, in a configuration similar to damped Lyα systems. Using stacking analyses of over 400,000 HETDEX LAE spectra, we argue that this background absorption is detectable in our data. We also argue that the absorption signal becomes negative due to HETDEX's sky-subtraction procedure. The amount that the absorption is oversubtracted is representative of the z ∼ 2.4 UV contribution to the overall extragalactic background light (EBL) at Lyα. Using this method, we determine an average intensity (in νJν units) of 12.9 ± 3.7 nW m−2 sr−1 at a median observed wavelength of 4134 Å, or a rest-frame UV background intensity of 508 ± 145 nW m−2 sr−1 at z ∼ 2.4. We find that this flux varies significantly depending on the density of galaxies in the field of observation. Our estimates are consistent with direct measurements of the overall EBL.

Citation

Weiss, L. H., Gebhardt, K., Davis, D., Mentuch Cooper, E., Lujan Niemeyer, M., Qezlou, M., Mirza Khanlari, M., Ciardullo, R., Farrow, D., Gawiser, E., Gazagnes, S., Gronwall, C., Hill, G. J., & Schneider, D. P. (2025). Using Lyα Absorption to Measure the Intensity and Variability of z ∼ 2.4 Ultraviolet Background Light. The Astrophysical journal, 983(1), Article 72. https://doi.org/10.3847/1538-4357/adc0f9

Journal Article Type Article
Acceptance Date Mar 13, 2025
Online Publication Date Apr 8, 2025
Publication Date Apr 10, 2025
Deposit Date Apr 9, 2025
Publicly Available Date Apr 10, 2025
Journal The Astrophysical Journal
Print ISSN 0004-637X
Publisher American Astronomical Society
Peer Reviewed Peer Reviewed
Volume 983
Issue 1
Article Number 72
DOI https://doi.org/10.3847/1538-4357/adc0f9
Keywords Galaxies; Damped Lyα systems; Lyα galaxies; Diffuse radiation
Public URL https://hull-repository.worktribe.com/output/5127483
Additional Information Article Title: Using Lyα Absorption to Measure the Intensity and Variability of z ∼ 2.4 Ultraviolet Background Light; Journal Title: The Astrophysical Journal; Article Type: paper; Copyright Information: © 2025. The Author(s). Published by the American Astronomical Society.; Date Received: 2024-12-09; Date Accepted: 2025-03-13; Online publication date: 2025-04-08

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Copyright Statement
© 2025. The Author(s). Published by the American Astronomical Society.
Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.




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