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

Journal Article · 03 April 2020 · Monthly Notices of the Royal Astronomical Society

DOI: https://doi.org/10.1093/mnras/staa832 · OSTI ID:1616204

Gupta, N.  ^[1]; Pannella, M. ^[2]; Mohr, J. J. ^[3]; Klein, M. ^[4]; Rykoff, E. S. ^[5]; Annis, J. ^[6]; Avila, S.  ^[7]; Bianchini, F. ^[8]; Brooks, D. ^[9]; Buckley-Geer, E.  ^[6]; Bulbul, E. ^[10]; Carnero Rosell, A.  ^[11]; Carrasco Kind, M.  ^[12]; Carretero, J. ^[13]; Chiu, I.  ^[14]; Costanzi, M. ^[2]; da Costa, L. N. ^[15]; De Vicente, J.  ^[7]; Desai, S. ^[16]; Dietrich, J. P. ^[17] ; Doel, P. ^[9]; Everett, S. ^[18]; Evrard, A. E.  ^[19]; García-Bellido, J. ^[7]; Gaztanaga, E.  ^[20]; Gruen, D.  ^[21]; Gruendl, R. A. ^[12]; Gschwend, J. ^[15]; Gutierrez, G. ^[6]; Hollowood, D. L. ^[18]; Honscheid, K. ^[22]; James, D. J. ^[23]; Jeltema, T. ^[18]; Kuehn, K. ^[24]; Lidman, C.  ^[25]; Lima, M. ^[26]; Maia, M. G. ^[15]; Marshall, J. L. ^[27]; McDonald, M. ^[28]; Menanteau, F. ^[12]; Miquel, R. ^[29]; Ogando, R. C. ^[15]; Palmese, A.  ^[6]; Paz-Chinchón, F. ^[12]; Plazas, A. A.  ^[30]; Reichardt, C. L.  ^[8]; Sanchez, E. ^[7]; Santiago, B. ^[31]; Saro, A. ^[32]; Scarpine, V. ^[6]; Schindler, R. ^[33]; Schubnell, M. ^[34]; Serrano, S. ^[20]; Sevilla-Noarbe, I. ^[7]; Shao, X. ^[2]; Smith, M.  ^[35]; Stott, J. P. ^[36]; Strazzullo, V. ^[2]; Suchyta, E.  ^[37]; Swanson, M. C. ^[38]; Vikram, V. ^[39]; Zenteno, A. ^[40]

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1. 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
2. Faculty of Physics, Ludwig-Maximilians-Universität, Scheinerstr 1, D-81679 Munich, Germany
3. 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
4. Faculty of Physics, Ludwig-Maximilians-Universität, Scheinerstr 1, D-81679 Munich, Germany;Max Planck Institute for Extraterrestrial Physics, Giessenbachstr, D-85748 Garching, Germany
5. 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
6. Fermi National Accelerator Laboratory, P. O. Box 500, Batavia, IL 60510, USA
7. Instituto de Fisica Teorica UAM/CSIC, Universidad Autonoma de Madrid, E-28049 Madrid, Spain
8. School of Physics, University of Melbourne, Parkville, VIC 3010, Australia
9. Department of Physics & Astronomy, University College London, Gower Street, London WC1E 6BT, UK
10. 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
11. 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
12. 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
13. Institut de Física d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology, Campus UAB, E-08193 Bellaterra, Barcelona, Spain
14. Academia Sinica Institute of Astronomy and Astrophysics, 11F of AS/NTU Astronomy-Mathematics Building, No.1, Section 4, Roosevelt Rd, Taipei 10617, Taiwan
15. 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
16. Department of Physics, IIT Hyderabad, Kandi, Telangana 502285, India
17. Faculty of Physics, Ludwig-Maximilians-Universität, Scheinerstr 1, D-81679 Munich, Germany;Excellence Cluster Origins, Boltzmannstr 2, D-85748 Garching, Germany
18. Santa Cruz Institute for Particle Physics, Santa Cruz, CA 95064, USA
19. Department of Astronomy, University of Michigan, Ann Arbor, MI 48109, USA;Department of Physics, University of Michigan, Ann Arbor, MI 48109, USA
20. 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
21. 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
22. Department of Physics, The Ohio State University, Columbus, OH 43210, USA
23. Center for Astrophysics Harvard & Smithsonian, 60 Garden Street, Cambridge, MA 02138, USA
24. Australian Astronomical Optics, Macquarie University, North Ryde, NSW 2113, Australia
25. The Research School of Astronomy and Astrophysics, Australian National University, ACT 2601, Australia
26. 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
27. 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
28. Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, 77 Massachusetts Avenue, Cambridge, MA 02139, USA
29. 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
30. Department of Astrophysical Sciences, Princeton University, Peyton Hall, Princeton, NJ 08544, USA
31. 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
32. 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
33. SLAC National Accelerator Laboratory, Menlo Park, CA 94025, USA
34. Department of Physics, University of Michigan, Ann Arbor, MI 48109, USA
35. School of Physics and Astronomy, University of Southampton, Southampton SO17 1BJ, UK
36. Department of Physics, Lancaster University, Lancaster LA1 4YB, UK
37. Computer Science and Mathematics Division, Oak Ridge National Laboratory, Oak Ridge, TN 37831, USA
38. National Center for Supercomputing Applications, 1205 West Clark St., Urbana, IL 61801, USA
39. Argonne National Laboratory, 9700 South Cass Avenue, Lemont, IL 60439, USA
40. Cerro Tololo Inter-American Observatory, Casilla 603, La Serena, Chile

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 γ_D = 3.0 ± 0.4 and γ_P = 0.21 ± 0.15 in the RM-Y3 sample, and γ_D = 2.6 ± 0.7 and γ_P = 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.

• Research Organization: Oak Ridge National Laboratory (ORNL), Oak Ridge, TN (United States); SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States); Fermi National Accelerator Laboratory (FNAL), Batavia, IL (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 Organization: USDOE Office of Science (SC), Advanced Scientific Computing Research (ASCR); USDOE Office of Science (SC), High Energy Physics (HEP)
• Contributing Organization: DES Collaboration
• Grant/Contract Number: AC05-00OR22725; AC02-07CH11359; AC02-05CH11231; 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; AC02-06CH11357; SC0019193
• OSTI ID: 1616204
• Alternate ID(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 Information: Monthly Notices of the Royal Astronomical Society, Vol. 494, Issue 2; ISSN 0035-8711
• Publisher: Royal Astronomical SocietyCopyright Statement
• Country of Publication: United States
• Language: English