Using Ly<i>α</i> Absorption to Measure the Intensity and Variability of <i>z</i> ∼ 2.4 Ultraviolet Background Light

Abstract We present measurements of z ∼ 2.4 ultraviolet (UV) background light using Ly α 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 Ly α 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 Ly α . Using this method, we determine an average intensity (in νJ ν 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.

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Publication Details

Journal
The Astrophysical Journal
Published
2025-04-08
DOI
https://doi.org/10.3847/1538-4357/adc0f9
Citations
2
Primary Topic
Photocathodes and Microchannel Plates
Type
article
Field-Weighted Citation Impact
1.35

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article

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

Mahdi Qezlou, Donald P. Schneider, Robin Ciardullo, Daniel J. Farrow et al.
2 citations
The Astrophysical Journal
Photocathodes and Microchannel Plates
1.35
article

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

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

Abstract

Abstract We present measurements of z ∼ 2.4 ultraviolet (UV) background light using Ly α 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 Ly α 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 Ly α . Using this method, we determine an average intensity (in νJ ν 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.

The Astrophysical JournalVol. 983(1)
Rutgers, The State University of New Jersey (US), Pennsylvania State University (US), University of Hull (GB), Max Planck Institute for Astrophysics (DE), The University of Texas at Austin (US)
National Science Foundation, Pennsylvania State University, University of Texas at Austin, Missouri University of Science and Technology, University of Oxford, Ministry of Education, Culture, Sports, Science and Technology, Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung, Georg-August-Universität Göttingen, University of Tokyo, Ludwig-Maximilians-Universität München, Leibniz-Institut für Astrophysik Potsdam, Max-Planck-Institut für Astrophysik, Department of Mechanical Engineering, University of Texas at Austin, U.S. Air Force, Leibniz-Gemeinschaft, Air Force Research Laboratory
Openalex Percentile: Top 21%
Photocathodes and Microchannel Plates
1.35
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