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Article
Report number arXiv:1502.01596
Title Planck 2015 results. XXII. A map of the thermal Sunyaev-Zeldovich effect
Author(s)

Aghanim, N. (Orsay, IAS) ; Arnaud, M. (AIM, Saclay) ; Ashdown, M. (Cambridge U., KICC ; Cambridge U.) ; Aumont, J. (Orsay, IAS) ; Baccigalupi, C. (INFN, Trieste ; SISSA, Trieste) ; Banday, A.J. (IRAP, Toulouse) ; Barreiro, R.B. (Cantabria U., Santander) ; Bartlett, J.G. (APC, Paris ; Caltech, JPL) ; Bartolo, N. (Padua U. ; INFN, Padua) ; Battaner, E. (Granada U., Theor. Phys. Astrophys.) ; Battye, R. (Jodrell Bank) ; Benabed, K. (Paris, Inst. Astrophys.) ; Benoît, A. (Neel Lab, Grenoble) ; Benoit-Lévy, A. (University Coll. London ; Paris, Inst. Astrophys.) ; Bernard, J.-P. (IRAP, Toulouse) ; Bersanelli, M. (Milan U. ; IASF, Milan) ; Bielewicz, P. (IRAP, Toulouse ; INFN, Trieste ; SISSA, Trieste) ; Bock, J.J. (Caltech, JPL ; Caltech) ; Bonaldi, A. (Jodrell Bank) ; Bonavera, L. (Cantabria U., Santander) ; Bond, J.R. (Canadian Inst. Theor. Astrophys.) ; Borrill, J. (LBL, Berkeley ; UC, Berkeley, Space Sci. Dept.) ; Bouchet, F.R. (Paris, Inst. Astrophys.) ; Burigana, C. (IASF, Bologna ; Ferrara U. ; INFN, Bologna) ; Butler, R.C. (IASF, Bologna) ; Calabrese, E. (Oxford U.) ; Cardoso, J.-F. (APC, Paris ; Paris, Inst. Astrophys.) ; Catalano, A. (LPSC, Grenoble ; Paris Observ.) ; Challinor, A. (Cambridge U., Inst. of Astron. ; Cambridge U., KICC ; Cambridge U., DAMTP) ; Chiang, H.C. (Princeton U. ; KwaZulu Natal U.) ; Christensen, P.R. (Bohr Inst.) ; Churazov, E. (Garching, Max Planck Inst., MPE ; Moscow, Space Res. Inst.) ; Clements, D.L. (Imperial Coll., London) ; Colombo, L.P.L. (Southern California U. ; Caltech, JPL) ; Combet, C. (LPSC, Grenoble) ; Coulais, A. (Paris Observ.) ; Crill, B.P. (Caltech, JPL ; Caltech) ; Curto, A. (Cambridge U. ; Cantabria U., Santander) ; Cuttaia, F. (IASF, Bologna) ; Danese, L. (INFN, Trieste ; SISSA, Trieste) ; Davies, R.D. (Jodrell Bank) ; Davis, R.J. (Jodrell Bank) ; de Bernardis, P. (Rome U.) ; de Rosa, A. (IASF, Bologna) ; de Zotti, G. (Padua Observ. ; INFN, Trieste ; SISSA, Trieste) ; Delabrouille, J. (APC, Paris) ; Désert, F.-X. (IPAG) ; Dickinson, C. (Jodrell Bank) ; Diego, J.M. (Cantabria U., Santander) ; Dolag, K. (Munich U. Observ. ; Garching, Max Planck Inst., MPE) ; Dole, H. (Orsay, IAS ; IUF, Paris) ; Donzelli, S. (IASF, Milan) ; Doré, O. (Caltech, JPL ; Caltech) ; Douspis, M. (Orsay, IAS) ; Ducout, A. (Paris, Inst. Astrophys. ; Imperial Coll., London) ; Dupac, X. (ESA, Madrid) ; Efstathiou, G. (Cambridge U., Inst. of Astron.) ; Elsner, F. (University Coll. London ; Paris, Inst. Astrophys.) ; Enßlin, T.A. (Garching, Max Planck Inst., MPE) ; Eriksen, H.K. (Inst. Theor. Astrophys., Oslo) ; Fergusson, J. (Cambridge U., DAMTP) ; Finelli, F. (IASF, Bologna ; INFN, Bologna) ; Forni, O. (IRAP, Toulouse) ; Frailis, M. (Trieste Observ.) ; Fraisse, A.A. (Princeton U.) ; Franceschi, E. (IASF, Bologna) ; Frejsel, A. (Bohr Inst.) ; Galeotta, S. (Trieste Observ.) ; Galli, S. (Paris, Inst. Astrophys.) ; Ganga, K. (APC, Paris) ; Génova-Santos, R.T. (IAC, La Laguna ; Laguna U., Tenerife) ; Giard, M. (IRAP, Toulouse) ; González-Nuevo, J. (Cantabria U., Santander ; INFN, Trieste ; SISSA, Trieste) ; Górski, K.M. (Caltech, JPL ; Warsaw U. Observ.) ; Gregorio, A. (Trieste U. ; Trieste Observ. ; INFN, Trieste) ; Gruppuso, A. (IASF, Bologna) ; Gudmundsson, J.E. (Princeton U.) ; Hansen, F.K. (Inst. Theor. Astrophys., Oslo) ; Harrison, D.L. (Cambridge U., Inst. of Astron. ; Cambridge U., KICC) ; Henrot-Versillé, S. (Orsay, LAL) ; Hernández-Monteagudo, C. (CEFCA, Teruel ; Garching, Max Planck Inst., MPE) ; Herranz, D. (Cantabria U., Santander) ; Hildebrandt, S.R. (Caltech, JPL ; Caltech) ; Hivon, E. (Paris, Inst. Astrophys.) ; Holmes, W.A. (Caltech, JPL) ; Hornstrup, A. (Denmark, Tech. U.) ; Huffenberger, K.M. (Florida State U.) ; Hurier, G. (Orsay, IAS) ; Jaffe, A.H. (Imperial Coll., London) ; Jones, W.C. (Princeton U.) ; Juvela, M. (Helsinki Inst. of Phys. ; Helsinki U.) ; Keihänen, E. (Helsinki Inst. of Phys. ; Helsinki U.) ; Keskitalo, R. (LBL, Berkeley) ; Kneissl, R. (European Southern Obs., Chile) ; Knoche, J. (Garching, Max Planck Inst., MPE) ; Kunz, M. (Geneva U., Dept. Theor. Phys. ; Orsay, IAS ; African Inst. Math. Sci., Cape Town) ; Kurki-Suonio, H. (Helsinki Inst. of Phys. ; Helsinki U.) ; Lacasa, F. (Orsay, IAS ; ICTP-SAIFR, Sao Paulo) ; Lagache, G. (Marseille, Lab. Astrophys. ; Orsay, IAS) ; Lähteenmäki, A. (Aalto U. ; Helsinki Inst. of Phys.) ; Lamarre, J.-M. (Paris Observ.) ; Lasenby, A. (Cambridge U. ; Cambridge U., KICC) ; Lattanzi, M. (Ferrara U.) ; Leonardi, R. (ESA, Madrid) ; Lesgourgues, J. (CERN ; Ecole Polytechnique, Lausanne ; Annecy, LAPTH) ; Levrier, F. (Paris Observ.) ; Liguori, M. (Padua U. ; INFN, Padua) ; Lilje, P.B. (Inst. Theor. Astrophys., Oslo) ; Linden-Vørnle, M. (Denmark, Tech. U.) ; López-Caniego, M. (ESA, Madrid ; Cantabria U., Santander) ; Macías-Pérez, J.F. (LPSC, Grenoble) ; Maffei, B. (Jodrell Bank) ; Maggio, G. (Trieste Observ.) ; Maino, D. (Milan U. ; IASF, Milan) ; Mandolesi, N. (IASF, Bologna ; Ferrara U.) ; Mangilli, A. (Orsay, IAS ; Orsay, LAL) ; Maris, M. (Trieste Observ.) ; Martin, P.G. (Canadian Inst. Theor. Astrophys.) ; Martínez-González, E. (Cantabria U., Santander) ; Masi, S. (Rome U.) ; Matarrese, S. (Padua U. ; INFN, Padua ; GSSI, Aquila) ; Melchiorri, A. (Rome U. ; INFN, Rome) ; Melin, J.-B. (IRFU, SPP, Saclay) ; Migliaccio, M. (Cambridge U., Inst. of Astron. ; Cambridge U., KICC) ; Miville-Deschênes, M.-A. (Orsay, IAS ; Canadian Inst. Theor. Astrophys.) ; Moneti, A. (Paris, Inst. Astrophys.) ; Montier, L. (IRAP, Toulouse) ; Morgante, G. (IASF, Bologna) ; Mortlock, D. (Imperial Coll., London) ; Munshi, D. (Cardiff U.) ; Murphy, J.A. (NUIM, Maynooth) ; Naselsky, P. (Bohr Inst.) ; Nati, F. (Princeton U.) ; Natoli, P. (Ferrara U. ; ASI, Rome ; IASF, Bologna) ; Noviello, F. (Jodrell Bank) ; Novikov, D. (Lebedev Inst.) ; Novikov, I. (Bohr Inst. ; Lebedev Inst.) ; Paci, F. (INFN, Trieste ; SISSA, Trieste) ; Pagano, L. (Rome U. ; INFN, Rome) ; Pajot, F. (Orsay, IAS) ; Paoletti, D. (IASF, Bologna ; INFN, Bologna) ; Pasian, F. (Trieste Observ.) ; Patanchon, G. (APC, Paris) ; Perdereau, O. (Orsay, LAL) ; Perotto, L. (LPSC, Grenoble) ; Pettorino, V. (U. Heidelberg, ITP) ; Piacentini, F. (Rome U.) ; Piat, M. (APC, Paris) ; Pierpaoli, E. (Southern California U.) ; Pietrobon, D. (Caltech, JPL) ; Plaszczynski, S. (Orsay, LAL) ; Pointecouteau, E. (IRAP, Toulouse) ; Polenta, G. (ASI, Rome ; Rome Observ.) ; Ponthieu, N. (Orsay, IAS ; IPAG) ; Pratt, G.W. (AIM, Saclay) ; Prunet, S. (Paris, Inst. Astrophys.) ; Puget, J.-L. (Orsay, IAS) ; Rachen, J.P. (Nijmegen U., IMAPP ; Garching, Max Planck Inst., MPE) ; Reinecke, M. (Garching, Max Planck Inst., MPE) ; Remazeilles, M. (Jodrell Bank ; Orsay, IAS ; APC, Paris) ; Renault, C. (LPSC, Grenoble) ; Renzi, A. (Rome U., Tor Vergata ; INFN, Rome2) ; Ristorcelli, I. (IRAP, Toulouse) ; Rocha, G. (Caltech, JPL ; Caltech) ; Rossetti, M. (Milan U. ; IASF, Milan) ; Roudier, G. (APC, Paris ; Paris Observ. ; Caltech, JPL) ; Rubiño-Martín, J.A. (IAC, La Laguna ; Laguna U., Tenerife) ; Rusholme, B. (Caltech, IPAC) ; Sandri, M. (IASF, Bologna) ; Santos, D. (LPSC, Grenoble) ; Sauvé, A. (IRAP, Toulouse) ; Savelainen, M. (Helsinki Inst. of Phys. ; Helsinki U.) ; Savini, G. (University Coll. London) ; Scott, D. (British Columbia U.) ; Spencer, L.D. (Cardiff U.) ; Stolyarov, V. (Cambridge U. ; Cambridge U., KICC ; Stavropol, Astrophys. Observ.) ; Stompor, R. (APC, Paris) ; Sunyaev, R. (Garching, Max Planck Inst., MPE ; Moscow, Space Res. Inst.) ; Sutton, D. (Cambridge U., Inst. of Astron. ; Cambridge U., KICC) ; Suur-Uski, A.-S. (Helsinki Inst. of Phys. ; Helsinki U.) ; Sygnet, J.-F. (Paris, Inst. Astrophys.) ; Tauber, J.A. (ESTEC, Noordwijk) ; Terenzi, L. (Rome U. ; IASF, Bologna) ; Toffolatti, L. (Oviedo U. ; Cantabria U., Santander ; IASF, Bologna) ; Tomasi, M. (Milan U. ; IASF, Milan) ; Tramonte, D. (IAC, La Laguna ; Laguna U., Tenerife) ; Tristram, M. (Orsay, LAL) ; Tucci, M. (Geneva U., Dept. Theor. Phys.) ; Tuovinen, J. (Trinity Coll., Dublin) ; Valenziano, L. (IASF, Bologna) ; Valiviita, J. (Helsinki Inst. of Phys. ; Helsinki U.) ; Van Tent, B. (Orsay, LPT) ; Vielva, P. (Cantabria U., Santander) ; Villa, F. (IASF, Bologna) ; Wade, L.A. (Caltech, JPL) ; Wandelt, B.D. (Paris, Inst. Astrophys. ; Illinois U., Urbana) ; Wehus, I.K. (Caltech, JPL) ; Yvon, D. (IRFU, SPP, Saclay) ; Zacchei, A. (Trieste Observ.)

Publication 2016-09-20
Imprint 05 Feb 2015
Number of pages 24
Note 25 pages, 19 figures, submitted to A&A
In: Astron. Astrophys. 594 (2016) A22
DOI 10.1051/0004-6361/201525826
Subject category Astrophysics and Astronomy
Abstract We have constructed all-sky y-maps of the thermal Sunyaev-Zeldovich (tSZ) effect by applying specifically tailored component separation algorithms to the 30 to 857 GHz frequency channel maps from the Planck satellite survey. These reconstructed y-maps are delivered as part of the Planck 2015 release. The y-maps are characterised in terms of noise properties and residual foreground contamination, mainly thermal dust emission at large angular scales and CIB and extragalactic point sources at small angular scales. Specific masks are defined to minimize foreground residuals and systematics. Using these masks we compute the y-map angular power spectrum and higher order statistics. From these we conclude that the y-map is dominated by tSZ signal in the multipole range, 20-600. We compare the measured tSZ power spectrum and higher order statistics to various physically motivated models and discuss the implications of our results in terms of cluster physics and cosmology.
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