Discovery of a 21 cm Absorption System at <i>z</i> = 2.327 with CHIME

Abstract We report the detection of a new 21 cm absorption system associated with the radio source NVSS J164725 + 375218 at a redshift of z = 2.327, identified through a pilot survey conducted by the Canadian Hydrogen Intensity Mapping Experiment (CHIME). This is the fifth detection of an associated system at z &gt; 2. By analyzing a subset of available data, we conduct a spectrally blind survey for 21 cm absorption systems within the redshift range of 0.78–2.55 along 202 lines of sight toward known sources in the declination range of 35° to 60°. We detect three 21 cm absorbers: two previously known intervening systems and one newly discovered associated system. By fitting the absorption profiles with models containing one to three Gaussian components and selecting the best model using the Bayesian information criterion, we estimate the optical depth, velocity-integrated optical depth, and the ratio between the H i column density and the spin temperature of the absorption systems. These results demonstrate CHIME’s ability to discover new absorbers, even in a small subset of its full dataset.

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Publication Details

Journal
The Astrophysical Journal
Published
2026-02-18
DOI
https://doi.org/10.3847/1538-4357/ae3de7
Primary Topic
Astrophysics and Cosmic Phenomena
Type
article
Field-Weighted Citation Impact
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article

Discovery of a 21 cm Absorption System at z = 2.327 with CHIME

C. Höfer, Arash Mirhosseini, Joshua MacEachern, Arnab Chakraborty et al.
The Astrophysical Journal
Astrophysics and Cosmic Phenomena
article

Discovery of a 21 cm Absorption System at z = 2.327 with CHIME

C. Höfer, Arash Mirhosseini, Joshua MacEachern, Arnab Chakraborty, F. X. Simon, R. van Lieshout, Albin Joseph, Yukari Uchibori, Dallas Wulf, Ue-Li Pen, Alex Reda, Tristan Pinsonneault-Marotte, Mandana Amiri, Seth R. Siegel, Alex S. Hill, Haochen Wang, Juan Mena-Parra, Mark Halpern, J. Richard Shaw, Gary Hinshaw, Kiyoshi W. Masui
article en

Abstract

Abstract We report the detection of a new 21 cm absorption system associated with the radio source NVSS J164725 + 375218 at a redshift of z = 2.327, identified through a pilot survey conducted by the Canadian Hydrogen Intensity Mapping Experiment (CHIME). This is the fifth detection of an associated system at z &gt; 2. By analyzing a subset of available data, we conduct a spectrally blind survey for 21 cm absorption systems within the redshift range of 0.78–2.55 along 202 lines of sight toward known sources in the declination range of 35° to 60°. We detect three 21 cm absorbers: two previously known intervening systems and one newly discovered associated system. By fitting the absorption profiles with models containing one to three Gaussian components and selecting the best model using the Bayesian information criterion, we estimate the optical depth, velocity-integrated optical depth, and the ratio between the H i column density and the spin temperature of the absorption systems. These results demonstrate CHIME’s ability to discover new absorbers, even in a small subset of its full dataset.

The Astrophysical JournalVol. 998(2)
Openalex Percentile: Top 49%
Astrophysics and Cosmic Phenomena
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