The evolution of AGN activity in brightest cluster galaxies
Somboonpanyakul et al. We present the results of an analysis of Wide-field Infrared Survey Explorer (WISE) observations of the full 2500 deg2 South Pole Telescope (SPT)-Sunyaev–Zel'dovich cluster sample. We describe a process for identifying active galactic nuclei (AGN) in brightest cluster gal...
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ftcsic:oai:digital.csic.es:10261/296028 2024-02-11T10:08:43+01:00 The evolution of AGN activity in brightest cluster galaxies Somboonpanyakul, T. McDonald, M. Carretero, Jorge Costanzi, M. Garcia-Bellido, Juan Gaztañaga, Enrique Serrano, S. Sevilla-Noarbe, I. Wilkinson, Reese D. National Aeronautics and Space Administration (US) National Science Foundation (US) Department of Energy (US) 2022 application/pdf http://hdl.handle.net/10261/296028 https://doi.org/10.3847/1538-3881/ac5030 en eng IOP Publishing Astronomical Journal Publisher's version https://doi.org/10.3847/1538-3881/ac5030 Sí Astronomical Journal 163(4): 146 (2022) http://hdl.handle.net/10261/296028 doi:10.3847/1538-3881/ac5030 1538-3881 open artículo 2022 ftcsic https://doi.org/10.3847/1538-3881/ac5030 2024-01-16T11:38:00Z Somboonpanyakul et al. We present the results of an analysis of Wide-field Infrared Survey Explorer (WISE) observations of the full 2500 deg2 South Pole Telescope (SPT)-Sunyaev–Zel'dovich cluster sample. We describe a process for identifying active galactic nuclei (AGN) in brightest cluster galaxies (BCGs) based on WISE mid-IR color and redshift. Applying this technique to the BCGs of the SPT-SZ sample, we calculate the AGN-hosting BCG fraction, which is defined as the fraction of BCGs hosting bright central AGNs over all possible BCGs. Assuming an evolving single-burst stellar population model, we find statistically significant evidence (>99.9%) for a mid-IR excess at high redshift compared to low redshift, suggesting that the fraction of AGN-hosting BCGs increases with redshift over the range of 0 < z < 1.3. The best-fit redshift trend of the AGN-hosting BCG fraction has the form (1 + z)4.1±1.0. These results are consistent with previous studies in galaxy clusters as well as as in field galaxies. One way to explain this result is that member galaxies at high redshift tend to have more cold gas. While BCGs in nearby galaxy clusters grow mostly by dry mergers with cluster members, leading to no increase in AGN activity, BCGs at high redshift could primarily merge with gas-rich satellites, providing fuel for feeding AGNs. If this observed increase in AGN activity is linked to gas-rich mergers rather than ICM cooling, we would expect to see an increase in scatter in the Pcav versus Lcool relation at z > 1. Last, this work confirms that the runaway cooling phase, as predicted by the classical cooling-flow model, in the Phoenix cluster is extremely rare and most BCGs have low (relative to Eddington) black hole accretion rates. T.S. and M.M. acknowledge support from the Kavli Research Investment Fund at MIT, and from NASA through Chandra grant GO5-16143. F.R. acknowledges financial support provided by NASA through SAO Award Number SV2-82023 issued by the Chandra X-Ray Observatory Center, which is ... Article in Journal/Newspaper South pole Digital.CSIC (Spanish National Research Council) Kavli ENVELOPE(7.837,7.837,62.581,62.581) South Pole The Astronomical Journal 163 4 146 |
institution |
Open Polar |
collection |
Digital.CSIC (Spanish National Research Council) |
op_collection_id |
ftcsic |
language |
English |
description |
Somboonpanyakul et al. We present the results of an analysis of Wide-field Infrared Survey Explorer (WISE) observations of the full 2500 deg2 South Pole Telescope (SPT)-Sunyaev–Zel'dovich cluster sample. We describe a process for identifying active galactic nuclei (AGN) in brightest cluster galaxies (BCGs) based on WISE mid-IR color and redshift. Applying this technique to the BCGs of the SPT-SZ sample, we calculate the AGN-hosting BCG fraction, which is defined as the fraction of BCGs hosting bright central AGNs over all possible BCGs. Assuming an evolving single-burst stellar population model, we find statistically significant evidence (>99.9%) for a mid-IR excess at high redshift compared to low redshift, suggesting that the fraction of AGN-hosting BCGs increases with redshift over the range of 0 < z < 1.3. The best-fit redshift trend of the AGN-hosting BCG fraction has the form (1 + z)4.1±1.0. These results are consistent with previous studies in galaxy clusters as well as as in field galaxies. One way to explain this result is that member galaxies at high redshift tend to have more cold gas. While BCGs in nearby galaxy clusters grow mostly by dry mergers with cluster members, leading to no increase in AGN activity, BCGs at high redshift could primarily merge with gas-rich satellites, providing fuel for feeding AGNs. If this observed increase in AGN activity is linked to gas-rich mergers rather than ICM cooling, we would expect to see an increase in scatter in the Pcav versus Lcool relation at z > 1. Last, this work confirms that the runaway cooling phase, as predicted by the classical cooling-flow model, in the Phoenix cluster is extremely rare and most BCGs have low (relative to Eddington) black hole accretion rates. T.S. and M.M. acknowledge support from the Kavli Research Investment Fund at MIT, and from NASA through Chandra grant GO5-16143. F.R. acknowledges financial support provided by NASA through SAO Award Number SV2-82023 issued by the Chandra X-Ray Observatory Center, which is ... |
author2 |
National Aeronautics and Space Administration (US) National Science Foundation (US) Department of Energy (US) |
format |
Article in Journal/Newspaper |
author |
Somboonpanyakul, T. McDonald, M. Carretero, Jorge Costanzi, M. Garcia-Bellido, Juan Gaztañaga, Enrique Serrano, S. Sevilla-Noarbe, I. Wilkinson, Reese D. |
spellingShingle |
Somboonpanyakul, T. McDonald, M. Carretero, Jorge Costanzi, M. Garcia-Bellido, Juan Gaztañaga, Enrique Serrano, S. Sevilla-Noarbe, I. Wilkinson, Reese D. The evolution of AGN activity in brightest cluster galaxies |
author_facet |
Somboonpanyakul, T. McDonald, M. Carretero, Jorge Costanzi, M. Garcia-Bellido, Juan Gaztañaga, Enrique Serrano, S. Sevilla-Noarbe, I. Wilkinson, Reese D. |
author_sort |
Somboonpanyakul, T. |
title |
The evolution of AGN activity in brightest cluster galaxies |
title_short |
The evolution of AGN activity in brightest cluster galaxies |
title_full |
The evolution of AGN activity in brightest cluster galaxies |
title_fullStr |
The evolution of AGN activity in brightest cluster galaxies |
title_full_unstemmed |
The evolution of AGN activity in brightest cluster galaxies |
title_sort |
evolution of agn activity in brightest cluster galaxies |
publisher |
IOP Publishing |
publishDate |
2022 |
url |
http://hdl.handle.net/10261/296028 https://doi.org/10.3847/1538-3881/ac5030 |
long_lat |
ENVELOPE(7.837,7.837,62.581,62.581) |
geographic |
Kavli South Pole |
geographic_facet |
Kavli South Pole |
genre |
South pole |
genre_facet |
South pole |
op_relation |
Astronomical Journal Publisher's version https://doi.org/10.3847/1538-3881/ac5030 Sí Astronomical Journal 163(4): 146 (2022) http://hdl.handle.net/10261/296028 doi:10.3847/1538-3881/ac5030 1538-3881 |
op_rights |
open |
op_doi |
https://doi.org/10.3847/1538-3881/ac5030 |
container_title |
The Astronomical Journal |
container_volume |
163 |
container_issue |
4 |
container_start_page |
146 |
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1790608272114319360 |