Discovery of a Powerful >10^61 erg AGN Outburst in Distant Galaxy Cluster SPT-CLJ0528-5300
We present ~103 ks of Chandra observations of the galaxy cluster SPT-CLJ0528-5300 (SPT0528, z=0.768). This cluster harbors the most radio-loud (L_1.4GHz = 1.01 x 10^33 erg/s/Hz) central AGN of any cluster in the South Pole Telescope (SPT) SZ survey with available X-ray data. We find evidence of AGN-...
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ftdatacite:10.48550/arxiv.1911.12828 2023-05-15T18:23:04+02:00 Discovery of a Powerful >10^61 erg AGN Outburst in Distant Galaxy Cluster SPT-CLJ0528-5300 Calzadilla, Michael S. McDonald, Michael Bayliss, Matthew Benson, Bradford A. Bleem, Lindsey E. Brodwin, Mark Edge, Alastair C. Floyd, Benjamin Gupta, Nikhel Hlavacek-Larrondo, Julie McNamara, Brian R. Reichardt, Christian L. 2019 https://dx.doi.org/10.48550/arxiv.1911.12828 https://arxiv.org/abs/1911.12828 unknown arXiv https://dx.doi.org/10.3847/2041-8213/ab5b07 arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ Astrophysics of Galaxies astro-ph.GA Cosmology and Nongalactic Astrophysics astro-ph.CO High Energy Astrophysical Phenomena astro-ph.HE FOS Physical sciences article-journal Article ScholarlyArticle Text 2019 ftdatacite https://doi.org/10.48550/arxiv.1911.12828 https://doi.org/10.3847/2041-8213/ab5b07 2022-03-10T16:27:27Z We present ~103 ks of Chandra observations of the galaxy cluster SPT-CLJ0528-5300 (SPT0528, z=0.768). This cluster harbors the most radio-loud (L_1.4GHz = 1.01 x 10^33 erg/s/Hz) central AGN of any cluster in the South Pole Telescope (SPT) SZ survey with available X-ray data. We find evidence of AGN-inflated cavities in the X-ray emission, which are consistent with the orientation of the jet direction revealed by ATCA radio data. The combined probability that two such depressions -- each at ~1.4-1.8sigma significance, oriented ~180 degrees apart and aligned with the jet axis -- would occur by chance is 0.1%. At >10^61 erg, the outburst in SPT0528 is among the most energetic known in the universe, and certainly the most powerful known at z>0.25. This work demonstrates that such powerful outbursts can be detected even in shallow X-ray exposures out to relatively high redshifts (z~0.8), providing an avenue for studying the evolution of extreme AGN feedback. The ratio of the cavity power (P_cav = 9.4+/-5.8 x 10^45 erg/s) to the cooling luminosity (L_cool = 1.5+/-0.5 x 10^44 erg/s) for SPT0528 is among the highest measured to date. If, in the future, additional systems are discovered at similar redshifts with equally high P_cav/L_cool ratios, it would imply that the feedback/cooling cycle was not as gentle at high redshifts as in the low-redshift universe. : Accepted to ApJL. 8 pages, 5 figures Article in Journal/Newspaper South pole DataCite Metadata Store (German National Library of Science and Technology) South Pole |
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DataCite Metadata Store (German National Library of Science and Technology) |
op_collection_id |
ftdatacite |
language |
unknown |
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Astrophysics of Galaxies astro-ph.GA Cosmology and Nongalactic Astrophysics astro-ph.CO High Energy Astrophysical Phenomena astro-ph.HE FOS Physical sciences |
spellingShingle |
Astrophysics of Galaxies astro-ph.GA Cosmology and Nongalactic Astrophysics astro-ph.CO High Energy Astrophysical Phenomena astro-ph.HE FOS Physical sciences Calzadilla, Michael S. McDonald, Michael Bayliss, Matthew Benson, Bradford A. Bleem, Lindsey E. Brodwin, Mark Edge, Alastair C. Floyd, Benjamin Gupta, Nikhel Hlavacek-Larrondo, Julie McNamara, Brian R. Reichardt, Christian L. Discovery of a Powerful >10^61 erg AGN Outburst in Distant Galaxy Cluster SPT-CLJ0528-5300 |
topic_facet |
Astrophysics of Galaxies astro-ph.GA Cosmology and Nongalactic Astrophysics astro-ph.CO High Energy Astrophysical Phenomena astro-ph.HE FOS Physical sciences |
description |
We present ~103 ks of Chandra observations of the galaxy cluster SPT-CLJ0528-5300 (SPT0528, z=0.768). This cluster harbors the most radio-loud (L_1.4GHz = 1.01 x 10^33 erg/s/Hz) central AGN of any cluster in the South Pole Telescope (SPT) SZ survey with available X-ray data. We find evidence of AGN-inflated cavities in the X-ray emission, which are consistent with the orientation of the jet direction revealed by ATCA radio data. The combined probability that two such depressions -- each at ~1.4-1.8sigma significance, oriented ~180 degrees apart and aligned with the jet axis -- would occur by chance is 0.1%. At >10^61 erg, the outburst in SPT0528 is among the most energetic known in the universe, and certainly the most powerful known at z>0.25. This work demonstrates that such powerful outbursts can be detected even in shallow X-ray exposures out to relatively high redshifts (z~0.8), providing an avenue for studying the evolution of extreme AGN feedback. The ratio of the cavity power (P_cav = 9.4+/-5.8 x 10^45 erg/s) to the cooling luminosity (L_cool = 1.5+/-0.5 x 10^44 erg/s) for SPT0528 is among the highest measured to date. If, in the future, additional systems are discovered at similar redshifts with equally high P_cav/L_cool ratios, it would imply that the feedback/cooling cycle was not as gentle at high redshifts as in the low-redshift universe. : Accepted to ApJL. 8 pages, 5 figures |
format |
Article in Journal/Newspaper |
author |
Calzadilla, Michael S. McDonald, Michael Bayliss, Matthew Benson, Bradford A. Bleem, Lindsey E. Brodwin, Mark Edge, Alastair C. Floyd, Benjamin Gupta, Nikhel Hlavacek-Larrondo, Julie McNamara, Brian R. Reichardt, Christian L. |
author_facet |
Calzadilla, Michael S. McDonald, Michael Bayliss, Matthew Benson, Bradford A. Bleem, Lindsey E. Brodwin, Mark Edge, Alastair C. Floyd, Benjamin Gupta, Nikhel Hlavacek-Larrondo, Julie McNamara, Brian R. Reichardt, Christian L. |
author_sort |
Calzadilla, Michael S. |
title |
Discovery of a Powerful >10^61 erg AGN Outburst in Distant Galaxy Cluster SPT-CLJ0528-5300 |
title_short |
Discovery of a Powerful >10^61 erg AGN Outburst in Distant Galaxy Cluster SPT-CLJ0528-5300 |
title_full |
Discovery of a Powerful >10^61 erg AGN Outburst in Distant Galaxy Cluster SPT-CLJ0528-5300 |
title_fullStr |
Discovery of a Powerful >10^61 erg AGN Outburst in Distant Galaxy Cluster SPT-CLJ0528-5300 |
title_full_unstemmed |
Discovery of a Powerful >10^61 erg AGN Outburst in Distant Galaxy Cluster SPT-CLJ0528-5300 |
title_sort |
discovery of a powerful >10^61 erg agn outburst in distant galaxy cluster spt-clj0528-5300 |
publisher |
arXiv |
publishDate |
2019 |
url |
https://dx.doi.org/10.48550/arxiv.1911.12828 https://arxiv.org/abs/1911.12828 |
geographic |
South Pole |
geographic_facet |
South Pole |
genre |
South pole |
genre_facet |
South pole |
op_relation |
https://dx.doi.org/10.3847/2041-8213/ab5b07 |
op_rights |
arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ |
op_doi |
https://doi.org/10.48550/arxiv.1911.12828 https://doi.org/10.3847/2041-8213/ab5b07 |
_version_ |
1766202486729736192 |