Constraining radio mode feedback in galaxy clusters with the cluster radio AGNs properties to z ∼ 1

Gupta, N.; Pannella, M.; Mohr, J. J.; Klein, M.; Rykoff, E. S.; Annis, J.; Avila, S.; Bianchini, F.; Brooks, D.; Buckley-Geer, E.; Bulbul, E.; Carnero Rosell, A.; Carrasco Kind, M.; Carretero, J.; Chiu, I.; Costanzi, M.; da Costa, L. N.; De Vicente, J.; Desai, S.; Dietrich, J. P.; Doel, P.; Everett, S.; Evrard, A. E.; García-Bellido, J.; Gaztanaga, E.; Gruen, D.; Gruendl, R. A.; Gschwend, J.; Gutierrez, G.; Hollowood, D. L.; Honscheid, K.; James, D. J.; Jeltema, T.; Kuehn, K.; Lidman, C.; Lima, M.; Maia, M. A. G.; Marshall, J. L.; McDonald, M.; Menanteau, F.; Miquel, R.; Ogando, R. L. C.; Palmese, A.; Paz-Chinchón, F.; Plazas, A. A.; Reichardt, C. L.; Sanchez, E.; Santiago, B.; Saro, A.; Scarpine, V.; Schindler, R.; Schubnell, M.; Serrano, S.; Sevilla-Noarbe, I.; Shao, X.; Smith, M.; Stott, J. P.; Strazzullo, V.; Suchyta, E.; Swanson, M. E. C.; Vikram, V.; Zenteno, A.

doi:10.1093/mnras/staa832

Title: Constraining radio mode feedback in galaxy clusters with the cluster radio AGNs properties to z ∼ 1

Abstract

Here, we study the properties of the Sydney University Molonglo Sky Survey (SUMSS) 843 MHz radio active galactic nuclei (AGNs) population in galaxy clusters from two large catalogues created using the Dark Energy Survey (DES): ~11,800 optically selected RM-Y3 and ~1000 X-ray selected MARD-Y3 clusters. We show that cluster radio loud AGNs are highly concentrated around cluster centres to $$z$$ ~ 1. We measure the halo occupation number for cluster radio AGNs above a threshold luminosity, finding that the number of radio AGNs per cluster increases with cluster halo mass as N ∝ M^1.2 ± 0.1 (N ∝ M^{0.68 ± 0.34}) for the RM-Y3 (MARD-Y3) sample. Together, these results indicate that radio mode feedback is favoured in more massive galaxy clusters. Using optical counterparts for these sources, we demonstrate weak redshift evolution in the host broad-band colours and the radio luminosity at fixed host galaxy stellar mass. We use the redshift evolution in radio luminosity to break the degeneracy between density and luminosity evolution scenarios in the redshift trend of the radio AGNs luminosity function (LF). The LF exhibits a redshift trend of the form (1 + $$z$$)^γ in density and luminosity, respectively, of γD = 3.0 ± 0.4 and γP = 0.21 ± 0.15 in the RM-Y3 sample, and γD = 2.6 ± 0.7 and γP = 0.31 ± 0.15 in MARD-Y3. We discuss the physical drivers of radio mode feedback in cluster AGNs, and we use the cluster radio galaxy LF to estimate the average radio-mode feedback energy as a function of cluster mass and redshift and compare it to the core (<0.1R₅₀₀) X-ray radiative losses for clusters at $$z$$ < 1.

Authors:

^[1]; Pannella, M. ^[2]; Mohr, J. J. ^[3]; Klein, M. ^[4]; Rykoff, E. S. ^[5]; Annis, J. ^[6];

^[7]; Bianchini, F. ^[8]; Brooks, D. ^[9];

^[6]; Bulbul, E. ^[10];

^[11];

^[12]; Carretero, J. ^[13];

^[14]; Costanzi, M. ^[2]; da Costa, L. N. ^[15];

^[7]; Desai, S. ^[16]; Dietrich, J. P. ^[17] more »

School of Physics, University of Melbourne, Parkville, VIC 3010, Australia, Faculty of Physics, Ludwig-Maximilians-Universität, Scheinerstr 1, D-81679 Munich, Germany, Excellence Cluster Origins, Boltzmannstr 2, D-85748 Garching, Germany, Max Planck Institute for Extraterrestrial Physics, Giessenbachstr, D-85748 Garching, Germany
Faculty of Physics, Ludwig-Maximilians-Universität, Scheinerstr 1, D-81679 Munich, Germany
Faculty of Physics, Ludwig-Maximilians-Universität, Scheinerstr 1, D-81679 Munich, Germany, Excellence Cluster Origins, Boltzmannstr 2, D-85748 Garching, Germany, Max Planck Institute for Extraterrestrial Physics, Giessenbachstr, D-85748 Garching, Germany
Faculty of Physics, Ludwig-Maximilians-Universität, Scheinerstr 1, D-81679 Munich, Germany, Max Planck Institute for Extraterrestrial Physics, Giessenbachstr, D-85748 Garching, Germany
Kavli Institute for Particle Astrophysics & Cosmology, Stanford University, P. O. Box 2450, Stanford, CA 94305, USA, SLAC National Accelerator Laboratory, Menlo Park, CA 94025, USA
Fermi National Accelerator Laboratory, P. O. Box 500, Batavia, IL 60510, USA
Instituto de Fisica Teorica UAM/CSIC, Universidad Autonoma de Madrid, E-28049 Madrid, Spain
School of Physics, University of Melbourne, Parkville, VIC 3010, Australia
Department of Physics & Astronomy, University College London, Gower Street, London WC1E 6BT, UK
Center for Astrophysics Harvard & Smithsonian, 60 Garden Street, Cambridge, MA 02138, USA, Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, 77 Massachusetts Avenue, Cambridge, MA 02139, USA
Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas (CIEMAT), Madrid, Spain, Laboratório Interinstitucional de e-Astronomia – LIneA, Rua Gal. José Cristino 77, Rio de Janeiro, RJ 20921-400, Brazil
Department of Astronomy, University of Illinois at Urbana-Champaign, 1002 W. Green Street, Urbana, IL 61801, USA, National Center for Supercomputing Applications, 1205 West Clark St., Urbana, IL 61801, USA
Institut de Física d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology, Campus UAB, E-08193 Bellaterra, Barcelona, Spain
Academia Sinica Institute of Astronomy and Astrophysics, 11F of AS/NTU Astronomy-Mathematics Building, No.1, Section 4, Roosevelt Rd, Taipei 10617, Taiwan
Laboratório Interinstitucional de e-Astronomia – LIneA, Rua Gal. José Cristino 77, Rio de Janeiro, RJ 20921-400, Brazil, Observatório Nacional, Rua Gal. José Cristino 77, Rio de Janeiro, RJ 20921-400, Brazil
Department of Physics, IIT Hyderabad, Kandi, Telangana 502285, India
Faculty of Physics, Ludwig-Maximilians-Universität, Scheinerstr 1, D-81679 Munich, Germany, Excellence Cluster Origins, Boltzmannstr 2, D-85748 Garching, Germany
Santa Cruz Institute for Particle Physics, Santa Cruz, CA 95064, USA
Department of Astronomy, University of Michigan, Ann Arbor, MI 48109, USA, Department of Physics, University of Michigan, Ann Arbor, MI 48109, USA
Institut d’Estudis Espacials de Catalunya (IEEC), E-08034 Barcelona, Spain, Institute of Space Sciences (ICE, CSIC), Campus UAB, Carrer de Can Magrans, s/n, E-08193 Barcelona, Spain
Kavli Institute for Particle Astrophysics & Cosmology, Stanford University, P. O. Box 2450, Stanford, CA 94305, USA, SLAC National Accelerator Laboratory, Menlo Park, CA 94025, USA, Department of Physics, Stanford University, 382 Via Pueblo Mall, Stanford, CA 94305, USA
Department of Physics, The Ohio State University, Columbus, OH 43210, USA
Center for Astrophysics Harvard & Smithsonian, 60 Garden Street, Cambridge, MA 02138, USA
Australian Astronomical Optics, Macquarie University, North Ryde, NSW 2113, Australia
The Research School of Astronomy and Astrophysics, Australian National University, ACT 2601, Australia
Laboratório Interinstitucional de e-Astronomia – LIneA, Rua Gal. José Cristino 77, Rio de Janeiro, RJ 20921-400, Brazil, Departamento de Física Matemática, Instituto de Física, Universidade de São Paulo, CP 66318, São Paulo, SP 05314-970, Brazil
George P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy, Department of Physics and Astronomy, Texas A&M University, College Station, TX 77843, USA
Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, 77 Massachusetts Avenue, Cambridge, MA 02139, USA
Institut de Física d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology, Campus UAB, E-08193 Bellaterra, Barcelona, Spain, Institució Catalana de Recerca i Estudis Avançats, E-08010 Barcelona, Spain
Department of Astrophysical Sciences, Princeton University, Peyton Hall, Princeton, NJ 08544, USA
Laboratório Interinstitucional de e-Astronomia – LIneA, Rua Gal. José Cristino 77, Rio de Janeiro, RJ 20921-400, Brazil, Instituto de Física, UFRGS, Caixa Postal 15051, Porto Alegre, RS 91501-970, Brazil
INAF – Osservatorio Astronomico di Trieste, via Tiepolo 11, I-34143 Trieste, Italy, IFPU – Institute for Fundamental Physics of the Universe, Via Beirut 2, I-34014 Trieste, Italy, INAF – Osservatorio Astronomico di Trieste, via G. B. Tiepolo 11, I-34143 Trieste, Italy
SLAC National Accelerator Laboratory, Menlo Park, CA 94025, USA
Department of Physics, University of Michigan, Ann Arbor, MI 48109, USA
School of Physics and Astronomy, University of Southampton, Southampton SO17 1BJ, UK
Department of Physics, Lancaster University, Lancaster LA1 4YB, UK
Computer Science and Mathematics Division, Oak Ridge National Laboratory, Oak Ridge, TN 37831, USA
National Center for Supercomputing Applications, 1205 West Clark St., Urbana, IL 61801, USA
Argonne National Laboratory, 9700 South Cass Avenue, Lemont, IL 60439, USA
Cerro Tololo Inter-American Observatory, Casilla 603, La Serena, Chile

Publication Date:: Fri Apr 03 00:00:00 EDT 2020

Research Org.:: SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States); Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States); Oak Ridge National Laboratory (ORNL), Oak Ridge, TN (United States); Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States). National Energy Research Scientific Computing Center (NERSC); Argonne National Laboratory (ANL), Argonne, IL (United States); Univ. of Michigan, Ann Arbor, MI (United States)

Sponsoring Org.:: USDOE Office of Science (SC), High Energy Physics (HEP); USDOE Office of Science (SC), Advanced Scientific Computing Research (ASCR)

Contributing Org.:: DES Collaboration

OSTI Identifier:: 1616204

Alternate Identifier(s):: OSTI ID: 1615369; OSTI ID: 1638179; OSTI ID: 1659578; OSTI ID: 1756413; OSTI ID: 1785453

Report Number(s):: arXiv:1906.11388; DES-2019-0324; FERMILAB-PUB-19-204-AE
Journal ID: ISSN 0035-8711

Grant/Contract Number:: AC02-05CH11231; AC02-07CH11359; AC02-76SF00515; PLR-1248097; AST-1138766; AST-1536171; GBMF 947; AYA2015-71825; ESP2015-66861; FPA2015-68048; SEV-2016-0588; SEV-2016-0597; MDM-2015-0509; FP7/2007-2013; 240672; 291329; 306478; 465376/2014-2; AC05-00OR22725; AC02-06CH11357; SC0019193

Resource Type:: Published Article

Journal Name:: Monthly Notices of the Royal Astronomical Society

Additional Journal Information:: Journal Name: Monthly Notices of the Royal Astronomical Society Journal Volume: 494 Journal Issue: 2; Journal ID: ISSN 0035-8711

Publisher:: Royal Astronomical Society

Country of Publication:: United Kingdom

Language:: English

Subject:: 79 ASTRONOMY AND ASTROPHYSICS; galaxies: clusters: general; galaxies: active; galaxies: luminosity function, mass function; submillimeter: galaxies; cosmology: observations; galaxies; active; clusters; luminosity function; mass function; cosmology; observations; submillimeter

Citation Formats


                    Gupta, N., Pannella, M., Mohr, J. J., Klein, M., Rykoff, E. S., Annis, J., Avila, S., Bianchini, F., Brooks, D., Buckley-Geer, E., Bulbul, E., Carnero Rosell, A., Carrasco Kind, M., Carretero, J., Chiu, I., Costanzi, M., da Costa, L. N., De Vicente, J., Desai, S., Dietrich, J. P., Doel, P., Everett, S., Evrard, A. E., García-Bellido, J., Gaztanaga, E., Gruen, D., Gruendl, R. A., Gschwend, J., Gutierrez, G., Hollowood, D. L., Honscheid, K., James, D. J., Jeltema, T., Kuehn, K., Lidman, C., Lima, M., Maia, M. A. G., Marshall, J. L., McDonald, M., Menanteau, F., Miquel, R., Ogando, R. L. C., Palmese, A., Paz-Chinchón, F., Plazas, A. A., Reichardt, C. L., Sanchez, E., Santiago, B., Saro, A., Scarpine, V., Schindler, R., Schubnell, M., Serrano, S., Sevilla-Noarbe, I., Shao, X., Smith, M., Stott, J. P., Strazzullo, V., Suchyta, E., Swanson, M. E. C., Vikram, V., and Zenteno, A. Constraining radio mode feedback in galaxy clusters with the cluster radio AGNs properties to z ∼ 1.  United Kingdom: N. p., 2020. 
Web.  doi:10.1093/mnras/staa832.

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                    Gupta, N., Pannella, M., Mohr, J. J., Klein, M., Rykoff, E. S., Annis, J., Avila, S., Bianchini, F., Brooks, D., Buckley-Geer, E., Bulbul, E., Carnero Rosell, A., Carrasco Kind, M., Carretero, J., Chiu, I., Costanzi, M., da Costa, L. N., De Vicente, J., Desai, S., Dietrich, J. P., Doel, P., Everett, S., Evrard, A. E., García-Bellido, J., Gaztanaga, E., Gruen, D., Gruendl, R. A., Gschwend, J., Gutierrez, G., Hollowood, D. L., Honscheid, K., James, D. J., Jeltema, T., Kuehn, K., Lidman, C., Lima, M., Maia, M. A. G., Marshall, J. L., McDonald, M., Menanteau, F., Miquel, R., Ogando, R. L. C., Palmese, A., Paz-Chinchón, F., Plazas, A. A., Reichardt, C. L., Sanchez, E., Santiago, B., Saro, A., Scarpine, V., Schindler, R., Schubnell, M., Serrano, S., Sevilla-Noarbe, I., Shao, X., Smith, M., Stott, J. P., Strazzullo, V., Suchyta, E., Swanson, M. E. C., Vikram, V., & Zenteno, A. Constraining radio mode feedback in galaxy clusters with the cluster radio AGNs properties to z ∼ 1.  United Kingdom.  https://doi.org/10.1093/mnras/staa832

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                    Gupta, N., Pannella, M., Mohr, J. J., Klein, M., Rykoff, E. S., Annis, J., Avila, S., Bianchini, F., Brooks, D., Buckley-Geer, E., Bulbul, E., Carnero Rosell, A., Carrasco Kind, M., Carretero, J., Chiu, I., Costanzi, M., da Costa, L. N., De Vicente, J., Desai, S., Dietrich, J. P., Doel, P., Everett, S., Evrard, A. E., García-Bellido, J., Gaztanaga, E., Gruen, D., Gruendl, R. A., Gschwend, J., Gutierrez, G., Hollowood, D. L., Honscheid, K., James, D. J., Jeltema, T., Kuehn, K., Lidman, C., Lima, M., Maia, M. A. G., Marshall, J. L., McDonald, M., Menanteau, F., Miquel, R., Ogando, R. L. C., Palmese, A., Paz-Chinchón, F., Plazas, A. A., Reichardt, C. L., Sanchez, E., Santiago, B., Saro, A., Scarpine, V., Schindler, R., Schubnell, M., Serrano, S., Sevilla-Noarbe, I., Shao, X., Smith, M., Stott, J. P., Strazzullo, V., Suchyta, E., Swanson, M. E. C., Vikram, V., and Zenteno, A. Fri .  
"Constraining radio mode feedback in galaxy clusters with the cluster radio AGNs properties to z ∼ 1".  United Kingdom.  https://doi.org/10.1093/mnras/staa832.

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@article{osti_1616204,

  title        = {Constraining radio mode feedback in galaxy clusters with the cluster radio AGNs properties to z ∼ 1},

  author       = {Gupta, N. and Pannella, M. and Mohr, J. J. and Klein, M. and Rykoff, E. S. and Annis, J. and Avila, S. and Bianchini, F. and Brooks, D. and Buckley-Geer, E. and Bulbul, E. and Carnero Rosell, A. and Carrasco Kind, M. and Carretero, J. and Chiu, I. and Costanzi, M. and da Costa, L. N. and De Vicente, J. and Desai, S. and Dietrich, J. P. and Doel, P. and Everett, S. and Evrard, A. E. and García-Bellido, J. and Gaztanaga, E. and Gruen, D. and Gruendl, R. A. and Gschwend, J. and Gutierrez, G. and Hollowood, D. L. and Honscheid, K. and James, D. J. and Jeltema, T. and Kuehn, K. and Lidman, C. and Lima, M. and Maia, M. A. G. and Marshall, J. L. and McDonald, M. and Menanteau, F. and Miquel, R. and Ogando, R. L. C. and Palmese, A. and Paz-Chinchón, F. and Plazas, A. A. and Reichardt, C. L. and Sanchez, E. and Santiago, B. and Saro, A. and Scarpine, V. and Schindler, R. and Schubnell, M. and Serrano, S. and Sevilla-Noarbe, I. and Shao, X. and Smith, M. and Stott, J. P. and Strazzullo, V. and Suchyta, E. and Swanson, M. E. C. and Vikram, V. and Zenteno, A.},

  abstractNote = {Here, we study the properties of the Sydney University Molonglo Sky Survey (SUMSS) 843 MHz radio active galactic nuclei (AGNs) population in galaxy clusters from two large catalogues created using the Dark Energy Survey (DES): ~11,800 optically selected RM-Y3 and ~1000 X-ray selected MARD-Y3 clusters. We show that cluster radio loud AGNs are highly concentrated around cluster centres to $z$ ~ 1. We measure the halo occupation number for cluster radio AGNs above a threshold luminosity, finding that the number of radio AGNs per cluster increases with cluster halo mass as N ∝ M1.2 ± 0.1 (N ∝ M0.68 ± 0.34) for the RM-Y3 (MARD-Y3) sample. Together, these results indicate that radio mode feedback is favoured in more massive galaxy clusters. Using optical counterparts for these sources, we demonstrate weak redshift evolution in the host broad-band colours and the radio luminosity at fixed host galaxy stellar mass. We use the redshift evolution in radio luminosity to break the degeneracy between density and luminosity evolution scenarios in the redshift trend of the radio AGNs luminosity function (LF). The LF exhibits a redshift trend of the form (1 + $z$)γ in density and luminosity, respectively, of γD = 3.0 ± 0.4 and γP = 0.21 ± 0.15 in the RM-Y3 sample, and γD = 2.6 ± 0.7 and γP = 0.31 ± 0.15 in MARD-Y3. We discuss the physical drivers of radio mode feedback in cluster AGNs, and we use the cluster radio galaxy LF to estimate the average radio-mode feedback energy as a function of cluster mass and redshift and compare it to the core (<0.1R500) X-ray radiative losses for clusters at $z$ < 1.},

  doi          = {10.1093/mnras/staa832},

  journal      = {Monthly Notices of the Royal Astronomical Society},

  number       = 2,

  volume       = 494,

  place        = {United Kingdom},

  year         = {Fri Apr 03 00:00:00 EDT 2020},

  month        = {Fri Apr 03 00:00:00 EDT 2020}

}

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Abstract

Citation Formats

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Extreme AGN feedback in the MAssive Cluster Survey: a detailed study of X-ray cavities at z>0.3 journal, February 2012

Radio jets in galaxies with actively accreting black holes: new insights from the SDSS journal, March 2008

A 10 10 SOLAR MASS FLOW OF MOLECULAR GAS IN THE A1835 BRIGHTEST CLUSTER GALAXY journal, March 2014

redMaPPer II: X-RAY AND SZ PERFORMANCE BENCHMARKS FOR THE SDSS CATALOG journal, February 2014

GALAXIES IN X-RAY SELECTED CLUSTERS AND GROUPS IN DARK ENERGY SURVEY DATA. I. STELLAR MASS GROWTH OF BRIGHT CENTRAL GALAXIES SINCE z ∼ 1.2 journal, January 2016

The Evolution of Radio Galaxies at Intermediate Redshift journal, May 2001

X-RAY CAVITIES IN A SAMPLE OF 83 SPT-SELECTED CLUSTERS OF GALAXIES: TRACING THE EVOLUTION OF AGN FEEDBACK IN CLUSTERS OF GALAXIES OUT TO z = 1.2 journal, May 2015

ON THE POPULATIONS OF RADIO GALAXIES WITH EXTENDED MORPHOLOGY AT z < 0.3 journal, October 2010

The evolution of optically selected QSOs – II journal, December 1988

Cosmic Evolution of Radio Selected Active Galactic Nuclei in the Cosmos Field journal, April 2009

Extreme active galactic nucleus feedback and cool-core destruction in the X-ray luminous galaxy cluster MACS J1931.8−2634: Extreme feedback in MACS J1931.8−2634 journal, November 2010

Simultaneous falsification of Λ CDM and quintessence with massive, distant clusters journal, January 2011

Detection of a Substantial Molecular Gas Reservoir in a Brightest Cluster Galaxy at z = 1.7 journal, July 2017

On the prevalence of radio-loud active galactic nuclei in brightest cluster galaxies: implications for AGN heating of cooling flows journal, August 2007

Linking macro-, meso- and microscales in multiphase AGN feeding and feedback journal, January 2020

A Relationship Between agn jet Power and Radio Power journal, August 2010

ALMA Observations of Molecular Clouds in Three Group-centered Elliptical Galaxies: NGC 5846, NGC 4636, and NGC 5044 journal, April 2018

Evidence for significant growth in the stellar mass of brightest cluster galaxies over the past 10 billion years: Brightest cluster galaxies journal, November 2012

GAMA/WiggleZ: the 1.4 GHz radio luminosity functions of high- and low-excitation radio galaxies and their redshift evolution to z = 0.75 journal, April 2016

Cooling Flows in Clusters of Galaxies journal, September 1994

The Dark Energy Survey Image Processing Pipeline journal, May 2018

High-Redshift Cool-Core Galaxy Clusters Detected via the Sunyaev-Zel'Dovich Effect in the South pole Telescope Survey journal, December 2012

Simulations of the Microwave sky journal, January 2010

Galaxy Populations in Massive Galaxy Clusters to $z$ = 1.1: Color Distribution, Concentration, Halo Occupation Number and Red Sequence Fraction journal, January 2017

Evidence for AGN Feedback in Galaxy Clusters and Groups journal, January 2012

SUMSS: A Wide-Field Radio Imaging Survey of the Southern Sky. I. Science Goals, Survey Design, and Instrumentation journal, March 1999

Weak-lensing analysis of SPT-selected galaxy clusters using Dark Energy Survey Science Verification data journal, January 2019

THE SLOAN DIGITAL SKY SURVEY COADD: 275 deg 2 OF DEEP SLOAN DIGITAL SKY SURVEY IMAGING ON STRIPE 82 journal, September 2014

The duty cycle of radio-mode feedback in complete samples of clusters journal, December 2012

The importance of major mergers in the build up of stellar mass in brightest cluster galaxies at z = 1 journal, June 2013

The Cosmic Evolution of Active Galactic Nuclei in Galaxy Clusters journal, March 2009

MAMPOSSt: Modelling Anisotropy and Mass Profiles of Observed Spherical Systems – I. Gaussian 3D velocities journal, January 2013

The Molonglo Observatory Synthesis Telescope journal, January 1981

A new RASS galaxy cluster catalogue with low contamination extending to z ∼ 1 in the DES overlap region journal, May 2019

AN ULTRA-DEEP NEAR-INFRARED SPECTRUM OF A COMPACT QUIESCENT GALAXY AT z = 2.2 journal, July 2009

Detection of the kinematic Sunyaev–Zel'dovich effect with DES Year 1 and SPT journal, June 2016

The Eighth data Release of the Sloan Digital sky Survey: First data from Sdss-Iii journal, March 2011

A multiwavelength photometric census of AGN and star formation activity in the brightest cluster galaxies of X-ray selected clusters journal, June 2016

The second epoch Molonglo Galactic Plane Survey: compact source catalogue journal, November 2007

K ‐band Properties of Galaxy Clusters and Groups: Brightest Cluster Galaxies and Intracluster Light journal, December 2004

Redshift evolution of the 1.4 GHz volume averaged radio luminosity function in clusters of galaxies journal, April 2011

Deep and narrow CO absorption revealing molecular clouds in the Hydra-A brightest cluster galaxy journal, February 2019

THE DEEP SWIRE FIELD. IV. FIRST PROPERTIES OF THE SUB-mJy GALAXY POPULATION: REDSHIFT DISTRIBUTION, AGN ACTIVITY, AND STAR FORMATION journal, April 2010

Parameter estimation in astronomy through application of the likelihood ratio journal, March 1979

First Results on the Cluster Galaxy Population from the Subaru Hyper Suprime-Cam Survey. III. Brightest Cluster Galaxies, Stellar Mass Distribution, and Active Galaxies journal, December 2017

How special are brightest group and cluster galaxies? journal, July 2007

SUMSS: a wide-field radio imaging survey of the southern sky - II. The source catalogue journal, July 2003

Central galaxy growth and feedback in the most massive nearby cool core cluster: The cool-core of RXCJ1504.1-0248 journal, June 2010

Molecular gas in the X-Ray Bright Group ngc 5044 as Revealed by alma journal, August 2014

A massive, cooling-flow-induced starburst in the core of a luminous cluster of galaxies journal, August 2012

Properties of the Intracluster Medium in an Ensemble of Nearby Galaxy Clusters journal, June 1999

The prevalence of AGN feedback in massive galaxies at z ≈ 1 journal, June 2013

Stellar population synthesis at the resolution of 2003 journal, October 2003

Active galactic nucleus feedback in clusters of galaxies journal, March 2010

On the fundamental dichotomy in the local radio-AGN population: accretion, evolution and host galaxy properties journal, February 2012

X-Ray Properties of AGN in Brightest Cluster Galaxies. I. A Systematic Study of the Chandra Archive in the 0.2 < z < 0.3 and 0.55 < z < 0.75 Redshift Range journal, May 2018

The triggering probability of radio-loud AGN: A comparison of high and low excitation radio galaxies in hosts of different colors journal, April 2012

A volume-limited sample of X-ray galaxy groups and clusters – I. Radial entropy and cooling time profiles journal, December 2013

Galaxy kinematics and mass calibration in massive SZE-selected galaxy clusters to z = 1.3 journal, October 2018

Mass calibration of the CODEX cluster sample using SPIDERS spectroscopy – I. The richness–mass relation journal, March 2019

THE GROWTH OF COOL CORES AND EVOLUTION OF COOLING PROPERTIES IN A SAMPLE OF 83 GALAXY CLUSTERS AT 0.3 < z < 1.2 SELECTED FROM THE SPT-SZ SURVEY journal, August 2013

The heating of gas in a galaxy cluster by X-ray cavities and large-scale shock fronts journal, January 2005

Coevolution of brightest cluster galaxies and intracluster light using CLASH journal, March 2015

SExtractor: Software for source extraction journal, June 1996

Second ROSAT all-sky survey (2RXS) source catalogue journal, March 2016

A Universal Density Profile from Hierarchical Clustering journal, December 1997

A relationship between halo mass, cooling, active galactic nuclei heating and the co-evolution of massive black holes journal, October 2016

Baryon content in a sample of 91 galaxy clusters selected by the South Pole Telescope at 0.2 <z < 1.25 journal, May 2018

K ‐Band Properties of Galaxy Clusters and Groups: Luminosity Function, Radial Distribution, and Halo Occupation Number journal, August 2004

Spectral Energy Distribution of Radio Sources in Nearby Clusters of Galaxies: Implications for Sunyaev-Zel'Dovich Effect Surveys journal, March 2009

Cold, clumpy accretion onto an active supermassive black hole journal, June 2016

redMaPPer. I. ALGORITHM AND SDSS DR8 CATALOG journal, April 2014

A study of high-redshift AGN feedback in SZ cluster samples journal, June 2017

The detection of molecular gas in the central galaxies of cooling flow clusters journal, December 2001

Cluster Cosmology Constraints from the 2500 deg 2 SPT-SZ Survey: Inclusion of Weak Gravitational Lensing Data from Magellan and the Hubble Space Telescope journal, June 2019

X-Ray Properties of SPT-selected Galaxy Clusters at 0.2 < z < 1.5 Observed with XMM-Newton journal, January 2019

Intracluster medium cooling, AGN feedback, and brightest cluster galaxy properties of galaxy groups: Five properties where groups differ from clusters
journal, November 2014

Extreme AGN feedback in the MAssive Cluster Survey: a detailed study of X-ray cavities at z>0.3
journal, February 2012

Radio jets in galaxies with actively accreting black holes: new insights from the SDSS
journal, March 2008

A 10 ¹⁰ SOLAR MASS FLOW OF MOLECULAR GAS IN THE A1835 BRIGHTEST CLUSTER GALAXY
journal, March 2014

redMaPPer II: X-RAY AND SZ PERFORMANCE BENCHMARKS FOR THE SDSS CATALOG
journal, February 2014

GALAXIES IN X-RAY SELECTED CLUSTERS AND GROUPS IN DARK ENERGY SURVEY DATA. I. STELLAR MASS GROWTH OF BRIGHT CENTRAL GALAXIES SINCE z ∼ 1.2
journal, January 2016

The Evolution of Radio Galaxies at Intermediate Redshift
journal, May 2001

X-RAY CAVITIES IN A SAMPLE OF 83 SPT-SELECTED CLUSTERS OF GALAXIES: TRACING THE EVOLUTION OF AGN FEEDBACK IN CLUSTERS OF GALAXIES OUT TO z = 1.2
journal, May 2015

ON THE POPULATIONS OF RADIO GALAXIES WITH EXTENDED MORPHOLOGY AT z < 0.3
journal, October 2010

The evolution of optically selected QSOs – II
journal, December 1988

Cosmic Evolution of Radio Selected Active Galactic Nuclei in the Cosmos Field
journal, April 2009

Extreme active galactic nucleus feedback and cool-core destruction in the X-ray luminous galaxy cluster MACS J1931.8−2634: Extreme feedback in MACS J1931.8−2634
journal, November 2010

Simultaneous falsification of $Λ CDM$ and quintessence with massive, distant clusters
journal, January 2011

Detection of a Substantial Molecular Gas Reservoir in a Brightest Cluster Galaxy at z = 1.7
journal, July 2017

On the prevalence of radio-loud active galactic nuclei in brightest cluster galaxies: implications for AGN heating of cooling flows
journal, August 2007

Linking macro-, meso- and microscales in multiphase AGN feeding and feedback
journal, January 2020

A Relationship Between agn jet Power and Radio Power
journal, August 2010

ALMA Observations of Molecular Clouds in Three Group-centered Elliptical Galaxies: NGC 5846, NGC 4636, and NGC 5044
journal, April 2018

Evidence for significant growth in the stellar mass of brightest cluster galaxies over the past 10 billion years: Brightest cluster galaxies
journal, November 2012

GAMA/WiggleZ: the 1.4 GHz radio luminosity functions of high- and low-excitation radio galaxies and their redshift evolution to z = 0.75
journal, April 2016

Cooling Flows in Clusters of Galaxies
journal, September 1994

The Dark Energy Survey Image Processing Pipeline
journal, May 2018

High-Redshift Cool-Core Galaxy Clusters Detected via the Sunyaev-Zel'Dovich Effect in the South pole Telescope Survey
journal, December 2012

Simulations of the Microwave sky
journal, January 2010

Galaxy Populations in Massive Galaxy Clusters to $z$ = 1.1: Color Distribution, Concentration, Halo Occupation Number and Red Sequence Fraction
journal, January 2017

Evidence for AGN Feedback in Galaxy Clusters and Groups
journal, January 2012

SUMSS: A Wide-Field Radio Imaging Survey of the Southern Sky. I. Science Goals, Survey Design, and Instrumentation
journal, March 1999

Weak-lensing analysis of SPT-selected galaxy clusters using Dark Energy Survey Science Verification data
journal, January 2019

THE SLOAN DIGITAL SKY SURVEY COADD: 275 deg ² OF DEEP SLOAN DIGITAL SKY SURVEY IMAGING ON STRIPE 82
journal, September 2014

The duty cycle of radio-mode feedback in complete samples of clusters
journal, December 2012

The importance of major mergers in the build up of stellar mass in brightest cluster galaxies at z = 1
journal, June 2013

The Cosmic Evolution of Active Galactic Nuclei in Galaxy Clusters
journal, March 2009

MAMPOSSt: Modelling Anisotropy and Mass Profiles of Observed Spherical Systems – I. Gaussian 3D velocities
journal, January 2013

The Molonglo Observatory Synthesis Telescope
journal, January 1981

A new RASS galaxy cluster catalogue with low contamination extending to z ∼ 1 in the DES overlap region
journal, May 2019

AN ULTRA-DEEP NEAR-INFRARED SPECTRUM OF A COMPACT QUIESCENT GALAXY AT z = 2.2
journal, July 2009

Detection of the kinematic Sunyaev–Zel'dovich effect with DES Year 1 and SPT
journal, June 2016

The Eighth data Release of the Sloan Digital sky Survey: First data from Sdss-Iii
journal, March 2011

A multiwavelength photometric census of AGN and star formation activity in the brightest cluster galaxies of X-ray selected clusters
journal, June 2016

The second epoch Molonglo Galactic Plane Survey: compact source catalogue
journal, November 2007

K ‐band Properties of Galaxy Clusters and Groups: Brightest Cluster Galaxies and Intracluster Light
journal, December 2004

Redshift evolution of the 1.4 GHz volume averaged radio luminosity function in clusters of galaxies
journal, April 2011

Deep and narrow CO absorption revealing molecular clouds in the Hydra-A brightest cluster galaxy
journal, February 2019

THE DEEP SWIRE FIELD. IV. FIRST PROPERTIES OF THE SUB-mJy GALAXY POPULATION: REDSHIFT DISTRIBUTION, AGN ACTIVITY, AND STAR FORMATION
journal, April 2010

Parameter estimation in astronomy through application of the likelihood ratio
journal, March 1979

First Results on the Cluster Galaxy Population from the Subaru Hyper Suprime-Cam Survey. III. Brightest Cluster Galaxies, Stellar Mass Distribution, and Active Galaxies
journal, December 2017

How special are brightest group and cluster galaxies?
journal, July 2007

SUMSS: a wide-field radio imaging survey of the southern sky - II. The source catalogue
journal, July 2003

Central galaxy growth and feedback in the most massive nearby cool core cluster: The cool-core of RXCJ1504.1-0248
journal, June 2010

Molecular gas in the X-Ray Bright Group ngc 5044 as Revealed by alma
journal, August 2014

A massive, cooling-flow-induced starburst in the core of a luminous cluster of galaxies
journal, August 2012

Properties of the Intracluster Medium in an Ensemble of Nearby Galaxy Clusters
journal, June 1999

The prevalence of AGN feedback in massive galaxies at z ≈ 1
journal, June 2013

Stellar population synthesis at the resolution of 2003
journal, October 2003

Active galactic nucleus feedback in clusters of galaxies
journal, March 2010

On the fundamental dichotomy in the local radio-AGN population: accretion, evolution and host galaxy properties
journal, February 2012

X-Ray Properties of AGN in Brightest Cluster Galaxies. I. A Systematic Study of the Chandra Archive in the 0.2 < z < 0.3 and 0.55 < z < 0.75 Redshift Range
journal, May 2018

The triggering probability of radio-loud AGN: A comparison of high and low excitation radio galaxies in hosts of different colors
journal, April 2012

A volume-limited sample of X-ray galaxy groups and clusters – I. Radial entropy and cooling time profiles
journal, December 2013

Galaxy kinematics and mass calibration in massive SZE-selected galaxy clusters to z = 1.3
journal, October 2018

Mass calibration of the CODEX cluster sample using SPIDERS spectroscopy – I. The richness–mass relation
journal, March 2019

THE GROWTH OF COOL CORES AND EVOLUTION OF COOLING PROPERTIES IN A SAMPLE OF 83 GALAXY CLUSTERS AT 0.3 < z < 1.2 SELECTED FROM THE SPT-SZ SURVEY
journal, August 2013

The heating of gas in a galaxy cluster by X-ray cavities and large-scale shock fronts
journal, January 2005

Coevolution of brightest cluster galaxies and intracluster light using CLASH
journal, March 2015

SExtractor: Software for source extraction
journal, June 1996

Second ROSAT all-sky survey (2RXS) source catalogue
journal, March 2016

A Universal Density Profile from Hierarchical Clustering
journal, December 1997

A relationship between halo mass, cooling, active galactic nuclei heating and the co-evolution of massive black holes
journal, October 2016

Baryon content in a sample of 91 galaxy clusters selected by the South Pole Telescope at 0.2 <z < 1.25
journal, May 2018

K ‐Band Properties of Galaxy Clusters and Groups: Luminosity Function, Radial Distribution, and Halo Occupation Number
journal, August 2004

Spectral Energy Distribution of Radio Sources in Nearby Clusters of Galaxies: Implications for Sunyaev-Zel'Dovich Effect Surveys
journal, March 2009

Cold, clumpy accretion onto an active supermassive black hole
journal, June 2016

redMaPPer. I. ALGORITHM AND SDSS DR8 CATALOG
journal, April 2014

A study of high-redshift AGN feedback in SZ cluster samples
journal, June 2017

The detection of molecular gas in the central galaxies of cooling flow clusters
journal, December 2001

Cluster Cosmology Constraints from the 2500 deg ² SPT-SZ Survey: Inclusion of Weak Gravitational Lensing Data from Magellan and the Hubble Space Telescope
journal, June 2019

X-Ray Properties of SPT-selected Galaxy Clusters at 0.2 < z < 1.5 Observed with XMM-Newton
journal, January 2019

`emcee` : The MCMC Hammer
journal, March 2013

The rapid evolution of AGN feedback in brightest cluster galaxies: switching from quasar-mode to radio-mode feedback
journal, March 2013

The VLA-COSMOS 3 GHz Large Project: Cosmic evolution of radio AGN and implications for radio-mode feedback since z ~ 5
journal, June 2017