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J/A+A/536/A8 Planck early results. VIII. ESZ sample. (Planck+, 2011)
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Beginning of ReadMe :J/A+A/536/A8 Planck early results. VIII. ESZ sample. (Planck+, 2011)
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Planck early results. VIII. The all-sky early Sunyaev-Zeldovich cluster sample.
Planck Collaboration, Ade P.A.R., Aghanim N., Arnaud M., Ashdown M.,
Aumont J., Baccigalupi C., Baker M., Balbi A., Banday A.J., Barreiro R.B.,
Bartlett J.G., Battaner E., Benabed K., Bennett K., Benoit A.,
Bernard J.-P., Bersanelli M., Bhatia R., Bock J.J., Bonaldi A., Bond J.R.,
Borrill J., Bouchet F.R., Bradshaw T., Bremer M., Bucher M., Burigana C.,
Butler R.C., Cabella P., Cantalupo C.M., Cappellini B., Cardoso J.-F.,
Carr R., Casale M., Catalano A., Cayon L., Challinor A., Chamballu A.,
Charra J., Chary R.-R., Chiang L.-Y., Chiang C., Christensen P.R.,
Clements D.L., Colombi S., Couchot F., Coulais A., Crill B.P., Crone G.,
Crook M., Cuttaia F., Danese L., D'Arcangelo O., Davies R.D., Davis R.J.,
De Bernardis P., De Bruin J., De Gasperis G., De Rosa A., De Zotti G.,
Delabrouille J., Delouis J.-M., Desert F.-X., Dick J., Dickinson C.,
Dolag K., Dole H., Donzelli S., Dore O., Doerl U., Douspis M., Dupac X.,
Efstathiou G., Ensslin T.A., Eriksen H.K., Finelli F., Foley S., Forni O.,
Fosalba P., Frailis M., Franceschi E., Freschi M., Gaier T.C., Galeotta S.,
Gallegos J., Gandolfo B., Ganga K., Giard M., Giardino G., Gienger G.,
Giraud-Heraud Y., Gonzalez J., Gonzalez-Nuevo J., Gorski K.M., Gratton S.,
Gregorio A., Gruppuso A., Guyot G., Haissinski J., Hansen F.K.,
Harrison D., Helou G., Henrot-Versille S., Hernandez-Monteagudo C.,
Herranz D., Hildebrandt S.R., Hivon E., Hobson M., Holmes W.A.,
Hornstrup A., Hovest W., Hoyland R.J., Huffenberger K.M., Jaffe A.H.,
Jagemann T., Jones W.C., Juillet J.J., Juvela M., Kangaslahti P.,
Keihaenen E., Keskitalo R., Kisner T.S., Kneissl R., Knox L.,
Krassenburg M., Kurki-Suonio H., Lagache G., Laehteenmaeki A.,
Lamarre J.-M., Lange A.E., Lasenby A., Laureijs R.J., Lawrence C.R.,
Leach S., Leahy J.P., Leonardi R., Leroy C., Lilje P.B., Linden-Vornle M.,
Lopez-Caniego M., Lowe S., Lubin P.M., Macias-Perez J.F., Maciaszek T.,
Mactavish C.J., Maffei B., Maino D., Mandolesi N., Mann R., Maris M.,
Martinez-Gonzalez E., Masi S., Massardi M., Matarrese S., Matthai F.,
Mazzotta P., McDonald A., McGehee P., Meinhold P.R., Melchiorri A.,
Melin J.-B., Mendes L., Mennella A., Mevi C., Miniscalco R., Mitra S.,
Miville-Deschenes M.-A., Moneti A., Montier L., Morgante G., Morisset N.,
Mortlock D., Munshi D., Murphy A., Naselsky P., Natoli P.,
Netterfield C.B., Norgaard-Nielsen H.U., Noviello F., Novikov D.,
Novikov I., O'dwyer I.J., Ortiz I., Osborne S., Osuna P., Oxborrow C.A.,
Pajot F., Paladini R., Partridge B., Pasian F., Passvogel T., Patanchon G.,
Pearson D., Pearson T.J., Perdereau O., Perotto L., Perrotta F.,
Piacentini F., Piat M., Pierpaoli E., Plaszczynski S., Platania P.,
Pointecouteau E., Polenta G., Ponthieu N., Popa L., Poutanen T.,
Prezeau G., Prunet S., Puget J.-L., Rachen J.P., Reach W.T., Rebolo R.,
Reinecke M., Reix J.-M., Renault C., Ricciardi S., Riller T.,
Ristorcelli I., Rocha G., Rosset C., Rowan-Robinson M., Rubino-Martin J.A.,
Rusholme B., Salerno E., Sandri M., Santos D., Savini G., Schaefer B.M.,
Scott D., Seiffert M.D., Shellard P., Simonetto A., Smoot G.F., Sozzi C.,
Starck J.-L., Sternberg J., Stivoli F., Stolyarov V., Stompor R.,
Stringhetti L., Sudiwala R., Sunyaev R., Sygnet J.-F., Tapiador D.,
Tauber J.A., Tavagnacco D., Taylor D., Terenzi L., Texier D.,
Toffolatti L., Tomasi M., Torre J.-P., Tristram M., Tuovinen J.,
Tuerler M., Tuttlebee M., Umana G., Valenziano L., Valiviita J., Varis J.,
Vibert L., Vielva P., Villa F., Vittorio N., Wade L.A., Wandelt B.D.,
Watson C., White S.D.M., White M., Wilkinson A., Yvon D., Zacchei A.,
Zonca A.
<Astron. Astrophys., 536, A8 (2011)>
=2011A&A...536A...8P
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ADC_Keywords: Clusters, galaxy ; Redshifts
Keywords: cosmology: observations - galaxies: clusters: general - catalogs
Abstract:
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 1x10^15^M_sun_.