Brightest cluster galaxy formation in the z = 4.3 protocluster SPT 2349-56 : discovery of a radio-loud active galactic nucleus
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Date
Authors
Chapman, S.C.
Hill, Ryley
Aravena, Manuel
Archipley, Melanie
Babul, Arif
Burgoyne, James
Canning, Rebecca E. A.
Deane, Roger
De Breuck, Carlos
Gonzalez, Anthony H.
Journal Title
Journal ISSN
Volume Title
Publisher
IOP Publishing
Abstract
Please read abstract in article.
Description
This paper includes archived data obtained through the CSIRO ASKAP Science Data Archive, CASDA (http://data.csiro.au). This paper makes use of the following ALMA data: ADS/JAO.ALMA#2015.1.01543.T, ADS/JAO.ALMA#2018.1.00058.S, and ADS/JAO.ALMA#2021.1.01010.P. ALMA is a partnership of ESO (representing its member states), NSF (USA) and NINS (Japan), together with NRC (Canada), MOST and ASIAA (Taiwan), and KASI (Republic of Korea), in cooperation with the Republic of Chile.
Keywords
Protocluster, Radio-loud, Submillimeter galaxies (SMGs), SDG-09: Industry, innovation and infrastructure, Active galactic nuclei (AGN), Australia telescope compact array (ATCA), Atacama large millimeter array (ALMA)
Sustainable Development Goals
SDG-09: Industry, innovation and infrastructure
Citation
Chapman, S.C., Hill, R., Aravena, M. et al. 2024, 'Brightest cluster galaxy formation in the z = 4.3 protocluster SPT 2349-56 : discovery of a radio-loud active galactic nucleus', The Astrophysical Journal, vol. 961, pp. 1-25, doi : 10.3847/1538-4357/ad0b77.