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The need for obscured supermassive black hole growth to explain quasar proximity zones in the epoch of reionization (2022)

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/10.48550/arxiv.2209.08103

Publication URI: https://arxiv.org/abs/2209.08103

Type: Other