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) x 10(15) M-circle dot. 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.

Ade, P., Aghanim, N., Armitage Caplan, C., Arnaud, M., Ashdown, M., Atrio Barandela, F., et al. (2014). Planck 2013 results. XXIX. The Planck catalogue of Sunyaev-Zeldovich sources. ASTRONOMY & ASTROPHYSICS, 571 [10.1051/0004-6361/201321523].

Planck 2013 results. XXIX. The Planck catalogue of Sunyaev-Zeldovich sources

MAZZOTTA, PASQUALE;MIGLIACCIO, MARINA;NATOLI, PAOLO;VITTORIO, NICOLA;
2014-01-01

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) x 10(15) M-circle dot. 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.
2014
Pubblicato
Rilevanza internazionale
Articolo
Esperti anonimi
Settore FIS/05 - ASTRONOMIA E ASTROFISICA
English
Ade, P., Aghanim, N., Armitage Caplan, C., Arnaud, M., Ashdown, M., Atrio Barandela, F., et al. (2014). Planck 2013 results. XXIX. The Planck catalogue of Sunyaev-Zeldovich sources. ASTRONOMY & ASTROPHYSICS, 571 [10.1051/0004-6361/201321523].
Ade, P; Aghanim, N; Armitage Caplan, C; Arnaud, M; Ashdown, M; Atrio Barandela, F; Aumont, J; Aussel, H; Baccigalupi, C; Banday, A; Barreiro, R; Barrena, R; Bartelinann, M; Bartlett, J; Battaner, E; Benabed, K; Benoit, A; Benoit Levy, A; Bernard, J; Bersanelli, M; Bielewicz, P; Bikmaev, I; Bobin, J; Bock, J; Boehringer, H; Bonaldi, A; Bond, J; Borrill, J; Bouchet, F; Bridges, M; Bucher, M; Burenin, R; Burigana, C; Butier, R; Cardoso, J; Carvalho, P; Catalano, A; Challinor, A; Chamballu, A; Chary, R; Chen, X; Chiang, H; Chiang, L; Chon, G; Christensen, P; Churazov, E; Church, S; Clements, D; Colombi, S; Colombo, L; Comis, B; Couchot, F; Coulais, A; Crill, B; Curto, A; Cuttaia, F; Da Silva, A; Dahle, H; Danese, L; Davies, R; Davis, R; de Bernardis, P; de Rosa, A; de Zotti, G; Delabrouilie, J; Delouis, J; Democles, J; Desert, F; Dickinson, C; Diego, I; Dolag, K; Dole, H; Donzelli, S; Dore, O; Douspis, M; Dupac, X; Efstathiou, G; Eisenhardt, P; Ensslin, T; Eriksen, H; Feroz, F; Finelli, F; Flores Cacho, I; Forni, O; Frailis, M; Franceschi, E; Fromenteau, S; Galeotta, S; Ganga, K; Genova Santos, R; Giard, M; Giardino, G; Gilfanov, M; Giraud Heraud, Y; Gonzalez Nuevo, J; Gorski, K; Grainge, K; Gratton, S; Gregorio, A; Groeneboom, N; Gruppuso, A; Hansen, F; Hanson, D; Harrison, D; Hempel, A; Elenrot Versille, S; Hernandez Monteagudo, C; Herranz, D; Hildebrandt, S; Hivon, E; Hobson, M; Holmes, W; Homstrup, A; Hovest, W; Huffenberger, K; Hurier, G; Hurley Walker, N; Jaffe, A; Jaffe, T; Jones, W; Juvela, M; Keihanen, E; Keskitalo, R; Khamitov, I; Kisner, T; Kneissl, R; Knoche, J; Knox, L; Kunz, M; Kinti Stionio, H; Laeache, G; Lahteenmaki, A; Lamarre, J; Lasenby, A; Laureijs, R; Lawrence, C; Leahy, J; Leonardi, R; Leon Tavares, J; Lesgourgues, J; Li, C; Liddle, A; Liguori, M; Lilje, P; Linden Vornle, M; Lopez Caniego, M; Lubin, P; Macias Perez, J; Mactavish, C; Maffei, B; Maino, D; Mandolesi, N; Maris, M; Marshal, D; Martin, P; Martinez Gonzalez, E; Masi, S; Massardi, M; Matarrese, S; Matthai, F; Mazzotta, P; Mei, S; Meinhold, P; Meichiorri, A; Melin, J; Mendes, L; Mennelia, A; Migliaccio, M; Mikkeisen, K; Mitra, S; Miville Deschenes, M; Moneti, A; Montier, L; Morgante, G; Mortlock, D; Munshi, D; Murphy, J; Naselsky, P; Nati, F; Natoli, P; Nesvadba, N; Netterfield, C; Norgaard Nielsen, H; Noviello, F; Novikov, D; Novilov, I; O'Dwyer, I; Olamaie, M; Osborne, S; Oxborrow, C; Paci, F; Pagano, L; Pajot, F; Paoletti, D; Pasian, F; Patanchon, G; Pearson, T; Perdereau, O; Perotto, L; Perrott, Y; Perrotta, F; Piacentini, F; Piat, M; Pierpaoli, E; Pletrobon, D; Plaszczynski, S; Pointecouteau, E; Polenta, O; Ponthieu, N; Popa, L; Poutanen, T; Pratt, G; Prezeau, G; Prunet, S; Puget, J; Rachen, J; Reach, W; Rebolo, R; Reinecke, M; Remazeilles, M; Renault, C; Ricciardi, S; Riller, T; Ristorcelli, I; Rocha, G; Rosset, C; Roudier, G; Rowan Robinson, M; Rubino Martin, J; Rumsey, C; Rusholme, B; Sandri, M; Santos, D; Saunders, R; Savini, G; Schammel, M; Scott, D; Seiffert, M; Shellard, E; Shimwell, T; Spencer, L; Stanford, S; Starck, J; Stolyarov, V; Stompor, R; Sudiwala, R; Sunyaev, R; Sureau, F; Sutton, D; Suur Uski, A; Sygnet, J; Tauber, J; Tavagnacco, D; Terenzi, L; Toffolatti, L; Tomasi, M; Tristram, M; Tucci, M; Tuovinen, J; Tuerler, M; Umana, G; Valenziano, L; Valiviita, J; Van Tent, B; Vibert, L; Vielva, P; Vilia, F; Vittorio, N; Wade, L; Wandelt, B; White, M; White, S; Yvon, D; Zacchei, A; Zonca, A
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/2108/177411
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