The need for obscured supermassive black hole growth to explain quasar proximity zones in the epoch of reionization (2023)

First Author: Satyavolu S

Attributed to: Durham DiRAC-2 petascale facility funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1093/mnras/stad729

Publication URI: http://dx.doi.org/10.1093/mnras/stad729

Type: Journal Article/Review

Parent Publication: Monthly Notices of the Royal Astronomical Society

Issue: 2