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dc.contributor.author | Chapman, S.C.![]() |
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dc.contributor.author | Hill, Ryley![]() |
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dc.contributor.author | Aravena, Manuel![]() |
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dc.contributor.author | Archipley, Melanie![]() |
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dc.contributor.author | Babul, Arif![]() |
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dc.contributor.author | Burgoyne, James![]() |
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dc.contributor.author | Canning, Rebecca E. A.![]() |
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dc.contributor.author | Deane, Roger![]() |
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dc.contributor.author | De Breuck, Carlos![]() |
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dc.contributor.author | Gonzalez, Anthony H.![]() |
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dc.contributor.author | Hayward, Christopher C.![]() |
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dc.contributor.author | Kim, Seon Woo![]() |
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dc.contributor.author | Malkan, Matt![]() |
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dc.contributor.author | Marrone, D.P.![]() |
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dc.contributor.author | McIntyre, Vincent![]() |
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dc.contributor.author | Murphy, Eric J.![]() |
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dc.contributor.author | Pass, Emily![]() |
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dc.contributor.author | Perry, Ryan W.![]() |
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dc.contributor.author | Phadke, Kedar A.![]() |
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dc.contributor.author | Rennehan, Douglas![]() |
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dc.contributor.author | Reuter, Cassie![]() |
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dc.contributor.author | Rotermund, Kaja M.![]() |
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dc.contributor.author | Scott, Douglas![]() |
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dc.contributor.author | Seymour, Nick![]() |
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dc.contributor.author | Solimano, Manuel![]() |
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dc.contributor.author | Spilker, Justin![]() |
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dc.contributor.author | Stark, Anthony A.![]() |
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dc.contributor.author | Sulzenauer, Nikolaus![]() |
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dc.contributor.author | Tothill, Nick![]() |
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dc.contributor.author | Vieira, Joaquin D.![]() |
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dc.contributor.author | Vizgan, David![]() |
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dc.contributor.author | Wang, George![]() |
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dc.contributor.author | Weiss, Axel![]() |
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dc.date.accessioned | 2024-08-19T12:10:47Z | |
dc.date.available | 2024-08-19T12:10:47Z | |
dc.date.issued | 2024-01 | |
dc.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. | en_US |
dc.description.abstract | Please read abstract in article. | en_US |
dc.description.department | Physics | en_US |
dc.description.sdg | SDG-09: Industry, innovation and infrastructure | en_US |
dc.description.sponsorship | The Australia Telescope Compact Array is part of the Australia Telescope National Facility (https://ror.org/05qajvd42), which is funded by the Australian Government for operation as a National Facility managed by CSIRO. The research of R.P.D. is supported by the South African Research Chairs Initiative of the Department of Science and Innovation and National Research Foundation. Operation of ASKAP is funded by the Australian Government with support from the National Collaborative Research Infrastructure Strategy. | en_US |
dc.description.uri | https://iopscience.iop.org/journal/0004-637X | en_US |
dc.identifier.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. | en_US |
dc.identifier.issn | 0004-637X (print) | |
dc.identifier.issn | 1538-4357 (online) | |
dc.identifier.other | 10.3847/1538-4357/ad0b77 | |
dc.identifier.uri | http://hdl.handle.net/2263/97718 | |
dc.language.iso | en | en_US |
dc.publisher | IOP Publishing | en_US |
dc.rights | © 2024. The Author(s). Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. | en_US |
dc.subject | Protocluster | en_US |
dc.subject | Radio-loud | en_US |
dc.subject | Submillimeter galaxies (SMGs) | en_US |
dc.subject | SDG-09 | en_US |
dc.subject | Active galactic nuclei (AGN) | en_US |
dc.subject | Australia telescope compact array (ATCA) | en_US |
dc.subject | Atacama large millimeter array (ALMA) | en_US |
dc.title | Brightest cluster galaxy formation in the z = 4.3 protocluster SPT 2349-56 : discovery of a radio-loud active galactic nucleus | en_US |
dc.type | Article | en_US |