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