J/A+A/536/A8 Planck early results. VIII. ESZ sample. (Planck+, 2011)
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 2011A&A...536A...8P
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 1x1015M☉.
File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
tablea1.dat 98 189 *The Early Sunyaev-Zeldovich (ESZ) sample
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Note on tablea1.dat: the full table is available as file 'esz.dat' in
the Cat. VIII/88.
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See also:
VIII/88 : Planck Early Release Compact Source Catalogue (Planck, 2011)
Byte-by-byte Description of file: tablea1.dat
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Bytes Format Units Label Explanations
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1- 4 A4 --- --- [PLCK]
5- 16 A12 --- PLCK Planck name of cluster candidate,
in Simbad
17- 22 F6.2 deg GLON Galactic longitude from Planck
24- 29 F6.2 deg GLAT Galactic latitude from Planck
31- 35 F5.2 --- S/N Signal-to-noise ratio returned by the matched
multi-Filter algorithm (MMF3)
37- 54 A18 --- Name Other name
56- 59 F4.2 --- z ?=- Redshift of cluster from the MCXC X-ray
cluster compilation unless otherwise
stated in the individual notes
61- 63 A3 --- r.X [---] Angular size at 5R500 from X-ray data
(THETA_X) (always empty)
65- 70 F6.4 arcmin2 Yps.X ?=- Integrated Compton parameter at X-ray
position and within 5R500
72- 77 F6.4 arcmin2 e_Yps.X ?=- rms uncertainty on Yps.X
79- 84 F6.2 deg r ?=- Estimated angular size from matched
multi-Filter (MMF3) (THETA)
86- 91 F6.4 arcmin2 Yps ?=- Integrated Compton parameter at Planck
position and within theta, from matched
multi-Filter (MMF3)
93- 98 F6.4 arcmin2 e_Yps ?=- rms uncertainty on Yps
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History:
From electronic version of the journal
References:
See Plank early results, 2011, A&A 526, A1-A26
(End) Patricia Vannier [CDS] 14-Feb-2012