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:  Peta-5: A National Facility for Petascale Data Intensive Computation and Analytics funded by EPSRC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.17863/cam.104211

Publication URI: https://www.repository.cam.ac.uk/handle/1810/361266

Type: Journal Article/Review