Authors:
Bucher, M.^{3} ; Delabrouille, J.^{3} ; Ganga, K.^{3} ; Giraud-Héraud, Y.^{3} ; Le Jeune, M.^{3} ; Piat, M.^{3} ; Rosset, C.^{3} ; Carvalho, P.^{3} ; Hobson, M.^{3} ; Bhatia, R.^{3} ; Bond, J.R.^{3} ; Bernard, J.-P.^{3} ; Hildebrandt, S.R.^{3} ; Da Silva, A.^{3} ; Melin, J.-B.^{3} ; Yvon, D.^{3} ; Linden-Vørnle, Michael^{1} ; Nørgaard-Nielsen, Hans Ulrik^{1} ; Frommert, M.^{3} ; Atrio-Barandela, F.^{3} ; Bikmaev, I.^{3} ; Scott, D.^{3} ; Pierpaoli, E.^{3} ; Liddle, A.^{3} ; Juvela, M.^{3} ; Keihänen, E.^{3} ; Meinhold, P.R.^{3} ; Zonca, A.^{3} ; Matarrese, S.^{3} ; De Bernardis, P.^{3} ; Masi, S.^{3} ; Piacentini, F.^{3} ; Balbi, A.^{3} ; Bourdin, H.^{3} ; De Gasperis, G.^{3} ; Mazzotta, P.^{3} ; Vittorio, N.^{3} ; Cabella, P.^{3} ; Kneissl, R.^{3} ; Dupac, X.^{3} ; Jagemann, T.^{3} ; Leonardi, R.^{3} ; Mendes, L.^{3} ; Tauber, J.A.^{3} ; Partridge, B.^{3} ; Kurki-Suonio, H.^{3} ; Poutanen, T.^{3} ; Suur-Uski, A.-S.^{3} ; Colafrancesco, S.^{3} ; Polenta, G.^{3} ; Borgani, S.^{3} ; Frailis, M.^{3} ; Galeotta, S.^{3} ; Gregorio, A.^{3} ; Maris, M.^{3} ; Zacchei, A.^{3} ; Burigana, C.^{3} ; Butler, R.C.^{3} ; Cuttaia, F.^{3} ; Finelli, F.^{3} ; Franceschi, E.^{3} ; Gruppuso, A.^{3} ; Mandolesi, N.^{3} ; Morgante, G.^{3} ; Natoli, P.^{3} ; Paoletti, D.^{3} ; Ricciardi, S.^{3} ; Sandri, M.^{3} ; Terenzi, L.^{3} ; Valenziano, L.^{3} ; Villa, F.^{3} ; Bersanelli, M.^{3} ; Donzelli, S.^{3} ; Maino, D.^{3} ; Rossetti, M.^{3} ; Tomasi, M.^{3} ; Melchiorri, A.^{3} ; Stivoli, F.^{3} ; Désert, F.-X.^{3} ; Chamballu, A.^{3} ; Clements, D.L.^{3} ; Pearson, T.J.^{3} ; Rusholme, B.^{3} ; Aghanim, N.^{3} ; Aumont, J.^{3} ; Dole, H.^{3} ; Douspis, M.^{3} ; Kunz, M.^{3} ; Lagache, G.^{3} ; Miville-Deschênes, M.-A.^{3} ; Pajot, F.^{3} ; Ponthieu, N.^{3} ; Puget, J.-L.^{3} ; Remazeilles, M.^{3} ; Sygnet, J.-F.^{3} ; Popa, L.^{3} ; Marleau, F.^{3} ; Chiang, L.-Y.^{3} ; Efstathiou, G.^{3} ; Dahle, H.^{3} ; Eriksen, H.K.^{3} ; Hansen, F.K.^{3} ; Lilje, P.B.^{3} ; Génova-Santos, R.T.^{3} ; Rebolo, R.^{3} ; Rubiño-Martín, J.A.^{3} ; Barreiro, R.B.^{3} ; Diego, J.M.^{3} ; Herranz, D.^{3} ; López-Caniego, M.^{3} ; Martínez-González, E.^{3} ; Toffolatti, L.^{3} ; Vielva, P.^{3} ; Platania, P.^{3} ; Bartlett, J.G.^{3} ; Doré, O.^{3} ; Holmes, W.A.^{3} ; Lawrence, C.R.^{3} ; Mitra, S.^{3} ; Rocha, G.^{3} ; Battye, R.^{3} ; Bonaldi, A.^{3} ; Brown, M.L.^{3} ; Davis, R.J.^{3} ; Noviello, F.^{3} ; Ashdown, M.^{3} ; Harrison, D.^{3} ; Lasenby, A.^{3} ; Sutton, D.^{3} ; Luzzi, G.^{3} ; Perdereau, O.^{3} ; Tristram, M.^{3} ; Coulais, A.^{3} ; Lamarre, J.-M.^{3} ; Arnaud, M.^{3} ; Démoclès, J.^{3} ; Piffaretti, R.^{3} ; Pratt, G.W.^{3} ; Starck, J.-L.^{3} ; Cardoso, J.-F.^{3} ; Hurier, G.^{3} ; MacÍas-Pérez, J.F.^{3} ; Renault, C.^{3} ; Van Tent, B.^{3} ; Enßlin, T.A.^{3} ; Hernández-Monteagudo, C.^{3} ; Knoche, J.^{3} ; Matthai, F.^{3} ; Rachen, J.P.^{3} ; Reinecke, M.^{3} ; White, S.D.M.^{3} ; Böhringer, H.^{3} ; Chon, G.^{3} ; Savini, G.^{3} ; Baccigalupi, C.^{3} ; González-Nuevo, J.^{3} ; Leach, S.^{3} ; Perrotta, F.^{3} ; Ade, P.A.R.^{3} ; Munshi, D.^{3} ; Sudiwala, R.^{3} ; Burenin, R.^{3} ; Sunyaev, R.^{3} ; Borrill, J.^{3} ; Stolyarov, V.^{3} ; Osborne, S.^{3} ; Khamitov, I.^{3} ; Benabed, K.^{3} ; Bouchet, F.R.^{3} ; Hivon, E.^{3} ; Prunet, S.^{3} ; Wandelt, B.D.^{3} ; Banday, A.J.^{3} ; Flores-Cacho, I.^{3} ; Forni, O.^{3} ; Giard, M.^{3} ; Marshall, D.J.^{3} ; Montier, L.^{3} ; Pointecouteau, E.^{3} ; Ristorcelli, I.^{3} ; Dolag, K.^{3} ; Weller, J.^{3} ; Battaner, E.^{3} ; Huffenberger, K.M.^{3} ; Górski, K.M.^{3}
Affiliations:
^{1} National Space Institute, Technical University of Denmark^{2} Astrophysics, National Space Institute, Technical University of Denmark^{3} unknown
DOI:
10.1051/0004-6361/201219398
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.
Type:
Journal article
Language:
English
Published in:
Astronomy and Astrophysics, 2013, Vol 550
Keywords:
Digital storage; Hydraulics; Hydrodynamics; X rays; Galaxies
Main Research Area:
Science/technology
Publication Status:
Published
Review type:
Peer Review
Submission year:
2013
Scientific Level:
Scientific
ID:
236372160
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