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

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

doi:10.1051/0004-6361/201219398

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

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

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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. © ESO, 2013.

Original language	English
Journal	Astronomy and Astrophysics
Volume	550
Pages (from-to)	A129
Number of pages	20
ISSN	0004-6361
DOIs	https://doi.org/10.1051/0004-6361/201219398
Publication status	Published - 2013

Keywords

Digital storage
Hydraulics
Hydrodynamics
X rays
Galaxies

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10.1051/0004-6361/201219398

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Bartlett, J. G., Bucher, M., Cardoso, J.-F., Delabrouille, J., Ganga, K., Giraud-Héraud, Y., Le Jeune, M., Piat, M., Remazeilles, M., Rosset, C., Poutanen, T., Bikmaev, I., Natoli, P., Polenta, G., Mandolesi, N., Ashdown, M., Carvalho, P., Hobson, M., Lasenby, A., ... Górski, K. M. (2013). Planck intermediate results: III. the relation between galaxy cluster mass and Sunyaev-Zeldovich signal. Astronomy and Astrophysics, 550, A129. https://doi.org/10.1051/0004-6361/201219398

@article{1098047b279f42489f333be6c5ed17c2,

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 = "Digital storage, Hydraulics, Hydrodynamics, X rays, Galaxies",

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

year = "2013",

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

language = "English",

volume = "550",

pages = "A129",

journal = "Astronomy and Astrophysics",

issn = "0004-6361",

publisher = "EDP Sciences",

}

Bartlett, JG, Bucher, M, Cardoso, J-F, Delabrouille, J, Ganga, K, Giraud-Héraud, Y, Le Jeune, M, Piat, M, Remazeilles, M, Rosset, C, Poutanen, T, Bikmaev, I, Natoli, P, Polenta, G, Mandolesi, N, Ashdown, M, Carvalho, P, Hobson, M, Lasenby, A, Stolyarov, V, Bhatia, R, Kneissl, R, Bond, JR, Miville-Deschênes, M-A, Banday, AJ, Bernard, J-P, Flores-Cacho, I, Forni, O, Giard, M, Marshall, DJ, Montier, L, Pointecouteau, E, Ristorcelli, I, Doré, O, Hildebrandt, SR, Pearson, TJ, Rocha, G, Dahle, H, Lilje, PB, Da Silva, A, Hernández-Monteagudo, C, Borrill, J, Rebolo, R, Melin, J-B, Piffaretti, R, Yvon, D, Linden-Vørnle, M, Nørgaard-Nielsen, HU, Frommert, M, Kunz, M, Atrio-Barandela, F, Toffolatti, L, Bikmaev, I, Rachen, JP, Scott, D, Pierpaoli, E, Liddle, A, Juvela, M, Keihänen, E, Kurki-Suonio, H, Poutanen, T, Suur-Uski, A-S, Meinhold, PR, Zonca, A, Wandelt, BD, Matarrese, S, De Bernardis, P, Masi, S, Melchiorri, A, Piacentini, F, Bersanelli, M, Maino, D, Rossetti, M, Borgani, S, Gregorio, A, Burigana, C, Natoli, P, Balbi, A, Bourdin, H, De Gasperis, G, Mazzotta, P, Vittorio, N, Cabella, P, Rebolo, R, Rubiño-Martín, JA, Kneissl, R, Dupac, X, Jagemann, T, Leonardi, R, Mendes, L, Tauber, JA, Partridge, B, Kurki-Suonio, H, Poutanen, T, Suur-Uski, A-S, Colafrancesco, S, Polenta, G, Borgani, S, Frailis, M, Galeotta, S, Gregorio, A, Maris, M, Zacchei, A, Burigana, C, Butler, RC, Cuttaia, F, Finelli, F, Franceschi, E, Gruppuso, A, Mandolesi, N, Morgante, G, Natoli, P, Paoletti, D, Ricciardi, S, Sandri, M, Terenzi, L, Valenziano, L, Villa, F, Bersanelli, M, Donzelli, S, Maino, D, Rossetti, M, Tomasi, M, Melchiorri, A, Stivoli, F, Désert, F-X, Ponthieu, N, Mitra, S, Chamballu, A, Clements, DL, Pearson, TJ, Rusholme, B, Dole, H, Aghanim, N, Aumont, J, Dole, H, Douspis, M, Kunz, M, Lagache, G, Miville-Deschênes, M-A, Pajot, F, Ponthieu, N, Puget, J-L, Remazeilles, M, Benabed, K, Bouchet, FR, Cardoso, J-F, Hivon, E, Prunet, S, Sygnet, J-F, Wandelt, BD, Popa, L, Marleau, F, Chiang, L-Y, Efstathiou, G, Harrison, D, Sutton, D, Dahle, H, Eriksen, HK, Hansen, FK, Lilje, PB, Génova-Santos, RT, Rebolo, R, Rubiño-Martín, JA, Barreiro, RB, Diego, JM, González-Nuevo, J, Herranz, D, López-Caniego, M, Martínez-González, E, Toffolatti, L, Vielva, P, Platania, P, Bartlett, JG, Doré, O, Górski, KM, Holmes, WA, Lawrence, CR, Mitra, S, Rocha, G, Battye, R, Bonaldi, A, Brown, ML, Davis, RJ, Noviello, F, Ashdown, M, Harrison, D, Lasenby, A, Stolyarov, V, Sutton, D, Luzzi, G, Perdereau, O, Tristram, M, Coulais, A, Lamarre, J-M, Arnaud, M, Démoclès, J, Piffaretti, R, Pratt, GW, Starck, J-L, Cardoso, J-F, Hurier, G, MacÍas-Pérez, JF, Renault, C, Van Tent, B, Dolag, K, Enßlin, TA, Hernández-Monteagudo, C, Knoche, J, Matthai, F, Rachen, JP, Reinecke, M, Sunyaev, R, White, SDM, Böhringer, H, Chon, G, Savini, G, Baccigalupi, C, González-Nuevo, J, Leach, S, Perrotta, F, Ade, PAR, Munshi, D, Sudiwala, R, Burenin, R, Sunyaev, R, Borrill, J, Stolyarov, V, Osborne, S, Khamitov, I, Benabed, K, Bouchet, FR, Hivon, E, Prunet, S, Wandelt, BD, Banday, AJ, Flores-Cacho, I, Forni, O, Giard, M, Marshall, DJ, Montier, L, Pointecouteau, E, Ristorcelli, I, Dolag, K, Weller, J, Battaner, E, Huffenberger, KM & Górski, KM 2013, 'Planck intermediate results: III. the relation between galaxy cluster mass and Sunyaev-Zeldovich signal', Astronomy and Astrophysics, vol. 550, pp. A129. https://doi.org/10.1051/0004-6361/201219398

TY - JOUR

T1 - Planck intermediate results: III. the relation between galaxy cluster mass and Sunyaev-Zeldovich signal

AU - Bartlett, J.G.

AU - Bucher, M.

AU - Cardoso, J.-F.

AU - Delabrouille, J.

AU - Ganga, K.

AU - Giraud-Héraud, Y.

AU - Le Jeune, M.

AU - Piat, M.

AU - Remazeilles, M.

AU - Rosset, C.

AU - Poutanen, T.

AU - Bikmaev, I.

AU - Natoli, P.

AU - Polenta, G.

AU - Mandolesi, N.

AU - Ashdown, M.

AU - Carvalho, P.

AU - Hobson, M.

AU - Lasenby, A.

AU - Stolyarov, V.

AU - Bhatia, R.

AU - Kneissl, R.

AU - Bond, J.R.

AU - Miville-Deschênes, M.-A.

AU - Banday, A.J.

AU - Bernard, J.-P.

AU - Flores-Cacho, I.

AU - Forni, O.

AU - Giard, M.

AU - Marshall, D.J.

AU - Montier, L.

AU - Pointecouteau, E.

AU - Ristorcelli, I.

AU - Doré, O.

AU - Hildebrandt, S.R.

AU - Pearson, T.J.

AU - Rocha, G.

AU - Dahle, H.

AU - Lilje, P.B.

AU - Da Silva, A.

AU - Hernández-Monteagudo, C.

AU - Borrill, J.

AU - Rebolo, R.

AU - Melin, J.-B.

AU - Piffaretti, R.

AU - Yvon, D.

AU - Linden-Vørnle, Michael

AU - Nørgaard-Nielsen, Hans Ulrik

AU - Frommert, M.

AU - Kunz, M.

AU - Atrio-Barandela, F.

AU - Toffolatti, L.

AU - Bikmaev, I.

AU - Rachen, J.P.

AU - Scott, D.

AU - Pierpaoli, E.

AU - Liddle, A.

AU - Juvela, M.

AU - Keihänen, E.

AU - Kurki-Suonio, H.

AU - Poutanen, T.

AU - Suur-Uski, A.-S.

AU - Meinhold, P.R.

AU - Zonca, A.

AU - Wandelt, B.D.

AU - Matarrese, S.

AU - De Bernardis, P.

AU - Masi, S.

AU - Melchiorri, A.

AU - Piacentini, F.

AU - Bersanelli, M.

AU - Maino, D.

AU - Rossetti, M.

AU - Borgani, S.

AU - Gregorio, A.

AU - Burigana, C.

AU - Natoli, P.

AU - Balbi, A.

AU - Bourdin, H.

AU - De Gasperis, G.

AU - Mazzotta, P.

AU - Vittorio, N.

AU - Cabella, P.

AU - Rebolo, R.

AU - Rubiño-Martín, J.A.

AU - Kneissl, R.

AU - Dupac, X.

AU - Jagemann, T.

AU - Leonardi, R.

AU - Mendes, L.

AU - Tauber, J.A.

AU - Partridge, B.

AU - Kurki-Suonio, H.

AU - Poutanen, T.

AU - Suur-Uski, A.-S.

AU - Colafrancesco, S.

AU - Polenta, G.

AU - Borgani, S.

AU - Frailis, M.

AU - Galeotta, S.

AU - Gregorio, A.

AU - Maris, M.

AU - Zacchei, A.

AU - Burigana, C.

AU - Butler, R.C.

AU - Cuttaia, F.

AU - Finelli, F.

AU - Franceschi, E.

AU - Gruppuso, A.

AU - Mandolesi, N.

AU - Morgante, G.

AU - Natoli, P.

AU - Paoletti, D.

AU - Ricciardi, S.

AU - Sandri, M.

AU - Terenzi, L.

AU - Valenziano, L.

AU - Villa, F.

AU - Bersanelli, M.

AU - Donzelli, S.

AU - Maino, D.

AU - Rossetti, M.

AU - Tomasi, M.

AU - Melchiorri, A.

AU - Stivoli, F.

AU - Désert, F.-X.

AU - Ponthieu, N.

AU - Mitra, S.

AU - Chamballu, A.

AU - Clements, D.L.

AU - Pearson, T.J.

AU - Rusholme, B.

AU - Dole, H.

AU - Aghanim, N.

AU - Aumont, J.

AU - Dole, H.

AU - Douspis, M.

AU - Kunz, M.

AU - Lagache, G.

AU - Miville-Deschênes, M.-A.

AU - Pajot, F.

AU - Ponthieu, N.

AU - Puget, J.-L.

AU - Remazeilles, M.

AU - Benabed, K.

AU - Bouchet, F.R.

AU - Cardoso, J.-F.

AU - Hivon, E.

AU - Prunet, S.

AU - Sygnet, J.-F.

AU - Wandelt, B.D.

AU - Popa, L.

AU - Marleau, F.

AU - Chiang, L.-Y.

AU - Efstathiou, G.

AU - Harrison, D.

AU - Sutton, D.

AU - Dahle, H.

AU - Eriksen, H.K.

AU - Hansen, F.K.

AU - Lilje, P.B.

AU - Génova-Santos, R.T.

AU - Rebolo, R.

AU - Rubiño-Martín, J.A.

AU - Barreiro, R.B.

AU - Diego, J.M.

AU - González-Nuevo, J.

AU - Herranz, D.

AU - López-Caniego, M.

AU - Martínez-González, E.

AU - Toffolatti, L.

AU - Vielva, P.

AU - Platania, P.

AU - Bartlett, J.G.

AU - Doré, O.

AU - Górski, K.M.

AU - Holmes, W.A.

AU - Lawrence, C.R.

AU - Mitra, S.

AU - Rocha, G.

AU - Battye, R.

AU - Bonaldi, A.

AU - Brown, M.L.

AU - Davis, R.J.

AU - Noviello, F.

AU - Ashdown, M.

AU - Harrison, D.

AU - Lasenby, A.

AU - Stolyarov, V.

AU - Sutton, D.

AU - Luzzi, G.

AU - Perdereau, O.

AU - Tristram, M.

AU - Coulais, A.

AU - Lamarre, J.-M.

AU - Arnaud, M.

AU - Démoclès, J.

AU - Piffaretti, R.

AU - Pratt, G.W.

AU - Starck, J.-L.

AU - Cardoso, J.-F.

AU - Hurier, G.

AU - MacÍas-Pérez, J.F.

AU - Renault, C.

AU - Van Tent, B.

AU - Dolag, K.

AU - Enßlin, T.A.

AU - Hernández-Monteagudo, C.

AU - Knoche, J.

AU - Matthai, F.

AU - Rachen, J.P.

AU - Reinecke, M.

AU - Sunyaev, R.

AU - White, S.D.M.

AU - Böhringer, H.

AU - Chon, G.

AU - Savini, G.

AU - Baccigalupi, C.

AU - González-Nuevo, J.

AU - Leach, S.

AU - Perrotta, F.

AU - Ade, P.A.R.

AU - Munshi, D.

AU - Sudiwala, R.

AU - Burenin, R.

AU - Sunyaev, R.

AU - Borrill, J.

AU - Stolyarov, V.

AU - Osborne, S.

AU - Khamitov, I.

AU - Benabed, K.

AU - Bouchet, F.R.

AU - Hivon, E.

AU - Prunet, S.

AU - Wandelt, B.D.

AU - Banday, A.J.

AU - Flores-Cacho, I.

AU - Forni, O.

AU - Giard, M.

AU - Marshall, D.J.

AU - Montier, L.

AU - Pointecouteau, E.

AU - Ristorcelli, I.

AU - Dolag, K.

AU - Weller, J.

AU - Battaner, E.

AU - Huffenberger, K.M.

AU - Górski, K.M.

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 - Digital storage

KW - Hydraulics

KW - Hydrodynamics

KW - X rays

KW - Galaxies

U2 - 10.1051/0004-6361/201219398

DO - 10.1051/0004-6361/201219398

M3 - Journal article

SN - 0004-6361

VL - 550

SP - A129

JO - Astronomy and Astrophysics

JF - Astronomy and Astrophysics

ER -

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

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