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. BondJ. 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

Research output: Contribution to journalArticleScientificpeer-review

53 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 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.

Original languageEnglish
Article numberA11
Number of pages14
JournalAstronomy and Astrophysics
Volume536
DOIs
Publication statusPublished - 12 Dec 2011
MoE publication typeNot Eligible

Fingerprint

Sunyaev-Zeldovich effect
galaxies
calibration
scaling
sky
x rays
XMM-Newton telescope
newton
luminosity
analogs
prediction
predictions
gases
gas
effect
temperature
parameter

Keywords

  • clusters
  • Cosmology
  • Galaxies
  • galaxies
  • interacluster medium
  • observations
  • X-rays

Cite this

Ade, P. A. R., Aghanim, N., Arnaud, M., Ashdown, M., Aumont, J., Baccigalupi, C., ... Planck Collaboration (2011). Planck early results. XI: Calibration of the local galaxy cluster Sunyaev-Zeldovich scaling relations. Astronomy and Astrophysics, 536, [A11]. https://doi.org/10.1051/0004-6361/201116458
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. ; Bond, J. R. ; Borrill, J. ; Bouchet, F. R. ; Bourdin, H. ; Brown, M. L. ; Bucher, M. ; Burigana, C. ; Cabella, P. ; Cardoso, J. F. ; Catalano, A. ; Cayón, L. ; Challinor, A. ; Chamballu, A. ; Chiang, L. Y. ; Chiang, C. ; Chon, G. ; Christensen, P. R. ; Churazov, E. ; Clements, D. L. ; Colafrancesco, S. ; Colombi, S. ; Couchot, F. ; Coulais, A. ; Crill, B. P. ; Cuttaia, F. ; Da Silva, A. ; Dahle, H. ; Danese, L. ; De Bernardis, P. ; De Gasperis, G. ; De Rosa, A. ; Planck Collaboration. / Planck early results. XI : Calibration of the local galaxy cluster Sunyaev-Zeldovich scaling relations. In: Astronomy and Astrophysics. 2011 ; Vol. 536.
@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 = "12",
day = "12",
doi = "10.1051/0004-6361/201116458",
language = "English",
volume = "536",
journal = "Astronomy and Astrophysics",
issn = "0004-6361",
publisher = "EDP Sciences",

}

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

Planck early results. XI : Calibration of the local galaxy cluster Sunyaev-Zeldovich scaling relations. / 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.; Bond, J. R.; Borrill, J.; Bouchet, F. R.; Bourdin, H.; Brown, M. L.; Bucher, M.; Burigana, C.; Cabella, P.; Cardoso, J. F.; Catalano, A.; Cayón, L.; Challinor, A.; Chamballu, A.; Chiang, L. Y.; Chiang, C.; Chon, G.; Christensen, P. R.; Churazov, E.; Clements, D. L.; Colafrancesco, S.; Colombi, S.; Couchot, F.; Coulais, A.; Crill, B. P.; Cuttaia, F.; Da Silva, A.; Dahle, H.; Danese, L.; De Bernardis, P.; De Gasperis, G.; De Rosa, A.; Planck Collaboration.

In: Astronomy and Astrophysics, Vol. 536, A11, 12.12.2011.

Research output: Contribution to journalArticleScientificpeer-review

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

VL - 536

JO - Astronomy and Astrophysics

JF - Astronomy and Astrophysics

SN - 0004-6361

M1 - A11

ER -