Planck early results. XI: Calibration of the local galaxy cluster Sunyaev-Zeldovich scaling relations

P. A.R. Ade; N. Aghanim; M. Arnaud; M. Ashdown; J. Aumont; C. Baccigalupi; A. Balbi; A. J. Banday; R. B. Barreiro; M. Bartelmann; J. G. Bartlett; E. Battaner; K. Benabed; A. Benoît; J. P. Bernard; M. Bersanelli; R. Bhatia; J. J. Bock; A. Bonaldi; J. R. Bond; J. Borrill; F. R. Bouchet; H. Bourdin; M. L. Brown; M. Bucher; C. Burigana; P. Cabella; J. F. Cardoso; A. Catalano; L. Cayón; A. Challinor; A. Chamballu; L. Y. Chiang; C. Chiang; G. Chon; P. R. Christensen; E. Churazov; D. L. Clements; S. Colafrancesco; S. Colombi; F. Couchot; A. Coulais; B. P. Crill; F. Cuttaia; A. Da Silva; H. Dahle; L. Danese; P. De Bernardis; G. De Gasperis; A. De Rosa; Planck Collaboration

doi:10.1051/0004-6361/201116458

Planck early results. XI: Calibration of the local galaxy cluster Sunyaev-Zeldovich scaling relations

P. A.R. Ade
, N. Aghanim
, M. Arnaud
, M. Ashdown
, J. Aumont
, C. Baccigalupi
, A. Balbi
, A. J. Banday
, R. B. Barreiro
, M. Bartelmann
, J. G. Bartlett
, E. Battaner
, K. Benabed
, A. Benoît
, J. P. Bernard
, M. Bersanelli
, R. Bhatia
, J. J. Bock
, A. Bonaldi
, J. R. Bond

J. Borrill, F. R. Bouchet, H. Bourdin, M. L. Brown, M. Bucher, C. Burigana, P. Cabella, J. F. Cardoso, A. Catalano, L. Cayón, A. Challinor, A. Chamballu, L. Y. Chiang, C. Chiang, G. Chon, P. R. Christensen, E. Churazov, D. L. Clements, S. Colafrancesco, S. Colombi, F. Couchot, A. Coulais, B. P. Crill, F. Cuttaia, A. Da Silva, H. Dahle, L. Danese, P. De Bernardis, G. De Gasperis, A. De Rosa, Planck Collaboration

VTT Technical Research Centre of Finland

Cardiff University
PSL Research University
Paris Diderot University
University of Cambridge
Scuola Internazionale Superiore di Studi Avanzati (SISSA)
University of Rome Tor Vergata
French National Center for Scientific Research (CNRS)
Max Planck Society
Université de Toulouse
Spanish National Research Council (CSIC)
Heidelberg University
California Institute of Technology
University of Granada
University of Milan
National Institute for Astrophysics (INAF)
ALMA Santiago Central Offices
Astronomical Observatory of Padua
University of Toronto
Lawrence Berkeley National Laboratory (LBNL)
University of California System
Purdue University West Lafayette
Imperial College London
Institute of Astrophysics and Astronomy, Academia Sinica
Princeton University
Max Planck Institute for Extraterrestrial Physics
University of Copenhagen
Space Research Institute of the Russian Academy of Sciences
Osservatorio Astronomico Roma
Universidade do Porto
University of Oslo
Sapienza University of Rome

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

66 Citations (Scopus)

Abstract

We present precise Sunyaev-Zeldovich (SZ) effect measurements in the direction of 62 nearby galaxy clusters (z < 0.5) detected at high signal-to-noise in the first Planck all-sky data set. The sample spans approximately a decade in total mass, 2 × 10¹⁴ M < M ₅₀₀ < 2 × 10¹⁵ M, where M₅₀₀ is the mass corresponding to a total density contrast of 500. Combining these high quality Planck measurements with deep XMM-Newton X-ray data, we investigate the relations between D_A ² Y₅₀₀, the integrated Compton parameter due to the SZ effect, and the X-ray-derived gas mass M _g,500, temperature T_X, luminosity L_X,500, SZ signal analogue Y_X,500 = M_g,500 × T_X, and total mass M₅₀₀. After correction for the effect of selection bias on the scaling relations, we find results that are in excellent agreement with both X-ray predictions and recently-published ground-based data derived from smaller samples. The present data yield an exceptionally robust, high-quality local reference, and illustrate Planck's unique capabilities for all-sky statistical studies of galaxy clusters.

Original language	English
Article number	A11
Number of pages	14
Journal	Astronomy and Astrophysics
Volume	536
DOIs	https://doi.org/10.1051/0004-6361/201116458
Publication status	Published - 12 Dec 2011
MoE publication type	Not Eligible

Keywords

clusters
Cosmology
Galaxies
galaxies
interacluster medium
observations
X-rays

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10.1051/0004-6361/201116458

Cite this

Ade, P. A. R., Aghanim, N., Arnaud, M., Ashdown, M., Aumont, J., Baccigalupi, C., Balbi, A., Banday, A. J., Barreiro, R. B., Bartelmann, M., Bartlett, J. G., Battaner, E., Benabed, K., Benoît, A., Bernard, J. P., Bersanelli, M., Bhatia, R., Bock, J. J., Bonaldi, A., ... Planck Collaboration (2011). Planck early results. XI: Calibration of the local galaxy cluster Sunyaev-Zeldovich scaling relations. Astronomy and Astrophysics, 536, Article A11. https://doi.org/10.1051/0004-6361/201116458

@article{4bbec024a0c44603a764fe7d1e720a41,

title = "Planck early results. XI: Calibration of the local galaxy cluster Sunyaev-Zeldovich scaling relations",

abstract = "We present precise Sunyaev-Zeldovich (SZ) effect measurements in the direction of 62 nearby galaxy clusters (z < 0.5) detected at high signal-to-noise in the first Planck all-sky data set. The sample spans approximately a decade in total mass, 2 × 1014 M < M 500 < 2 × 1015 M, where M500 is the mass corresponding to a total density contrast of 500. Combining these high quality Planck measurements with deep XMM-Newton X-ray data, we investigate the relations between DA 2 Y500, the integrated Compton parameter due to the SZ effect, and the X-ray-derived gas mass M g,500, temperature TX, luminosity LX,500, SZ signal analogue YX,500 = Mg,500 × TX, and total mass M500. After correction for the effect of selection bias on the scaling relations, we find results that are in excellent agreement with both X-ray predictions and recently-published ground-based data derived from smaller samples. The present data yield an exceptionally robust, high-quality local reference, and illustrate Planck's unique capabilities for all-sky statistical studies of galaxy clusters.",

keywords = "clusters, Cosmology, Galaxies, galaxies, interacluster medium, observations, X-rays",

author = "Ade, \{P. A.R.\} and N. Aghanim and M. Arnaud and M. Ashdown and J. Aumont and C. Baccigalupi and A. Balbi and Banday, \{A. J.\} and Barreiro, \{R. B.\} and M. Bartelmann and Bartlett, \{J. G.\} and E. Battaner and K. Benabed and A. Beno{\^i}t and Bernard, \{J. P.\} and M. Bersanelli and R. Bhatia and Bock, \{J. J.\} and A. Bonaldi and Bond, \{J. R.\} and J. Borrill and Bouchet, \{F. R.\} and H. Bourdin and Brown, \{M. L.\} and M. Bucher and C. Burigana and P. Cabella and Cardoso, \{J. F.\} and A. Catalano and L. Cay{\'o}n and A. Challinor and A. Chamballu and Chiang, \{L. Y.\} and C. Chiang and G. Chon and Christensen, \{P. R.\} and E. Churazov and Clements, \{D. L.\} and S. Colafrancesco and S. Colombi and F. Couchot and A. Coulais and Crill, \{B. P.\} and F. Cuttaia and \{Da Silva\}, A. and H. Dahle and L. Danese and \{De Bernardis\}, P. and \{De Gasperis\}, G. and \{De Rosa\}, A. and \{Planck Collaboration\}",

note = "Project code: 18080",

year = "2011",

month = dec,

day = "12",

doi = "10.1051/0004-6361/201116458",

language = "English",

volume = "536",

journal = "Astronomy and Astrophysics",

issn = "0004-6361",

}

Ade, PAR, Aghanim, N, Arnaud, M, Ashdown, M, Aumont, J, Baccigalupi, C, Balbi, A, Banday, AJ, Barreiro, RB, Bartelmann, M, Bartlett, JG, Battaner, E, Benabed, K, Benoît, A, Bernard, JP, Bersanelli, M, Bhatia, R, Bock, JJ, Bonaldi, A, Bond, JR, Borrill, J, Bouchet, FR, Bourdin, H, Brown, ML, Bucher, M, Burigana, C, Cabella, P, Cardoso, JF, Catalano, A, Cayón, L, Challinor, A, Chamballu, A, Chiang, LY, Chiang, C, Chon, G, Christensen, PR, Churazov, E, Clements, DL, Colafrancesco, S, Colombi, S, Couchot, F, Coulais, A, Crill, BP, Cuttaia, F, Da Silva, A, Dahle, H, Danese, L, De Bernardis, P, De Gasperis, G, De Rosa, A & Planck Collaboration 2011, 'Planck early results. XI: Calibration of the local galaxy cluster Sunyaev-Zeldovich scaling relations', Astronomy and Astrophysics, vol. 536, A11. https://doi.org/10.1051/0004-6361/201116458

TY - JOUR

T1 - Planck early results. XI

T2 - Calibration of the local galaxy cluster Sunyaev-Zeldovich scaling relations

AU - Ade, P. A.R.

AU - Aghanim, N.

AU - Arnaud, M.

AU - Ashdown, M.

AU - Aumont, J.

AU - Baccigalupi, C.

AU - Balbi, A.

AU - Banday, A. J.

AU - Barreiro, R. B.

AU - Bartelmann, M.

AU - Bartlett, J. G.

AU - Battaner, E.

AU - Benabed, K.

AU - Benoît, A.

AU - Bernard, J. P.

AU - Bersanelli, M.

AU - Bhatia, R.

AU - Bock, J. J.

AU - Bonaldi, A.

AU - Bond, J. R.

AU - Borrill, J.

AU - Bouchet, F. R.

AU - Bourdin, H.

AU - Brown, M. L.

AU - Bucher, M.

AU - Burigana, C.

AU - Cabella, P.

AU - Cardoso, J. F.

AU - Catalano, A.

AU - Cayón, L.

AU - Challinor, A.

AU - Chamballu, A.

AU - Chiang, L. Y.

AU - Chiang, C.

AU - Chon, G.

AU - Christensen, P. R.

AU - Churazov, E.

AU - Clements, D. L.

AU - Colafrancesco, S.

AU - Colombi, S.

AU - Couchot, F.

AU - Coulais, A.

AU - Crill, B. P.

AU - Cuttaia, F.

AU - Da Silva, A.

AU - Dahle, H.

AU - Danese, L.

AU - De Bernardis, P.

AU - De Gasperis, G.

AU - De Rosa, A.

AU - Planck Collaboration

N1 - Project code: 18080

PY - 2011/12/12

Y1 - 2011/12/12

N2 - We present precise Sunyaev-Zeldovich (SZ) effect measurements in the direction of 62 nearby galaxy clusters (z < 0.5) detected at high signal-to-noise in the first Planck all-sky data set. The sample spans approximately a decade in total mass, 2 × 1014 M < M 500 < 2 × 1015 M, where M500 is the mass corresponding to a total density contrast of 500. Combining these high quality Planck measurements with deep XMM-Newton X-ray data, we investigate the relations between DA 2 Y500, the integrated Compton parameter due to the SZ effect, and the X-ray-derived gas mass M g,500, temperature TX, luminosity LX,500, SZ signal analogue YX,500 = Mg,500 × TX, and total mass M500. After correction for the effect of selection bias on the scaling relations, we find results that are in excellent agreement with both X-ray predictions and recently-published ground-based data derived from smaller samples. The present data yield an exceptionally robust, high-quality local reference, and illustrate Planck's unique capabilities for all-sky statistical studies of galaxy clusters.

AB - We present precise Sunyaev-Zeldovich (SZ) effect measurements in the direction of 62 nearby galaxy clusters (z < 0.5) detected at high signal-to-noise in the first Planck all-sky data set. The sample spans approximately a decade in total mass, 2 × 1014 M < M 500 < 2 × 1015 M, where M500 is the mass corresponding to a total density contrast of 500. Combining these high quality Planck measurements with deep XMM-Newton X-ray data, we investigate the relations between DA 2 Y500, the integrated Compton parameter due to the SZ effect, and the X-ray-derived gas mass M g,500, temperature TX, luminosity LX,500, SZ signal analogue YX,500 = Mg,500 × TX, and total mass M500. After correction for the effect of selection bias on the scaling relations, we find results that are in excellent agreement with both X-ray predictions and recently-published ground-based data derived from smaller samples. The present data yield an exceptionally robust, high-quality local reference, and illustrate Planck's unique capabilities for all-sky statistical studies of galaxy clusters.

KW - clusters

KW - Cosmology

KW - Galaxies

KW - galaxies

KW - interacluster medium

KW - observations

KW - X-rays

U2 - 10.1051/0004-6361/201116458

DO - 10.1051/0004-6361/201116458

M3 - Article

AN - SCOPUS:82955188053

SN - 0004-6361

VL - 536

JO - Astronomy and Astrophysics

JF - Astronomy and Astrophysics

M1 - A11

ER -

Planck early results. XI: Calibration of the local galaxy cluster Sunyaev-Zeldovich scaling relations

Abstract

Keywords

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