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

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

doi:10.1093/MNRAS/STAA832

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

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

^*Corresponding author for this work

Research output: Contribution to journal › Article › peer-review

7 Citations (Scopus)

Abstract

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 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.

Original language	English
Pages (from-to)	1705-1723
Number of pages	19
Journal	Monthly Notices of the Royal Astronomical Society
Volume	494
Issue number	2
DOIs	https://doi.org/10.1093/MNRAS/STAA832
Publication status	Published - 2020

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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., ... Zenteno, A. (2020). Constraining radio mode feedback in galaxy clusters with the cluster radio AGNs properties to z ∼ 1. Monthly Notices of the Royal Astronomical Society, 494(2), 1705-1723. https://doi.org/10.1093/MNRAS/STAA832

@article{74a9599ffa114778bc3383afc04abb7f,

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

abstract = "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 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.",

keywords = "Cosmology: Observations, Galaxies: Active, Galaxies: Clusters: General, Galaxies: Luminosity function, mass function, Submillimeter: Galaxies",

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

year = "2020",

doi = "10.1093/MNRAS/STAA832",

language = "English",

volume = "494",

pages = "1705--1723",

journal = "Monthly Notices of the Royal Astronomical Society",

issn = "0035-8711",

publisher = "Oxford University Press",

number = "2",

}

Gupta, N, Pannella, M, Mohr, JJ, Klein, M, Rykoff, ES, 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, LN, De Vicente, J, Desai, S, Dietrich, JP, Doel, P, Everett, S, Evrard, AE, Garcia-Bellido, J, Gaztanaga, E, Gruen, D, Gruendl, RA, Gschwend, J, Gutierrez, G, Hollowood, DL, Honscheid, K, James, DJ, Jeltema, T, Kuehn, K, Lidman, C, Lima, M, Maia, MAG, Marshall, JL, McDonald, M, Menanteau, F, Miquel, R, Ogando, RLC, Palmese, A, Paz-Chinchon, F, Plazas, AA, Reichardt, CL, Sanchez, E, Santiago, B, Saro, A, Scarpine, V, Schindler, R, Schubnell, M, Serrano, S, Sevilla-Noarbe, I, Shao, X, Smith, M, Stott, JP, Strazzullo, V, Suchyta, E, Swanson, MEC, Vikram, V & Zenteno, A 2020, 'Constraining radio mode feedback in galaxy clusters with the cluster radio AGNs properties to z ∼ 1', Monthly Notices of the Royal Astronomical Society, vol. 494, no. 2, pp. 1705-1723. https://doi.org/10.1093/MNRAS/STAA832

TY - JOUR

T1 - Constraining radio mode feedback in galaxy clusters with the cluster radio AGNs properties to z ∼ 1

AU - Gupta, N.

AU - Pannella, M.

AU - Mohr, J. J.

AU - Klein, M.

AU - Rykoff, E. S.

AU - Annis, J.

AU - Avila, S.

AU - Bianchini, F.

AU - Brooks, D.

AU - Buckley-Geer, E.

AU - Bulbul, E.

AU - Carnero Rosell, A.

AU - Carrasco Kind, M.

AU - Carretero, J.

AU - Chiu, I.

AU - Costanzi, M.

AU - da Costa, L. N.

AU - De Vicente, J.

AU - Desai, S.

AU - Dietrich, J. P.

AU - Doel, P.

AU - Everett, S.

AU - Evrard, A. E.

AU - Garcia-Bellido, J.

AU - Gaztanaga, E.

AU - Gruen, D.

AU - Gruendl, R. A.

AU - Gschwend, J.

AU - Gutierrez, G.

AU - Hollowood, D. L.

AU - Honscheid, K.

AU - James, D. J.

AU - Jeltema, T.

AU - Kuehn, K.

AU - Lidman, C.

AU - Lima, M.

AU - Maia, M. A.G.

AU - Marshall, J. L.

AU - McDonald, M.

AU - Menanteau, F.

AU - Miquel, R.

AU - Ogando, R. L.C.

AU - Palmese, A.

AU - Paz-Chinchon, F.

AU - Plazas, A. A.

AU - Reichardt, C. L.

AU - Sanchez, E.

AU - Santiago, B.

AU - Saro, A.

AU - Scarpine, V.

AU - Schindler, R.

AU - Schubnell, M.

AU - Serrano, S.

AU - Sevilla-Noarbe, I.

AU - Shao, X.

AU - Smith, M.

AU - Stott, J. P.

AU - Strazzullo, V.

AU - Suchyta, E.

AU - Swanson, M. E.C.

AU - Vikram, V.

AU - Zenteno, A.

PY - 2020

Y1 - 2020

N2 - 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 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.

AB - 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 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.

KW - Cosmology: Observations

KW - Galaxies: Active

KW - Galaxies: Clusters: General

KW - Galaxies: Luminosity function, mass function

KW - Submillimeter: Galaxies

UR - http://www.scopus.com/inward/record.url?scp=85095504615&partnerID=8YFLogxK

U2 - 10.1093/MNRAS/STAA832

DO - 10.1093/MNRAS/STAA832

M3 - Article

SN - 0035-8711

VL - 494

SP - 1705

EP - 1723

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

IS - 2

ER -

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

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