Planck intermediate results: III. The relation between galaxy cluster mass and Sunyaev-Zeldovich signal

P. A R Ade; N. Aghanim; M. Arnaud; M. Ashdown; F. Atrio-Barandela; J. Aumont; C. Baccigalupi; A. Balbi; A. J. Banday; R. B. Barreiro; J. G. Bartlett; E. Battaner; R. Battye; K. Benabed; J. P. Bernard; M. Bersanelli; R. Bhatia; I. Bikmaev; H. Böhringer; A. Bonaldi; J. R. Bond; S. Borgani; J. Borrill; F. R. Bouchet; H. Bourdin; M. L. Brown; M. Bucher; R. Burenin; C. Burigana; R. C. Butler; P. Cabella; J. F. Cardoso; P. Carvalho; A. Chamballu; L. Y. Chiang; G. Chon; D. L. Clements; S. Colafrancesco; A. Coulais; F. Cuttaia; A. Da Silva; H. Dahle; R. J. Davis; P. De Bernardis; G. De Gasperis; J. Delabrouille; J. Démoclès; F. X. Désert; J. M. Diego; K. Dolag; H. Dole; S. Donzelli; O. Doré; M. Douspis; X. Dupac; G. Efstathiou; T. A. Enßlin; H. K. Eriksen; F. Finelli; I. Flores-Cacho; O. Forni; M. Frailis; E. Franceschi; M. Frommert; S. Galeotta; K. Ganga; R. T. Génova-Santos; M. Giard; Y. Giraud-Héraud; J. González-Nuevo; K. M. Górski; A. Gregorio; A. Gruppuso; F. K. Hansen; D. Harrison; C. Hernández-Monteagudo; D. Herranz; S. R. Hildebrandt; E. Hivon; M. Hobson; W. A. Holmes; K. M. Huffenberger; G. Hurier; T. Jagemann; M. Juvela; E. Keihänen; I. Khamitov; R. Kneissl; J. Knoche; M. Kunz; H. Kurki-Suonio; G. Lagache; J. M. Lamarre; A. Lasenby; C. R. Lawrence; M. Le Jeune; S. Leach; R. Leonardi; A. Liddle; P. B. Lilje; M. Linden-Vørnle; M. López-Caniego; G. Luzzi; J. F. MacÍas-Pérez; D. Maino; N. Mandolesi; M. Maris; F. Marleau; D. J. Marshall; E. Martínez-González; S. Masi; S. Matarrese; F. Matthai; P. Mazzotta; P. R. Meinhold; A. Melchiorri; J. B. Melin; L. Mendes; S. Mitra; M. A. Miville-Deschênes; L. Montier; G. Morgante; D. Munshi; P. Natoli; H. U. Nørgaard-Nielsen; F. Noviello; S. Osborne; F. Pajot; D. Paoletti; B. Partridge; T. J. Pearson; O. Perdereau; F. Perrotta; F. Piacentini; M. Piat; E. Pierpaoli; R. Piffaretti; P. Platania; E. Pointecouteau; G. Polenta; N. Ponthieu; L. Popa; T. Poutanen; G. W. Pratt; S. Prunet; J. L. Puget; J. P. Rachen; R. Rebolo; M. Reinecke; M. Remazeilles; C. Renault; S. Ricciardi; I. Ristorcelli; G. Rocha; C. Rosset; M. Rossetti; J. A. Rubiño-Martín; B. Rusholme; M. Sandri; G. Savini; D. Scott; J. L. Starck; F. Stivoli; V. Stolyarov; R. Sudiwala; R. Sunyaev; D. Sutton; A. S. Suur-Uski; J. F. Sygnet; J. A. Tauber; L. Terenzi; L. Toffolatti; M. Tomasi; M. Tristram; L. Valenziano; B. Van Tent; P. Vielva; F. Villa; N. Vittorio; B. D. Wandelt; J. Weller; S. D M White; D. Yvon; A. Zacchei; A. Zonca

doi:10.1051/0004-6361/201219398

Planck intermediate results: III. The relation between galaxy cluster mass and Sunyaev-Zeldovich signal

P. A R Ade, N. Aghanim, M. Arnaud, M. Ashdown, F. Atrio-Barandela, J. Aumont, C. Baccigalupi, A. Balbi, A. J. Banday, R. B. Barreiro, J. G. Bartlett, E. Battaner, R. Battye, K. Benabed, J. P. Bernard, M. Bersanelli, R. Bhatia, I. Bikmaev, H. Böhringer, A. BonaldiJ. R. Bond, S. Borgani, J. Borrill, F. R. Bouchet, H. Bourdin, M. L. Brown, M. Bucher, R. Burenin, C. Burigana, R. C. Butler, P. Cabella, J. F. Cardoso, P. Carvalho, A. Chamballu, L. Y. Chiang, G. Chon, D. L. Clements, S. Colafrancesco, A. Coulais, F. Cuttaia, A. Da Silva, H. Dahle, R. J. Davis, P. De Bernardis, G. De Gasperis, J. Delabrouille, J. Démoclès, F. X. Désert, J. M. Diego, K. Dolag, H. Dole, S. Donzelli, O. Doré, M. Douspis, X. Dupac, G. Efstathiou, T. A. Enßlin, H. K. Eriksen, F. Finelli, I. Flores-Cacho, O. Forni, M. Frailis, E. Franceschi, M. Frommert, S. Galeotta, K. Ganga, R. T. Génova-Santos, M. Giard, Y. Giraud-Héraud, J. González-Nuevo, K. M. Górski, A. Gregorio, A. Gruppuso, F. K. Hansen, D. Harrison, C. Hernández-Monteagudo, D. Herranz, S. R. Hildebrandt, E. Hivon, M. Hobson, W. A. Holmes, K. M. Huffenberger, G. Hurier, T. Jagemann, M. Juvela, E. Keihänen, I. Khamitov, R. Kneissl, J. Knoche, M. Kunz, H. Kurki-Suonio, G. Lagache, J. M. Lamarre, A. Lasenby, C. R. Lawrence, M. Le Jeune, S. Leach, R. Leonardi, A. Liddle, P. B. Lilje, M. Linden-Vørnle, M. López-Caniego, G. Luzzi, J. F. MacÍas-Pérez, D. Maino, N. Mandolesi, M. Maris, F. Marleau, D. J. Marshall, E. Martínez-González, S. Masi, S. Matarrese, F. Matthai, P. Mazzotta, P. R. Meinhold, A. Melchiorri, J. B. Melin, L. Mendes, S. Mitra, M. A. Miville-Deschênes, L. Montier, G. Morgante, D. Munshi, P. Natoli, H. U. Nørgaard-Nielsen, F. Noviello, S. Osborne, F. Pajot, D. Paoletti, B. Partridge, T. J. Pearson, O. Perdereau, F. Perrotta, F. Piacentini, M. Piat, E. Pierpaoli, R. Piffaretti, P. Platania, E. Pointecouteau, G. Polenta, N. Ponthieu, L. Popa, T. Poutanen, G. W. Pratt^*, S. Prunet, J. L. Puget, J. P. Rachen, R. Rebolo, M. Reinecke, M. Remazeilles, C. Renault, S. Ricciardi, I. Ristorcelli, G. Rocha, C. Rosset, M. Rossetti, J. A. Rubiño-Martín, B. Rusholme, M. Sandri, G. Savini, D. Scott, J. L. Starck, F. Stivoli, V. Stolyarov, R. Sudiwala, R. Sunyaev, D. Sutton, A. S. Suur-Uski, J. F. Sygnet, J. A. Tauber, L. Terenzi, L. Toffolatti, M. Tomasi, M. Tristram, L. Valenziano, B. Van Tent, P. Vielva, F. Villa, N. Vittorio, B. D. Wandelt, J. Weller, S. D M White, D. Yvon, A. Zacchei, A. Zonca

^*Corresponding author for this work

Metsähovi Radio Observatory

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Abstract

We examine the relation between the galaxy cluster mass M and Sunyaev-Zeldovich (SZ) effect signal D_A² Y₅₀₀ for a sample of 19 objects for which weak lensing (WL) mass measurements obtained from Subaru Telescope data are available in the literature. Hydrostatic X-ray masses are derived from XMM-Newton archive data, and the SZ effect signal is measured from Planck all-sky survey data. We find an M_WL-D _A² Y₅₀₀ relation that is consistent in slope and normalisation with previous determinations using weak lensing masses; however, there is a normalisation offset with respect to previous measures based on hydrostatic X-ray mass-proxy relations. We verify that our SZ effect measurements are in excellent agreement with previous determinations from Planck data. For the present sample, the hydrostatic X-ray masses at R₅₀₀ are on average ~ 20 percent larger than the corresponding weak lensing masses, which is contrary to expectations. We show that the mass discrepancy is driven by a difference in mass concentration as measured by the two methods and, for the present sample, that the mass discrepancy and difference in mass concentration are especially large for disturbed systems. The mass discrepancy is also linked to the offset in centres used by the X-ray and weak lensing analyses, which again is most important in disturbed systems. We outline several approaches that are needed to help achieve convergence in cluster mass measurement with X-ray and weak lensing observations. © ESO, 2013.

Original language	English
Article number	A129
Number of pages	20
Journal	Astronomy and Astrophysics
Volume	550
Issue number	A129
DOIs	https://doi.org/10.1051/0004-6361/201219398
Publication status	Published - 2013
MoE publication type	A1 Journal article-refereed

Keywords

Cosmology: observations
Galaxies: clusters: general
Galaxies: clusters: intracluster medium
X-rays: galaxies: clusters

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10.1051/0004-6361/201219398

Planck intermediate results. III. The relationFinal published version, 1.74 MB

Cite this

Ade, P. A. R., Aghanim, N., Arnaud, M., Ashdown, M., Atrio-Barandela, F., Aumont, J., Baccigalupi, C., Balbi, A., Banday, A. J., Barreiro, R. B., Bartlett, J. G., Battaner, E., Battye, R., Benabed, K., Bernard, J. P., Bersanelli, M., Bhatia, R., Bikmaev, I., Böhringer, H., ... Zonca, A. (2013). Planck intermediate results: III. The relation between galaxy cluster mass and Sunyaev-Zeldovich signal. Astronomy and Astrophysics, 550(A129), Article A129. https://doi.org/10.1051/0004-6361/201219398

@article{a4be4a59439d498696c4a495fb7f8c1d,

title = "Planck intermediate results: III. The relation between galaxy cluster mass and Sunyaev-Zeldovich signal",

abstract = "We examine the relation between the galaxy cluster mass M and Sunyaev-Zeldovich (SZ) effect signal DA2 Y500 for a sample of 19 objects for which weak lensing (WL) mass measurements obtained from Subaru Telescope data are available in the literature. Hydrostatic X-ray masses are derived from XMM-Newton archive data, and the SZ effect signal is measured from Planck all-sky survey data. We find an MWL-D A2 Y500 relation that is consistent in slope and normalisation with previous determinations using weak lensing masses; however, there is a normalisation offset with respect to previous measures based on hydrostatic X-ray mass-proxy relations. We verify that our SZ effect measurements are in excellent agreement with previous determinations from Planck data. For the present sample, the hydrostatic X-ray masses at R500 are on average ~ 20 percent larger than the corresponding weak lensing masses, which is contrary to expectations. We show that the mass discrepancy is driven by a difference in mass concentration as measured by the two methods and, for the present sample, that the mass discrepancy and difference in mass concentration are especially large for disturbed systems. The mass discrepancy is also linked to the offset in centres used by the X-ray and weak lensing analyses, which again is most important in disturbed systems. We outline several approaches that are needed to help achieve convergence in cluster mass measurement with X-ray and weak lensing observations. {\textcopyright} ESO, 2013.",

keywords = "Cosmology: observations, Galaxies: clusters: general, Galaxies: clusters: intracluster medium, X-rays: galaxies: clusters",

author = "Ade, {P. A R} and N. Aghanim and M. Arnaud and M. Ashdown and F. Atrio-Barandela and J. Aumont and C. Baccigalupi and A. Balbi and Banday, {A. J.} and Barreiro, {R. B.} and Bartlett, {J. G.} and E. Battaner and R. Battye and K. Benabed and Bernard, {J. P.} and M. Bersanelli and R. Bhatia and I. Bikmaev and H. B{\"o}hringer and A. Bonaldi and Bond, {J. R.} and S. Borgani and J. Borrill and Bouchet, {F. R.} and H. Bourdin and Brown, {M. L.} and M. Bucher and R. Burenin and C. Burigana and Butler, {R. C.} and P. Cabella and Cardoso, {J. F.} and P. Carvalho and A. Chamballu and Chiang, {L. Y.} and G. Chon and Clements, {D. L.} and S. Colafrancesco and A. Coulais and F. Cuttaia and {Da Silva}, A. and H. Dahle and Davis, {R. J.} and {De Bernardis}, P. and {De Gasperis}, G. and J. Delabrouille and J. D{\'e}mocl{\`e}s and D{\'e}sert, {F. X.} and Diego, {J. M.} and K. Dolag and H. Dole and S. Donzelli and O. Dor{\'e} and M. Douspis and X. Dupac and G. Efstathiou and En{\ss}lin, {T. A.} and Eriksen, {H. K.} and F. Finelli and I. Flores-Cacho and O. Forni and M. Frailis and E. Franceschi and M. Frommert and S. Galeotta and K. Ganga and G{\'e}nova-Santos, {R. T.} and M. Giard and Y. Giraud-H{\'e}raud and J. Gonz{\'a}lez-Nuevo and G{\'o}rski, {K. M.} and A. Gregorio and A. Gruppuso and Hansen, {F. K.} and D. Harrison and C. Hern{\'a}ndez-Monteagudo and D. Herranz and Hildebrandt, {S. R.} and E. Hivon and M. Hobson and Holmes, {W. A.} and Huffenberger, {K. M.} and G. Hurier and T. Jagemann and M. Juvela and E. Keih{\"a}nen and I. Khamitov and R. Kneissl and J. Knoche and M. Kunz and H. Kurki-Suonio and G. Lagache and Lamarre, {J. M.} and A. Lasenby and Lawrence, {C. R.} and {Le Jeune}, M. and S. Leach and R. Leonardi and A. Liddle and Lilje, {P. B.} and M. Linden-V{\o}rnle and M. L{\'o}pez-Caniego and G. Luzzi and Mac{\'I}as-P{\'e}rez, {J. F.} and D. Maino and N. Mandolesi and M. Maris and F. Marleau and Marshall, {D. J.} and E. Mart{\'i}nez-Gonz{\'a}lez and S. Masi and S. Matarrese and F. Matthai and P. Mazzotta and Meinhold, {P. R.} and A. Melchiorri and Melin, {J. B.} and L. Mendes and S. Mitra and Miville-Desch{\^e}nes, {M. A.} and L. Montier and G. Morgante and D. Munshi and P. Natoli and N{\o}rgaard-Nielsen, {H. U.} and F. Noviello and S. Osborne and F. Pajot and D. Paoletti and B. Partridge and Pearson, {T. J.} and O. Perdereau and F. Perrotta and F. Piacentini and M. Piat and E. Pierpaoli and R. Piffaretti and P. Platania and E. Pointecouteau and G. Polenta and N. Ponthieu and L. Popa and T. Poutanen and Pratt, {G. W.} and S. Prunet and Puget, {J. L.} and Rachen, {J. P.} and R. Rebolo and M. Reinecke and M. Remazeilles and C. Renault and S. Ricciardi and I. Ristorcelli and G. Rocha and C. Rosset and M. Rossetti and Rubi{\~n}o-Mart{\'i}n, {J. A.} and B. Rusholme and M. Sandri and G. Savini and D. Scott and Starck, {J. L.} and F. Stivoli and V. Stolyarov and R. Sudiwala and R. Sunyaev and D. Sutton and Suur-Uski, {A. S.} and Sygnet, {J. F.} and Tauber, {J. A.} and L. Terenzi and L. Toffolatti and M. Tomasi and M. Tristram and L. Valenziano and {Van Tent}, B. and P. Vielva and F. Villa and N. Vittorio and Wandelt, {B. D.} and J. Weller and White, {S. D M} and D. Yvon and A. Zacchei and A. Zonca",

year = "2013",

doi = "10.1051/0004-6361/201219398",

language = "English",

volume = "550",

journal = "Astronomy and Astrophysics",

issn = "0004-6361",

publisher = "EDP Sciences",

number = "A129",

}

Ade, PAR, Aghanim, N, Arnaud, M, Ashdown, M, Atrio-Barandela, F, Aumont, J, Baccigalupi, C, Balbi, A, Banday, AJ, Barreiro, RB, Bartlett, JG, Battaner, E, Battye, R, Benabed, K, Bernard, JP, Bersanelli, M, Bhatia, R, Bikmaev, I, Böhringer, H, Bonaldi, A, Bond, JR, Borgani, S, Borrill, J, Bouchet, FR, Bourdin, H, Brown, ML, Bucher, M, Burenin, R, Burigana, C, Butler, RC, Cabella, P, Cardoso, JF, Carvalho, P, Chamballu, A, Chiang, LY, Chon, G, Clements, DL, Colafrancesco, S, Coulais, A, Cuttaia, F, Da Silva, A, Dahle, H, Davis, RJ, De Bernardis, P, De Gasperis, G, Delabrouille, J, Démoclès, J, Désert, FX, Diego, JM, Dolag, K, Dole, H, Donzelli, S, Doré, O, Douspis, M, Dupac, X, Efstathiou, G, Enßlin, TA, Eriksen, HK, Finelli, F, Flores-Cacho, I, Forni, O, Frailis, M, Franceschi, E, Frommert, M, Galeotta, S, Ganga, K, Génova-Santos, RT, Giard, M, Giraud-Héraud, Y, González-Nuevo, J, Górski, KM, Gregorio, A, Gruppuso, A, Hansen, FK, Harrison, D, Hernández-Monteagudo, C, Herranz, D, Hildebrandt, SR, Hivon, E, Hobson, M, Holmes, WA, Huffenberger, KM, Hurier, G, Jagemann, T, Juvela, M, Keihänen, E, Khamitov, I, Kneissl, R, Knoche, J, Kunz, M, Kurki-Suonio, H, Lagache, G, Lamarre, JM, Lasenby, A, Lawrence, CR, Le Jeune, M, Leach, S, Leonardi, R, Liddle, A, Lilje, PB, Linden-Vørnle, M, López-Caniego, M, Luzzi, G, MacÍas-Pérez, JF, Maino, D, Mandolesi, N, Maris, M, Marleau, F, Marshall, DJ, Martínez-González, E, Masi, S, Matarrese, S, Matthai, F, Mazzotta, P, Meinhold, PR, Melchiorri, A, Melin, JB, Mendes, L, Mitra, S, Miville-Deschênes, MA, Montier, L, Morgante, G, Munshi, D, Natoli, P, Nørgaard-Nielsen, HU, Noviello, F, Osborne, S, Pajot, F, Paoletti, D, Partridge, B, Pearson, TJ, Perdereau, O, Perrotta, F, Piacentini, F, Piat, M, Pierpaoli, E, Piffaretti, R, Platania, P, Pointecouteau, E, Polenta, G, Ponthieu, N, Popa, L, Poutanen, T, Pratt, GW, Prunet, S, Puget, JL, Rachen, JP, Rebolo, R, Reinecke, M, Remazeilles, M, Renault, C, Ricciardi, S, Ristorcelli, I, Rocha, G, Rosset, C, Rossetti, M, Rubiño-Martín, JA, Rusholme, B, Sandri, M, Savini, G, Scott, D, Starck, JL, Stivoli, F, Stolyarov, V, Sudiwala, R, Sunyaev, R, Sutton, D, Suur-Uski, AS, Sygnet, JF, Tauber, JA, Terenzi, L, Toffolatti, L, Tomasi, M, Tristram, M, Valenziano, L, Van Tent, B, Vielva, P, Villa, F, Vittorio, N, Wandelt, BD, Weller, J, White, SDM, Yvon, D, Zacchei, A & Zonca, A 2013, 'Planck intermediate results: III. The relation between galaxy cluster mass and Sunyaev-Zeldovich signal', Astronomy and Astrophysics, vol. 550, no. A129, A129. https://doi.org/10.1051/0004-6361/201219398

TY - JOUR

T1 - Planck intermediate results

T2 - III. The relation between galaxy cluster mass and Sunyaev-Zeldovich signal

AU - Ade, P. A R

AU - Aghanim, N.

AU - Arnaud, M.

AU - Ashdown, M.

AU - Atrio-Barandela, F.

AU - Aumont, J.

AU - Baccigalupi, C.

AU - Balbi, A.

AU - Banday, A. J.

AU - Barreiro, R. B.

AU - Bartlett, J. G.

AU - Battaner, E.

AU - Battye, R.

AU - Benabed, K.

AU - Bernard, J. P.

AU - Bersanelli, M.

AU - Bhatia, R.

AU - Bikmaev, I.

AU - Böhringer, H.

AU - Bonaldi, A.

AU - Bond, J. R.

AU - Borgani, S.

AU - Borrill, J.

AU - Bouchet, F. R.

AU - Bourdin, H.

AU - Brown, M. L.

AU - Bucher, M.

AU - Burenin, R.

AU - Burigana, C.

AU - Butler, R. C.

AU - Cabella, P.

AU - Cardoso, J. F.

AU - Carvalho, P.

AU - Chamballu, A.

AU - Chiang, L. Y.

AU - Chon, G.

AU - Clements, D. L.

AU - Colafrancesco, S.

AU - Coulais, A.

AU - Cuttaia, F.

AU - Da Silva, A.

AU - Dahle, H.

AU - Davis, R. J.

AU - De Bernardis, P.

AU - De Gasperis, G.

AU - Delabrouille, J.

AU - Démoclès, J.

AU - Désert, F. X.

AU - Diego, J. M.

AU - Dolag, K.

AU - Dole, H.

AU - Donzelli, S.

AU - Doré, O.

AU - Douspis, M.

AU - Dupac, X.

AU - Efstathiou, G.

AU - Enßlin, T. A.

AU - Eriksen, H. K.

AU - Finelli, F.

AU - Flores-Cacho, I.

AU - Forni, O.

AU - Frailis, M.

AU - Franceschi, E.

AU - Frommert, M.

AU - Galeotta, S.

AU - Ganga, K.

AU - Génova-Santos, R. T.

AU - Giard, M.

AU - Giraud-Héraud, Y.

AU - González-Nuevo, J.

AU - Górski, K. M.

AU - Gregorio, A.

AU - Gruppuso, A.

AU - Hansen, F. K.

AU - Harrison, D.

AU - Hernández-Monteagudo, C.

AU - Herranz, D.

AU - Hildebrandt, S. R.

AU - Hivon, E.

AU - Hobson, M.

AU - Holmes, W. A.

AU - Huffenberger, K. M.

AU - Hurier, G.

AU - Jagemann, T.

AU - Juvela, M.

AU - Keihänen, E.

AU - Khamitov, I.

AU - Kneissl, R.

AU - Knoche, J.

AU - Kunz, M.

AU - Kurki-Suonio, H.

AU - Lagache, G.

AU - Lamarre, J. M.

AU - Lasenby, A.

AU - Lawrence, C. R.

AU - Le Jeune, M.

AU - Leach, S.

AU - Leonardi, R.

AU - Liddle, A.

AU - Lilje, P. B.

AU - Linden-Vørnle, M.

AU - López-Caniego, M.

AU - Luzzi, G.

AU - MacÍas-Pérez, J. F.

AU - Maino, D.

AU - Mandolesi, N.

AU - Maris, M.

AU - Marleau, F.

AU - Marshall, D. J.

AU - Martínez-González, E.

AU - Masi, S.

AU - Matarrese, S.

AU - Matthai, F.

AU - Mazzotta, P.

AU - Meinhold, P. R.

AU - Melchiorri, A.

AU - Melin, J. B.

AU - Mendes, L.

AU - Mitra, S.

AU - Miville-Deschênes, M. A.

AU - Montier, L.

AU - Morgante, G.

AU - Munshi, D.

AU - Natoli, P.

AU - Nørgaard-Nielsen, H. U.

AU - Noviello, F.

AU - Osborne, S.

AU - Pajot, F.

AU - Paoletti, D.

AU - Partridge, B.

AU - Pearson, T. J.

AU - Perdereau, O.

AU - Perrotta, F.

AU - Piacentini, F.

AU - Piat, M.

AU - Pierpaoli, E.

AU - Piffaretti, R.

AU - Platania, P.

AU - Pointecouteau, E.

AU - Polenta, G.

AU - Ponthieu, N.

AU - Popa, L.

AU - Poutanen, T.

AU - Pratt, G. W.

AU - Prunet, S.

AU - Puget, J. L.

AU - Rachen, J. P.

AU - Rebolo, R.

AU - Reinecke, M.

AU - Remazeilles, M.

AU - Renault, C.

AU - Ricciardi, S.

AU - Ristorcelli, I.

AU - Rocha, G.

AU - Rosset, C.

AU - Rossetti, M.

AU - Rubiño-Martín, J. A.

AU - Rusholme, B.

AU - Sandri, M.

AU - Savini, G.

AU - Scott, D.

AU - Starck, J. L.

AU - Stivoli, F.

AU - Stolyarov, V.

AU - Sudiwala, R.

AU - Sunyaev, R.

AU - Sutton, D.

AU - Suur-Uski, A. S.

AU - Sygnet, J. F.

AU - Tauber, J. A.

AU - Terenzi, L.

AU - Toffolatti, L.

AU - Tomasi, M.

AU - Tristram, M.

AU - Valenziano, L.

AU - Van Tent, B.

AU - Vielva, P.

AU - Villa, F.

AU - Vittorio, N.

AU - Wandelt, B. D.

AU - Weller, J.

AU - White, S. D M

AU - Yvon, D.

AU - Zacchei, A.

AU - Zonca, A.

PY - 2013

Y1 - 2013

N2 - We examine the relation between the galaxy cluster mass M and Sunyaev-Zeldovich (SZ) effect signal DA2 Y500 for a sample of 19 objects for which weak lensing (WL) mass measurements obtained from Subaru Telescope data are available in the literature. Hydrostatic X-ray masses are derived from XMM-Newton archive data, and the SZ effect signal is measured from Planck all-sky survey data. We find an MWL-D A2 Y500 relation that is consistent in slope and normalisation with previous determinations using weak lensing masses; however, there is a normalisation offset with respect to previous measures based on hydrostatic X-ray mass-proxy relations. We verify that our SZ effect measurements are in excellent agreement with previous determinations from Planck data. For the present sample, the hydrostatic X-ray masses at R500 are on average ~ 20 percent larger than the corresponding weak lensing masses, which is contrary to expectations. We show that the mass discrepancy is driven by a difference in mass concentration as measured by the two methods and, for the present sample, that the mass discrepancy and difference in mass concentration are especially large for disturbed systems. The mass discrepancy is also linked to the offset in centres used by the X-ray and weak lensing analyses, which again is most important in disturbed systems. We outline several approaches that are needed to help achieve convergence in cluster mass measurement with X-ray and weak lensing observations. © ESO, 2013.

AB - We examine the relation between the galaxy cluster mass M and Sunyaev-Zeldovich (SZ) effect signal DA2 Y500 for a sample of 19 objects for which weak lensing (WL) mass measurements obtained from Subaru Telescope data are available in the literature. Hydrostatic X-ray masses are derived from XMM-Newton archive data, and the SZ effect signal is measured from Planck all-sky survey data. We find an MWL-D A2 Y500 relation that is consistent in slope and normalisation with previous determinations using weak lensing masses; however, there is a normalisation offset with respect to previous measures based on hydrostatic X-ray mass-proxy relations. We verify that our SZ effect measurements are in excellent agreement with previous determinations from Planck data. For the present sample, the hydrostatic X-ray masses at R500 are on average ~ 20 percent larger than the corresponding weak lensing masses, which is contrary to expectations. We show that the mass discrepancy is driven by a difference in mass concentration as measured by the two methods and, for the present sample, that the mass discrepancy and difference in mass concentration are especially large for disturbed systems. The mass discrepancy is also linked to the offset in centres used by the X-ray and weak lensing analyses, which again is most important in disturbed systems. We outline several approaches that are needed to help achieve convergence in cluster mass measurement with X-ray and weak lensing observations. © ESO, 2013.

KW - Cosmology: observations

KW - Galaxies: clusters: general

KW - Galaxies: clusters: intracluster medium

KW - X-rays: galaxies: clusters

UR - http://www.scopus.com/inward/record.url?scp=84873647387&partnerID=8YFLogxK

U2 - 10.1051/0004-6361/201219398

DO - 10.1051/0004-6361/201219398

M3 - Article

SN - 0004-6361

VL - 550

JO - Astronomy and Astrophysics

JF - Astronomy and Astrophysics

IS - A129

M1 - A129

ER -

Planck intermediate results: III. The relation between galaxy cluster mass and Sunyaev-Zeldovich signal

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Planck intermediate results: III. The relation between galaxy cluster mass and Sunyaev-Zeldovich signal

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