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Cosmological-scale Lyα Forest Absorption around Galaxies and AGNs Probed with the HETDEX and SDSS Spectroscopic Data

Sun, Dongsheng; Mawatari, Ken; Ouchi, Masami; Ono, Yoshiaki; Yajima, Hidenobu; Zhang, Yechi; Abe, Makito; Bowman, William P.; Cooper, Erin Mentuch; Davis, Dustin; Farrow, Daniel J.; Gebhardt, Karl; Hill, Gary J.; Liu, Chenxu; Schneider, Donald P.

Authors

Dongsheng Sun

Ken Mawatari

Masami Ouchi

Yoshiaki Ono

Hidenobu Yajima

Yechi Zhang

Makito Abe

William P. Bowman

Erin Mentuch Cooper

Dustin Davis

Karl Gebhardt

Gary J. Hill

Chenxu Liu

Donald P. Schneider



Abstract

We present cosmological-scale three-dimensional neutral hydrogen (H i) tomographic maps at z = 2-3 over a total of 837 deg2 in two blank fields that are developed with Lyα forest absorptions of 14,736 background Sloan Digital Sky Survey (SDSS) quasars at z = 2.08-3.67. Using the tomographic maps, we investigate the large-scale (≳10 h −1 cMpc) average H i radial profiles and two-direction profiles of the line-of-sight (LOS) and transverse directions around galaxies and active galactic nuclei (AGNs) at z = 2-3 identified by the Hobby-Eberly Telescope Dark Energy eXperiment survey and SDSS, respectively. The peak of the H i radial profile around galaxies is lower than the one around AGNs, suggesting that the dark matter halos of galaxies are less massive on average than those of AGNs. The LOS profile of AGNs is narrower than the transverse profile, indicating the Kaiser effect. There exist weak absorption outskirts at ≳30 h −1 cMpc beyond H i structures of galaxies and AGNs found in the LOS profiles that can be explained by the H i gas at ≳30 h −1 cMpc falling toward the source position. Our findings indicate that the H i radial profile of AGNs has transitions from proximity zones (≲a few h −1 cMpc) to the H i structures (∼1-30 h −1 cMpc) and the weak absorption outskirts (≳30 h −1 cMpc). Although there is no significant dependence of AGN types (type 1 vs. type 2) on the H i profiles, the peaks of the radial profiles anticorrelate with AGN luminosities, suggesting that AGNs’ ionization effects are stronger than the gas mass differences.

Citation

Sun, D., Mawatari, K., Ouchi, M., Ono, Y., Yajima, H., Zhang, Y., Abe, M., Bowman, W. P., Cooper, E. M., Davis, D., Farrow, D. J., Gebhardt, K., Hill, G. J., Liu, C., & Schneider, D. P. (2023). Cosmological-scale Lyα Forest Absorption around Galaxies and AGNs Probed with the HETDEX and SDSS Spectroscopic Data. The Astrophysical journal, 951(1), Article 25. https://doi.org/10.3847/1538-4357/accf88

Journal Article Type Article
Acceptance Date Apr 20, 2023
Online Publication Date Jun 29, 2023
Publication Date Jul 1, 2023
Deposit Date Apr 17, 2024
Publicly Available Date Apr 23, 2024
Journal Astrophysical Journal
Print ISSN 0004-637X
Electronic ISSN 1538-4357
Publisher American Astronomical Society
Peer Reviewed Peer Reviewed
Volume 951
Issue 1
Article Number 25
DOI https://doi.org/10.3847/1538-4357/accf88
Public URL https://hull-repository.worktribe.com/output/4626435

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Publisher Licence URL
http://creativecommons.org/licenses/by/4.0

Copyright Statement
© 2023. 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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