M Fossati
MUSE analysis of gas around galaxies (MAGG) – III. The gas and galaxy environment of z = 3–4.5 quasars
Fossati, M; Fumagalli, M; Lofthouse, EK; Dutta, R; Cantalupo, S; Arrigoni Battaia, F; Fynbo, JPU; Lusso, E; Murphy, MT; Prochaska, JX; Theuns, T; Cooke, RJ
Authors
M Fumagalli
EK Lofthouse
R Dutta
S Cantalupo
F Arrigoni Battaia
JPU Fynbo
E Lusso
MT Murphy
JX Prochaska
Professor Tom Theuns tom.theuns@durham.ac.uk
Professor
Professor Ryan Cooke ryan.j.cooke@durham.ac.uk
Professor
Abstract
We present a study of the environment of 27 z = 3–4.5 bright quasars from the MUSE Analysis of Gas around Galaxies (MAGG) survey. With medium-depth Multi Unit Spectroscopic Explorer (MUSE) observations (4 h on target per field), we characterize the effects of quasars on their surroundings by studying simultaneously the properties of extended gas nebulae and Ly α emitters (LAEs) in the quasar host haloes. We detect extended (up to ≈100 kpc) Ly α emission around all MAGG quasars, finding a very weak redshift evolution between z = 3 and z = 6. By stacking the MUSE datacubes, we confidently detect extended emission of C IV and only marginally detect extended He II up to ≈40 kpc, implying that the gas is metal enriched. Moreover, our observations show a significant overdensity of LAEs within 300 km s−1 from the quasar systemic redshifts estimated from the nebular emission. The luminosity functions and equivalent width distributions of these LAEs show similar shapes with respect to LAEs away from quasars suggesting that the Ly α emission of the majority of these sources is not significantly boosted by the quasar radiation or other processes related to the quasar environment. Within this framework, the observed LAE overdensities and our kinematic measurements imply that bright quasars at z = 3–4.5 are hosted by haloes in the mass range ≈1012.0−−1012.5 M⊙.
Citation
Fossati, M., Fumagalli, M., Lofthouse, E., Dutta, R., Cantalupo, S., Arrigoni Battaia, F., Fynbo, J., Lusso, E., Murphy, M., Prochaska, J., Theuns, T., & Cooke, R. (2021). MUSE analysis of gas around galaxies (MAGG) – III. The gas and galaxy environment of z = 3–4.5 quasars. Monthly Notices of the Royal Astronomical Society, 503(2), 3044-3064. https://doi.org/10.1093/mnras/stab660
Journal Article Type | Article |
---|---|
Acceptance Date | Mar 1, 2021 |
Online Publication Date | Mar 8, 2021 |
Publication Date | 2021-05 |
Deposit Date | Jul 14, 2021 |
Publicly Available Date | Jul 14, 2021 |
Journal | Monthly Notices of the Royal Astronomical Society |
Print ISSN | 0035-8711 |
Electronic ISSN | 1365-2966 |
Publisher | Royal Astronomical Society |
Peer Reviewed | Peer Reviewed |
Volume | 503 |
Issue | 2 |
Pages | 3044-3064 |
DOI | https://doi.org/10.1093/mnras/stab660 |
Public URL | https://durham-repository.worktribe.com/output/1245568 |
Files
Published Journal Article
(7.4 Mb)
PDF
Copyright Statement
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2021 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
You might also like
The impact and response of mini-haloes and the interhalo medium on cosmic reionization
(2024)
Journal Article
Downloadable Citations
About Durham Research Online (DRO)
Administrator e-mail: dro.admin@durham.ac.uk
This application uses the following open-source libraries:
SheetJS Community Edition
Apache License Version 2.0 (http://www.apache.org/licenses/)
PDF.js
Apache License Version 2.0 (http://www.apache.org/licenses/)
Font Awesome
SIL OFL 1.1 (http://scripts.sil.org/OFL)
MIT License (http://opensource.org/licenses/mit-license.html)
CC BY 3.0 ( http://creativecommons.org/licenses/by/3.0/)
Powered by Worktribe © 2025
Advanced Search