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  5. New quasar proximity zone size measurements at z ∼ 6 using the enlarged XQR-30 sample
 

New quasar proximity zone size measurements at z ∼ 6 using the enlarged XQR-30 sample

Journal
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY  
Date Issued
2023
Author(s)
Satyavolu, Sindhu
•
Eilers, Anna-Christina
•
Kulkarni, Girish
•
Ryan-Weber, Emma
•
Davies, Rebecca L.
•
Becker, George D.
•
Bosman, Sarah E. I.
•
Greig, Bradley
•
Mazzucchelli, Chiara
•
Bañados, Eduardo
•
BISCHETTI, Manuela  
•
D'ODORICO, Valentina  
•
Fan, Xiaohui
•
Farina, Emanuele Paolo
•
Haehnelt, Martin G.
•
Keating, Laura C.
•
Lai, Samuel
•
Walter, Fabian
DOI
10.1093/mnras/stad1326
Abstract
Proximity zones of high-redshift quasars are unique probes of their central supermassive black holes as well as the intergalactic medium (IGM) in the last stages of reionization. We present 22 new measurements of proximity zones of quasars with redshifts between 5.8 and 6.6, using the enlarged XQR-30 sample of high-resolution, high-SNR quasar spectra. The quasars in our sample have ultraviolet magnitudes of M1450 ~ -27 and black hole masses of 109-1010 M⊙. Our inferred proximity zone sizes are 2-7 physical Mpc, with a typical uncertainty of less than 0.5 physical Mpc, which, for the first time, also includes uncertainty in the quasar continuum. We find that the correlation between proximity zone sizes and the quasar redshift, luminosity, or black hole mass, indicates a large diversity of quasar lifetimes. Two of our proximity zone sizes are exceptionally small. The spectrum of one of these quasars, with z = 6.02, displays, unusually for this redshift, damping wing absorption without any detectable metal lines, which could potentially originate from the IGM. The other quasar has a high-ionization absorber ~0.5 pMpc from the edge of the proximity zone. This work increases the number of proximity zone measurements available in the last stages of cosmic reionization to 87. This data will lead to better constraints on quasar lifetimes and obscuration fractions at high redshift, that in turn will help probe the seed mass and formation redshift of supermassive black holes.
Volume
522
Issue
4
Start page
4918
Uri
http://hdl.handle.net/20.500.12386/35413
Url
https://academic.oup.com/mnras/article/522/4/4918/7150699
http://arxiv.org/abs/2305.00998v1
Issn Identifier
0035-8711
Ads BibCode
2023MNRAS.522.4918S
Rights
open.access
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