Planck early results. VIII. The all-sky early Sunyaev-Zeldovich cluster sample

We present the first all-sky sample of galaxy clusters detected blindly by the Planck satellite through the Sunyaev-Zeldovich (SZ) effect from its six highest frequencies. This early SZ (ESZ) sample is comprised of 189 candidates, which have a high signal-to-noise ratio ranging from 6 to 29. Its hig...

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Veröffentlicht in:Astronomy and astrophysics (Berlin) 2011-12, Vol.536, p.A8
Hauptverfasser: Aghanim, N., Baccigalupi, C., Balbi, A., Banday, A. J., Bartelmann, M., Bartlett, J. G., Battaner, E., Benoît, A., Bhatia, R., Bock, J. J., Bond, J. R., Brown, M. L., Bucher, M., Burigana, C., Cantalupo, C. M., Cardoso, J.-F., Catalano, A., Christensen, P. R., Churazov, E., Couchot, F., Coulais, A., de Bernardis, P., Diego, J. M., Douspis, M., Eisenhardt, P., Feroz, F., Fosalba, P., Frailis, M., Fromenteau, S., Ganga, K., Giraud-Héraud, Y., González-Riestra, R., Górski, K. M., Gratton, S., Gregorio, A., Gruppuso, A., Harrison, D., Heinämäki, P., Henrot-Versillé, S., Hernández-Monteagudo, C., Herranz, D., Hildebrandt, S. R., Hovest, W., Hoyland, R. J., Huffenberger, K. M., Jaffe, A. H., Jones, W. C., Keskitalo, R., Kisner, T. S., Knox, L., Laureijs, R. J., Le Jeune, M., Leach, S., Li, C., Linden-Vørnle, M., López-Caniego, M., MacTavish, C. J., Maffei, B., Maris, M., Marleau, F., Martínez-González, E., Matarrese, S., Mennella, A., Mitra, S., Munshi, D., Nati, F., Nørgaard-Nielsen, H. U., Osborne, S., Patanchon, G., Perdereau, O., Perotto, L., Perrotta, F., Piat, M., Pierpaoli, E., Plaszczynski, S., Ponthieu, N., Pratt, G. W., Rachen, J. P., Reinecke, M., Riller, T., Rocha, G., Rosset, C., Santos, D., Saunders, R. D. E., Schaefer, B. M., Scott, D., Smoot, G. F., Stanford, A., Sudiwala, R., Sutton, D., Terenzi, L., Toffolatti, L., Tomasi, M., Torre, J.-P., Valenziano, L., Vibert, L., Wade, L. A., Weller, J., Yvon, D., Zacchei, A.
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Sprache:eng
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Zusammenfassung:We present the first all-sky sample of galaxy clusters detected blindly by the Planck satellite through the Sunyaev-Zeldovich (SZ) effect from its six highest frequencies. This early SZ (ESZ) sample is comprised of 189 candidates, which have a high signal-to-noise ratio ranging from 6 to 29. Its high reliability (purity above 95%) is further ensured by an extensive validation process based on Planck internal quality assessments and by external cross-identification and follow-up observations. Planck provides the first measured SZ signal for about 80% of the 169 previously-known ESZ clusters. Planck furthermore releases 30 new cluster candidates, amongst which 20 meet the ESZ signal-to-noise selection criterion. At the submission date, twelve of the 20 ESZ candidates were confirmed as new clusters, with eleven confirmed using XMM-Newton snapshot observations, most of them with disturbed morphologies and low luminosities. The ESZ clusters are mostly at moderate redshifts (86% with z below 0.3) and span more than a decade in mass, up to the rarest and most massive clusters with masses above 1 × 1015   M⊙.
ISSN:0004-6361
1432-0746
1432-0756
DOI:10.1051/0004-6361/201116459