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