학술논문

Planck Early Results XI: Calibration of the local galaxy cluster Sunyaev-Zeldovich scaling relations
Document Type
Working Paper
Author
Planck CollaborationAde, 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. -YChiang, 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.de Zotti, G.Delabrouille, J.Delouis, J. -M.Désert, F. -X.Diego, J. M.Dolag, K.Donzelli, S.Doré, O.Dörl, U.Douspis, M.Dupac, X.Efstathiou, G.Enßlin, T. A.Finelli, F.Flores, I.Forni, O.Frailis, M.Franceschi, E.Fromenteau, S.Galeotta, S.Ganga, K.Génova-Santos, R. T.Giard, M.Giardino, G.Giraud-Héraud, Y.González-Nuevo, J.Górski, K. M.Gratton, S.Gregorio, A.Gruppuso, A.Harrison, D.Henrot-Versillé, S.Hernández-Monteagudo, C.Herranz, D.Hildebrandt, S. R.Hivon, E.Hobson, M.Holmes, W. A.Hovest, W.Hoyland, R. J.Huffenberger, K. M.Jaffe, A. H.Jones, W. C.Juvela, M.Keihänen, E.Keskitalo, R.Kisner, T. S.Kneissl, R.Knox, L.Kurki-Suonio, H.Lagache, G.Lamarre, J. -M.Lanoux, J.Lasenby, A.Laureijs, R. J.Lawrence, C. R.Leach, S.Leonardi, R.Liddle, A.Lilje, P. B.Linden-Vørnle, M.López-Caniego, M.Lubin, P. M.Macías-Pérez, J. F.MacTavish, C. J.Maffei, B.Maino, D.Mandolesi, N.Mann, R.Maris, M.Marleau, F.Martínez-González, E.Masi, S.Matarrese, S.Matthai, F.Mazzotta, P.Melchiorri, A.Melin, J. -B.Mendes, L.Mennella, A.Mitra, S.Miville-Deschênes, M. -A.Moneti, A.Montier, L.Morgante, G.Mortlock, D.Munshi, D.Murphy, A.Naselsky, P.Natoli, P.Netterfield, C. B.Nørgaard-Nielsen, H. U.Noviello, F.Novikov, D.Novikov, I.Osborne, S.Pajot, F.Pasian, F.Patanchon, G.Perdereau, O.Perotto, L.Perrotta, F.Piacentini, F.Piat, M.Pierpaoli, E.Piffaretti, R.Plaszczynski, S.Pointecouteau, E.Polenta, G.Ponthieu, N.Poutanen, T.Pratt, G. W.Prézeau, G.Prunet, S.Puget, J. -L.Rachen, J. P.Rebolo, R.Reinecke, M.Renault, C.Ricciardi, S.Riller, T.Ristorcelli, I.Rocha, G.Rosset, C.Rubiño-Martín, J. A.Rusholme, B.Sandri, M.Santos, D.Savini, G.Schaefer, B. M.Scott, D.Seiffert, M. D.Shellard, P.Smoot, G. F.Starck, J. -L.Stivoli, F.Stolyarov, V.Sudiwala, R.Sunyaev, R.Sygnet, J. -F.Tauber, J. A.Terenzi, L.Toffolatti, L.Tomasi, M.Torre, J. -P.Tristram, M.Tuovinen, J.Valenziano, L.Vibert, L.Vielva, P.Villa, F.Vittorio, N.Wade, L. A.Wandelt, B. D.White, S. D. M.White, M.Yvon, D.Zacchei, A.Zonca, A.
Source
Astron.Astrophys. 536 (2011) A11
Subject
Astrophysics - Cosmology and Nongalactic Astrophysics
Language
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 dataset. The sample spans approximately a decade in total mass, 10^14 < M_500 < 10^15, where M_500 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 Y_500, 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, SZ signal analogue Y_X,500 = M_g,500 * T_X, and total mass M_500. 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.
Comment: 14 pages, 6 figures, to appear in A&A; final version corrects values for A1413 and A3921 in Table 1