Systematic Bias in Ionizing Radiation Escape Fraction Measurements from Foreground Large-scale Structures

Abstract We investigate the relationship between the Ly α forest transmission in the intergalactic medium (IGM) and the environmental density of galaxies, focusing on its implications for the measurement of ionizing radiation escape fractions. Using a sample of 268 spectroscopically confirmed background galaxies at 2.7 < z < 3.0 and a galaxy density map at z ≈ 2.5 within the COSMOS field, we measure the Ly α transmission photometrically, leveraging the multiwavelength data available from the COSMOS2020 catalog. Our results reveal a weak but statistically significant positive correlation between Ly α optical depth and galaxy density contrast, suggesting that overdense regions are enriched in neutral gas, which could bias escape fraction measurements. This emphasizes the need to account for the large-scale structure of the IGM in analyses of ionizing radiation escape fractions and highlights the advantages of a photometric approach for increasing the number of sampled lines of sight across large fields. The photometric redshifts provided by upcoming all-sky surveys, such as Euclid, will make it possible to account for this bias, which can also be minimized by using fields separated in the sky by many degrees.

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Publication Details

Journal
The Astrophysical Journal
Published
2025-05-19
DOI
https://doi.org/10.3847/1538-4357/adcf9a
Citations
2
Primary Topic
Radiation Detection and Scintillator Technologies
Type
article
Field-Weighted Citation Impact
3.77
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article

Systematic Bias in Ionizing Radiation Escape Fraction Measurements from Foreground Large-scale Structures

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The Astrophysical Journal
Radiation Detection and Scintillator Technologies
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article

Systematic Bias in Ionizing Radiation Escape Fraction Measurements from Foreground Large-scale Structures

Matthew Hayes, Ali Ahmad Khostovan, Marc Rafelski, Sina Taamoli, Yu-Heng Lin, M. Salvato, Caitlin M. Casey, Weida Hu, Claudia Scarlata, Jeyhan S. Kartaltepe, Andreas L. Faisst
article en
2 citations

Abstract

Abstract We investigate the relationship between the Ly α forest transmission in the intergalactic medium (IGM) and the environmental density of galaxies, focusing on its implications for the measurement of ionizing radiation escape fractions. Using a sample of 268 spectroscopically confirmed background galaxies at 2.7 < z < 3.0 and a galaxy density map at z ≈ 2.5 within the COSMOS field, we measure the Ly α transmission photometrically, leveraging the multiwavelength data available from the COSMOS2020 catalog. Our results reveal a weak but statistically significant positive correlation between Ly α optical depth and galaxy density contrast, suggesting that overdense regions are enriched in neutral gas, which could bias escape fraction measurements. This emphasizes the need to account for the large-scale structure of the IGM in analyses of ionizing radiation escape fractions and highlights the advantages of a photometric approach for increasing the number of sampled lines of sight across large fields. The photometric redshifts provided by upcoming all-sky surveys, such as Euclid, will make it possible to account for this bias, which can also be minimized by using fields separated in the sky by many degrees.

The Astrophysical JournalVol. 985(1)
University of California, Riverside (US), California Institute of Technology (US), Space Telescope Science Institute (US), University of Minnesota (US), University of Kentucky (US), Johns Hopkins University (US), University of California, Santa Barbara (US), Rochester Institute of Technology (US), Stockholm University (SE), Max Planck Institute for Extraterrestrial Physics (DE), Université Bourgogne Franche-Comté (FR), AlbaNova (SE), Infrared Processing and Analysis Center (US), The University of Texas at Austin (US)
Openalex Percentile: Top 8%
Radiation Detection and Scintillator Technologies
3.77
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