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Article
Report number arXiv:1303.5089 ; CERN-PH-TH-2013-141 ; CERN-PH-TH-2013-141
Title Planck 2013 results. XXIX. Planck catalogue of Sunyaev-Zeldovich sources
Author(s)

Ade, P.A.R. (Cardiff U.) ; Aghanim, N. (Paris, Inst. Astrophys.) ; Armitage-Caplan, C. (Oxford U.) ; Arnaud, M. (DAPNIA, Saclay) ; Ashdown, M. (Cambridge U., Inst. of Astron. ; Cambridge U.) ; Atrio-Barandela, F. (Salamanca U.) ; Aumont, J. (Paris, Inst. Astrophys.) ; Aussel, H. (DAPNIA, Saclay) ; Baccigalupi, C. (SISSA, Trieste) ; Banday, A.J. (IRAP, Toulouse ; Toulouse III U.) ; Barreiro, R.B. (Cantabria Inst. of Phys.) ; Barrena, R. (IAC, La Laguna) ; Bartelmann, M. (Garching, Max Planck Inst. ; Heidelberg U.) ; Bartlett, J.G. (Caltech ; APC, Paris) ; Battaner, E. (Granada U.) ; Benabed, K. (Paris U., VI-VII ; Paris, Inst. Astrophys.) ; Benoit, A. (LPSC, Grenoble) ; Benoit-Levy, A. (Paris U., VI-VII ; Paris, Inst. Astrophys. ; University Coll. London) ; Bernard, J.P. (IRAP, Toulouse) ; Bersanelli, M. (Brera Observ. ; Milan U.) ; Bielewicz, P. (SISSA, Trieste ; IRAP, Toulouse ; Toulouse III U.) ; Bikmaev, I. (Acad. Sci. of Tatarstan ; Kazan State U.) ; Bobin, J. (DAPNIA, Saclay) ; Bock, J.J. (Caltech) ; Bohringer, H. (Garching, Max Planck Inst., MPE) ; Bonaldi, A. (Manchester U.) ; Bond, J.R. (Canadian Inst. Theor. Astrophys.) ; Borrill, J. (UC, Berkeley ; LBL, Berkeley) ; Bouchet, F.R. (Paris U., VI-VII ; Paris, Inst. Astrophys.) ; Bridges, M. (Cambridge U. ; Cambridge U., Inst. of Astron.) ; Bucher, M. (APC, Paris) ; Burenin, R. (Moscow, MIPT ; Moscow, Space Res. Inst.) ; Burigana, C. (Ferrara U. ; Bologna Observ.) ; Butler, R.C. (Bologna Observ.) ; Cardoso, J.F. (Paris, Inst. Astrophys. ; APC, Paris ; LTCI, Paris) ; Carvalho, P. (Cambridge U.) ; Catalano, A. (LERMA, Ivry ; LPSC, Grenoble) ; Challinor, A. (Cambridge U., DAMTP ; Cambridge U., Inst. of Astron. ; Cambridge U.) ; Chamballu, A. (Paris, Inst. Astrophys. ; DAPNIA, Saclay) ; Chary, R.R. (Caltech) ; Chen, X. (Caltech) ; Chiang, L.Y. (Taipei, Inst. Astron. Astrophys.) ; Chiang, H.C. (KwaZulu Natal U. ; Princeton U.) ; Chon, G. (Garching, Max Planck Inst., MPE) ; Christensen, P.R. (Bohr Inst.) ; Churazov, E. (Moscow, Space Res. Inst. ; Garching, Max Planck Inst.) ; Church, S. (Stanford U., Phys. Dept.) ; Clements, D.L. (Imperial Coll., London) ; Colombi, S. (Paris U., VI-VII ; Paris, Inst. Astrophys.) ; Colombo, L.P.L. (Caltech ; UCLA) ; Comis, B. (LPSC, Grenoble) ; Couchot, F. (Orsay, LAL) ; Coulais, A. (LERMA, Ivry) ; Crill, B.P. (Caltech) ; Curto, A. (Cantabria Inst. of Phys. ; Cambridge U.) ; Cuttaia, F. (Bologna Observ.) ; Da Silva, A. (Porto U., Astron. Dept.) ; Dahle, H. (Oslo U.) ; Danese, L. (SISSA, Trieste) ; Davies, R.D. (Manchester U.) ; Davis, R.J. (Manchester U.) ; de Bernardis, P. (Rome U.) ; de Rosa, A. (Bologna Observ.) ; de Zotti, G. (SISSA, Trieste ; Padua Observ.) ; Delabrouille, J. (APC, Paris) ; Delouis, J.M. (Paris U., VI-VII ; Paris, Inst. Astrophys.) ; Democles, J. (DAPNIA, Saclay) ; Desert, F.X. (Grenoble Observ.) ; Dickinson, C. (Manchester U.) ; Diego, J.M. (Cantabria Inst. of Phys.) ; Dolag, K. (Garching, Max Planck Inst. ; Munich U.) ; Dole, H. (IUF, Paris ; Paris, Inst. Astrophys.) ; Donzelli, S. (Brera Observ.) ; Dore, O. (Caltech) ; Douspis, M. (Paris, Inst. Astrophys.) ; Dupac, X. (ESA, Madrid) ; Efstathiou, G. (Cambridge U.) ; Ensslin, T.A. (Garching, Max Planck Inst.) ; Eriksen, H.K. (Oslo U.) ; Feroz, F. (Cambridge U.) ; Finelli, F. (INFN, Bologna ; Bologna Observ.) ; Flores-Cacho, I. (Toulouse III U. ; IRAP, Toulouse) ; Forni, O. (IRAP, Toulouse ; Toulouse III U.) ; Frailis, M. (Trieste Observ.) ; Franceschi, E. (Bologna Observ.) ; Fromenteau, S. (Paris, Inst. Astrophys. ; APC, Paris) ; Galeotta, S. (Trieste Observ.) ; Ganga, K. (APC, Paris) ; Genova-Santos, R.T. (IAC, La Laguna) ; Giard, M. (IRAP, Toulouse ; Toulouse III U.) ; Giardino, G. (ESTEC, Noordwijk) ; Gilfanov, M. (Moscow, Space Res. Inst. ; Garching, Max Planck Inst.) ; Giraud-Heraud, Y. (APC, Paris) ; Gonzalez-Nuevo, J. (SISSA, Trieste ; Cantabria Inst. of Phys.) ; Gorski, K.M. (Warsaw U. ; Caltech) ; Grainge, K.J.B. (Cambridge U., Inst. of Astron. ; Cambridge U.) ; Gratton, S. (Cambridge U., Inst. of Astron. ; Cambridge U.) ; Gregorio, A. (Trieste Observ. ; Trieste U.) ; N, E.Groeneboom (Oslo U.) ; Gruppuso, A. (Bologna Observ.) ; Hansen, F.K. (Oslo U.) ; Hanson, D. (Canadian Inst. Theor. Astrophys. ; Caltech ; Rutherford) ; Harrison, D. (Cambridge U., Inst. of Astron. ; Cambridge U.) ; Hempel, A. (Laguna U., Tenerife ; IAC, La Laguna) ; Henrot-Versille, S. (Orsay, LAL) ; Hernandez-Monteagudo, C. (Garching, Max Planck Inst. ; CEFCA, Teruel) ; Herranz, D. (Cantabria Inst. of Phys.) ; Hildebrandt, S.R. (Caltech) ; Hivon, E. (Paris U., VI-VII ; Paris, Inst. Astrophys.) ; Hobson, M. (Cambridge U.) ; Holmes, W.A. (Caltech) ; Hornstrup, A. (Denmark, Tech. U.) ; Hovest, W. (Garching, Max Planck Inst.) ; Huffenberger, K.M. (Miami U.) ; Hurier, G. (LPSC, Grenoble ; Paris, Inst. Astrophys.) ; Hurley-Walker, N. (Cambridge U.) ; Jaffe, T.R. (IRAP, Toulouse ; Toulouse III U.) ; Jaffe, A.H. (Imperial Coll., London) ; Jones, W.C. (Princeton U.) ; Juvela, M. (Helsinki U.) ; Keihanen, E. (Helsinki U.) ; Keskitalo, R. (LBL, Berkeley ; UC, Berkeley) ; Khamitov, I. (Kazan State U. ; Akdeniz U.) ; Kisner, T.S. (LBL, Berkeley) ; Kneissl, R. (European Southern Obs., Chile) ; Knoche, J. (Garching, Max Planck Inst.) ; Knox, L. (UC, Davis) ; Kunz, M. (African Inst. Math. Sci., Cape Town ; Paris, Inst. Astrophys. ; Geneva U.) ; Kurki-Suonio, H. (Helsinki Inst. of Phys. ; Helsinki U.) ; Lagache, G. (Paris, Inst. Astrophys.) ; Lahteenmaki, A. (Helsinki Inst. of Phys. ; Aalto U.) ; Lamarre, J.M. (LERMA, Ivry) ; Lasenby, A. (Cambridge U.) ; Laureijs, R.J. (ESTEC, Noordwijk) ; Lawrence, C.R. (Caltech) ; Leahy, J.P. (Manchester U.) ; Leonardi, R. (ESA, Madrid) ; Leon-Tavares, J. (Aalto U. ; Turku U.) ; Lesgourgues, J. (LPHE, Lausanne ; CERN) ; Li, C. (Garching, Max Planck Inst. ; Shanghai, Astron. Observ.) ; Liddle, A. (Sussex U. ; Royal Observ., Edinburgh) ; Liguori, M. (Padua U.) ; Lilje, P.B. (Oslo U.) ; Linden-Vornle, M. (Denmark, Tech. U.) ; Lopez-Caniego, M. (Cantabria Inst. of Phys.) ; Lubin, P.M. (UC, Santa Barbara) ; Macias-Perez, J.F. (LPSC, Grenoble) ; MacTavish, C.J. (Cambridge U.) ; Maffei, B. (Manchester U.) ; Maino, D. (Brera Observ. ; Milan U.) ; Mandolesi, N. (Ferrara U. ; ASI, Rome ; Bologna Observ.) ; Maris, M. (Trieste Observ.) ; Marshall, D.J. (DAPNIA, Saclay) ; Martin, P.G. (Canadian Inst. Theor. Astrophys.) ; Martinez-Gonzalez, E. (Cantabria Inst. of Phys.) ; Masi, S. (Rome U.) ; Matarrese, S. (Padua U.) ; Matthai, F. (Garching, Max Planck Inst.) ; Mazzotta, P. (Rome U.) ; Mei, S. (Caltech ; APC, Paris ; DARC, Meudon) ; Meinhold, P.R. (UC, Santa Barbara) ; Melchiorri, A. (INFN, Rome ; Rome U.) ; Melin, J.B. (DAPNIA, Saclay) ; Mendes, L. (ESA, Madrid) ; Mennella, A. (Brera Observ. ; Milan U.) ; Migliaccio, M. (Cambridge U., Inst. of Astron. ; Cambridge U.) ; Mitra, S. (Caltech ; Pune U.) ; Miville-Deschenes, M.A. (Canadian Inst. Theor. Astrophys. ; Paris, Inst. Astrophys.) ; Moneti, A. (Paris, Inst. Astrophys.) ; Montier, L. (IRAP, Toulouse ; Toulouse III U.) ; Morgante, G. (Bologna Observ.) ; Mortlock, D. (Imperial Coll., London) ; Munshi, D. (Cardiff U.) ; Naselsky, P. (Bohr Inst.) ; Nati, F. (Rome U.) ; Natoli, P. (Bologna Observ. ; ASDC, Frascati ; Ferrara U.) ; Nesvadba, N.P.H. (Paris, Inst. Astrophys.) ; Netterfield, C.B. (Toronto U.) ; Norgaard-Nielsen, H.U. (Denmark, Tech. U.) ; Noviello, F. (Manchester U.) ; Novikov, D. (Imperial Coll., London) ; Novikov, I. (Bohr Inst.) ; O'Dwyer, I.J. (Caltech) ; Olamaie, M. (Cambridge U.) ; Osborne, S. (Stanford U., Phys. Dept.) ; Oxborrow, C.A. (Denmark, Tech. U.) ; Paci, F. (SISSA, Trieste) ; Pagano, L. (INFN, Rome ; Rome U.) ; Pajot, F. (Paris, Inst. Astrophys.) ; Paoletti, D. (INFN, Bologna ; Bologna Observ.) ; Pasian, F. (Trieste Observ.) ; Patanchon, G. (APC, Paris) ; Pearson, T.J. (Caltech) ; Perdereau, O. (Orsay, LAL) ; Perotto, L. (LPSC, Grenoble) ; Perrott, Y.C. (Cambridge U.) ; Perrotta, F. (SISSA, Trieste) ; Piacentini, F. (Rome U.) ; Piat, M. (APC, Paris) ; Pierpaoli, E. (UCLA) ; Pietrobon, D. (Caltech) ; Plaszczynski, S. (Orsay, LAL) ; Pointecouteau, E. (IRAP, Toulouse ; Toulouse III U.) ; Polenta, G. (Rome Observ. ; ASDC, Frascati) ; Ponthieu, N. (Grenoble Observ. ; Paris, Inst. Astrophys.) ; Popa, L. (Bucharest, Inst. Space Science) ; Poutanen, T. (Aalto U. ; Helsinki U. ; Helsinki Inst. of Phys.) ; Pratt, G.W. (DAPNIA, Saclay) ; Prezeau, G. (Caltech) ; Prunet, S. (Paris U., VI-VII ; Paris, Inst. Astrophys.) ; Puget, J.L. (Paris, Inst. Astrophys.) ; Rachen, J.P. (Garching, Max Planck Inst. ; Nijmegen U.) ; Reach, W.T. (USRA, Huntsville) ; Rebolo, R. (Laguna U., Tenerife ; CSIC, Madrid ; IAC, La Laguna) ; Reinecke, M. (Garching, Max Planck Inst.) ; Remazeilles, M. (APC, Paris ; Paris, Inst. Astrophys.) ; Renault, C. (LPSC, Grenoble) ; Ricciardi, S. (Bologna Observ.) ; Riller, T. (Garching, Max Planck Inst.) ; Ristorcelli, I. (IRAP, Toulouse ; Toulouse III U.) ; Rocha, G. (Caltech) ; Rosset, C. (APC, Paris) ; Roudier, G. (Caltech ; LERMA, Ivry ; APC, Paris) ; Rowan-Robinson, M. (Imperial Coll., London) ; Rubino-Martin, J.A. (Laguna U., Tenerife ; IAC, La Laguna) ; Rumsey, C. (Cambridge U.) ; Rusholme, B. (Caltech) ; Sandri, M. (Bologna Observ.) ; Santos, D. (LPSC, Grenoble) ; Saunders, R.D.E. (Cambridge U., Inst. of Astron. ; Cambridge U.) ; Savini, G. (University Coll. London) ; Scott, D. (British Columbia U.) ; Seiffert, M.D. (Caltech) ; Shellard, E.P.S. (Cambridge U., DAMTP) ; Shimwell, T.W. (Cambridge U.) ; Spencer, L.D. (Cardiff U.) ; Starck, J.L. (DAPNIA, Saclay) ; Stolyarov, V. (Stavropol, Astrophys. Observ. ; Cambridge U., Inst. of Astron. ; Cambridge U.) ; Stompor, R. (APC, Paris) ; Sudiwala, R. (Cardiff U.) ; Sunyaev, R. (Moscow, Space Res. Inst. ; Garching, Max Planck Inst.) ; Sureau, F. (DAPNIA, Saclay) ; Sutton, D. (Cambridge U., Inst. of Astron. ; Cambridge U.) ; Suur-Uski, A.S. (Helsinki Inst. of Phys. ; Helsinki U.) ; Sygnet, J.F. (Paris, Inst. Astrophys.) ; Tauber, J.A. (ESTEC, Noordwijk) ; Tavagnacco, D. (Trieste U. ; Trieste Observ.) ; Terenzi, L. (Bologna Observ.) ; Toffolatti, L. (Cantabria Inst. of Phys. ; Oviedo U.) ; Tomasi, M. (Brera Observ.) ; Tristram, M. (Orsay, LAL) ; Tucci, M. (Orsay, LAL ; Geneva U.) ; Tuovinen, J. (MilliLab) ; Turler, M. (Geneva U.) ; Umana, G. (Catania Astrophys. Observ.) ; Valenziano, L. (Bologna Observ.) ; Valiviita, J. (Oslo U. ; Helsinki U. ; Helsinki Inst. of Phys.) ; Van Tent, B. (Orsay, LPT) ; Vibert, L. (Paris, Inst. Astrophys.) ; Vielva, P. (Cantabria Inst. of Phys.) ; Villa, F. (Bologna Observ.) ; Vittorio, N. (Rome U.) ; Wade, L.A. (Caltech) ; Wandelt, B.D. (Illinois U., Urbana ; Paris U., VI-VII ; Paris, Inst. Astrophys.) ; White, M. (UC, Berkeley) ; White, S.D.M. (Garching, Max Planck Inst.) ; Yvon, D. (DAPNIA, Saclay) ; Zacchei, A. (Trieste Observ.) ; Zonca, A. (UC, Santa Barbara)

Publication 2014-10-29
Imprint 22 Mar 2013
Number of pages 41
Note Comments: 42 pages, submitted to A&A;, catalogue available at ESA's Planck Legacy Archive
42 pages, accepted for publication by A&A;, catalogue available at ESA's Planck Legacy Archive and at SZ cluster database http://szcluster-db.ias.u-psud.fr
In: Astron. Astrophys. 571 (2014) A29
DOI 10.1051/0004-6361/201321523
Subject category Astrophysics and Astronomy
Accelerator/Facility, Experiment PLANCK RE24
Abstract We describe the all-sky Planck catalogue of clusters and cluster candidates derived from Sunyaev--Zeldovich (SZ) effect detections using the first 15.5 months of Planck satellite observations. The catalogue contains 1227 entries, making it over six times the size of the Planck Early SZ (ESZ) sample and the largest SZ-selected catalogue to date. It contains 861 confirmed clusters, of which 178 have been confirmed as clusters, mostly through follow-up observations, and a further 683 are previously-known clusters. The remaining 366 have the status of cluster candidates, and we divide them into three classes according to the quality of evidence that they are likely to be true clusters. The Planck SZ catalogue is the deepest all-sky cluster catalogue, with redshifts up to about one, and spans the broadest cluster mass range from (0.1 to 1.6) 10^{15}Msun. Confirmation of cluster candidates through comparison with existing surveys or cluster catalogues is extensively described, as is the statistical characterization of the catalogue in terms of completeness and statistical reliability. The outputs of the validation process are provided as additional information. This gives, in particular, an ensemble of 813 cluster redshifts, and for all these Planck clusters we also include a mass estimated from a newly-proposed SZ-mass proxy. A refined measure of the SZ Compton parameter for the clusters with X-ray counter-parts is provided, as is an X-ray flux for all the Planck clusters not previously detected in X-ray surveys.
Copyright/License Preprint: © 2013-2024 CERN (License: CC-BY-3.0)



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 Δημιουργία εγγραφής 2013-03-23, τελευταία τροποποίηση 2024-05-03


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