Measuring the Variance of the Macquart Relation in Redshift–Extragalactic Dispersion Measure Modeling by Jay Baptista, J. Xavier Prochaska, Alexandra G. Mannings, C. W. James, R. M. Shannon, Stuart D. Ryder, A. T. Deller, Danica R. Scott, Marcin Glowacki, Nicolas Tejos

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EIGER. I. A Large Sample of [O iii]-emitting Galaxies at 5.3 < z < 6.9 and Direct Evidence for Local Reionization by Galaxies by Daichi Kashino, Simon J. Lilly, Jorryt Matthee, Anna-Christina Eilers, Ruari Mackenzie, Rongmon Bordoloi, Robert A. Simcoe

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UV and Lyα Halos of Lyα Emitters across Environments at z = 2.84 by Satoshi Kikuta, Yuichi Matsuda, Shigeki Inoue, Charles C. Steidel, Renyue Cen, Zheng Zheng, Hidenobu Yajima, Rieko Momose, Masatoshi Imanishi, Yutaka Komiyama

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Magnetogenesis in a Collisionless Plasma: From Weibel Instability to Turbulent Dynamo by Muni Zhou, Vladimir Zhdankin, Matthew W. Kunz, Nuno F. Loureiro, Dmitri A. Uzdensky

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Reconstructing Lyα Fields from Low-resolution Hydrodynamical Simulations with Deep Learning by Cooper Jacobus, Peter Harrington, Zarija Lukić

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Cosmological redshift and Hubble tension explained by means of the FLRWT time-metric framework and transit physics in the IGM by Alessandro Trinchera

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Quasar Factor Analysis—An Unsupervised and Probabilistic Quasar Continuum Prediction Algorithm with Latent Factor Analysis by Zechang Sun, Yuan-Sen Ting, Zheng Cai

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The Origin of Intergalactic Light in Compact Groups of Galaxies by Mark J. Henriksen

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The Bimodal Absorption System Imaging Campaign (BASIC). I. A Dual Population of Low-metallicity Absorbers at z < 1 by Michelle A. Berg, Nicolas Lehner, J. Christopher Howk, John M. O’Meara, Joop Schaye, Lorrie A. Straka, Kathy L. Cooksey, Todd M. Tripp, J. Xavier Prochaska, Benjamin D. Oppenheimer, Sean D. Johnson, Sowgat Muzahid, Rongmon Bordoloi, Jessica K. Werk, Andrew J. Fox, Neal Katz, Martin Wendt, Molly S. Peeples, Joseph Ribaudo, Jason Tumlinson

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Simulating the Detection of the Global 21 cm Signal with MIST for Different Models of the Soil and Beam Directivity by Raul A. Monsalve, Christian H. Bye, Jonathan L. Sievers, Vadym Bidula, Ricardo Bustos, H. Cynthia Chiang, Xinze Guo, Ian Hendricksen, Francis McGee, F. Patricio Mena, Garima Prabhakar, Oscar Restrepo, Nithyanandan Thyagarajan

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The Cool Circumgalactic Medium of Low-redshift Star-forming Galaxies. I. Empirical Model and Mean Properties by Yakov Faerman, Jessica K. Werk

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Evidence of Extended Dust and Feedback around z ≈ 1 Quiescent Galaxies via Millimeter Observations by Jeremy Meinke, Seth Cohen, Jenna Moore, Kathrin Böckmann, Philip Mauskopf, Evan Scannapieco

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Observational Evidence for Large-scale Gas Heating in a Galaxy Protocluster at z = 2.30 by Chenze Dong, Khee-Gan Lee, Metin Ata, Benjamin Horowitz, Rieko Momose

Subjects: “…Intergalactic medium…”
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Detection of Thermal Sunyaev–Zel’dovich Effect in the Circumgalactic Medium of Low-mass Galaxies—A Surprising Pattern in Self-similarity and Baryon Sufficiency by Sanskriti Das, Yi-Kuan Chiang, Smita Mathur

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Radio Astronomy by Shao, Micheal, Staelin, David H., Melcher, James R., Rosenkranz, Philip W., Barrett, Alan H., Myers, Philip C., Burke, Bernard F., Walker, Robert C., Haschick, Aubrey D., Giuffrida, Thomas S., Garcia-Barreto, J. Antonio

Subjects: “…Radio Astronomy Studies of the Intergalactic Medium…”
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Resistive Magnetic Field Generation at Cosmic Dawn by Miniati, F, Bell, A

“…Relativistic charged particles (CR for cosmic-rays) produced by Supernova explosion of the first generation of massive stars that are responsible for the re-ionization of the universe escape into the intergalactic medium, carrying an electric current. Charge imbalance and induction give rise to a return current, $\vec j_t$, carried by the cold thermal plasma which tends to cancel the CR current. …”

The discovery of a galaxy-wide superwind from a young massive galaxy at redshift z approximately 3. by Wilman, R, Gerssen, J, Bower, R, Morris, S, Bacon, R, de Zeeuw, P, Davies, R

“…This screen was ejected from the galaxy during a starburst several 10(8) years earlier and has subsequently swept up gas from the surrounding intergalactic medium and cooled. This demonstrates the galaxy-wide impact of high-redshift superwinds.…”

Probing the epoch of reionization with redshifted 21 cm HI emission by Bowman, Judd D. (Judd David)

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Baryons in the Cosmic Web of IllustrisTNG – I: gas in knots, filaments, sheets, and voids by Martizzi, Davide, Vogelsberger, Mark, Artale, Maria Celeste, Haider, Markus, Torrey, Paul, Marinacci, Federico, Nelson, Dylan, Pillepich, Annalisa, Weinberger, Rainer, Hernquist, Lars, Naiman, Jill, Springel, Volker

“…We also show that the cool, diffuse intergalactic medium [IGM; $T\lt 105 \, {\rm K}$, $n-{\rm H}\lt 10{-4}(1+z) \, {\rm cm{-3}}$] and the warm-hot intergalactic medium [WHIM; $105 \lt T\lt 107 \, {\rm K}$, $n-{\rm H} \lt 10{-4}(1+z)\, {\rm cm{-3}}$] constitute ${\sim } 39$ and ${\sim } 46{{\ \rm per\ cent}}$ of the baryons at redshift z = 0, respectively. …”
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Planck intermediate results. VIII. Filaments between interacting clusters by Collaboration, P, Ade, P, Aghanim, N, Arnaud, M, Ashdown, M, Atrio-Barandela, F, Aumont, J, Baccigalupi, C, Balbi, A, Banday, A, Barreiro, R, Bartlett, J, Battaner, E, Benabed, K, Benoît, A, Bernard, J, Bersanelli, M, Bhatia, R, Bikmaev, I, Böhringer, H, Bonaldi, A, Bond, JR, Borrill, J, Bouchet, F, Bourdin, H

“…Cluster pairs are good candidates for searching for the hotter and denser phase of the intergalactic medium (which is more easily observed through the SZ effect). …”