2011A&A...536A..11P

Query : 2011A&A...536A..11P

2011A&A...536A..11P - Astronomy and Astrophysics, volume 536A, 11-11 (2011/12-1)

Planck early results. XI. Calibration of the local galaxy cluster Sunyaev-Zeldovich scaling relations.

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. and ZONCA A.

Abstract (from CDS):

We present precise Sunyaev-Zeldovich (SZ) effect measurements in the direction of 62 nearby galaxy clusters (z<0.5) detected at high signal-to-noise in the first Planck all-sky data set. The sample spans approximately a decade in total mass, 2x1014M☉<M500<2x1015M☉, where M500 is the mass corresponding to a total density contrast of 500. Combining these high quality Planck measurements with deep XMM-Newton X-ray data, we investigate the relations between DA2 Y500, the integrated Compton parameter due to the SZ effect, and the X-ray-derived gas mass Mg,500, temperature TX, luminosity LX,500, SZ signal analogue YX,500=Mg,500xTX, and total mass M500. After correction for the effect of selection bias on the scaling relations, we find results that are in excellent agreement with both X-ray predictions and recently-published ground-based data derived from smaller samples. The present data yield an exceptionally robust, high-quality local reference, and illustrate Planck's unique capabilities for all-sky statistical studies of galaxy clusters.

Abstract Copyright: ∼

Journal keyword(s): galaxies: clusters: interacluster medium - X-rays: galaxies: clusters - cosmology: observations

Simbad objects: 62

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Number of rows : 62
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2024 		#notes
1 ACO 2744 ClG 00 14 20.03 -30 23 17.8           ~ 813 0
2 ACO 85 ClG 00 41 36.21 -09 19 30.4           ~ 909 0
3 ACO 2813 ClG 00 43 32.377 -20 35 23.51           ~ 96 0
4 ACO 119 ClG 00 56 08.57 -01 12 00.8           ~ 555 2
5 ACT-CL J0232.2-4421 ClG 02 32 18.69 -44 20 41.5           ~ 110 0
6 ACO 401 ClG 02 58 56.9 +13 34 56           ~ 566 0
7 RXC J0303.8-7752 ClG 03 03 00.0 -77 52 00           ~ 12 0
8 ACO 3112 ClG 03 17 52.4 -44 14 35           ~ 311 1
9 ACO 3158 ClG 03 42 39.6 -53 37 50           ~ 304 0
10 ACO 478 ClG 04 13 20.7 +10 28 35           ~ 502 0
11 ACO 3266 ClG 04 31 11.9 -61 24 23           ~ 410 0
12 ACO 520 ClG 04 54 10.1 +02 55 38           ~ 436 0
13 ACO S 520 ClG 05 16 37.40 -54 30 01.5           ~ 95 0
14 ACT-CL J0528.8-3927 ClG 05 28 56.2 -39 27 49           ~ 68 0
15 ACT-CL J0532.9-3701 ClG 05 32 56.4 -37 01 34           ~ 48 0
16 ACO 3364 ClG 05 47 38.1 -31 52 15           ~ 75 0
17 ACO 3376 ClG 06 01 25.000 -39 59 51.00           ~ 305 0
18 ACO 3378 ClG 06 05 53.7 -35 18 06           ~ 81 1
19 ACO 3404 ClG 06 45 29.50 -54 13 37.0           ~ 96 0
20 ClG 0657-56 ClG 06 58 29.6 -55 56 39           ~ 963 1
21 ACO 665 ClG 08 30 45.2 +65 52 55           ~ 437 0
22 ACO 754 ClG 09 09 08.4 -09 39 58           ~ 666 1
23 ACO 773 ClG 09 17 51.3 +51 43 20           ~ 295 0
24 ACO 781 ClG 09 20 25.4 +30 30 07           ~ 153 0
25 ACO 868 ClG 09 45 28.1 -08 38 51           ~ 60 0
26 ACO 963 ClG 10 17 03.4 +39 02 56           ~ 400 0
27 ACO 1300 ClG 11 32 00.7 -19 53 34           ~ 151 0
28 ACO 1413 ClG 11 55 12.87 +23 23 46.9           ~ 430 0
29 MCS J1206.2-0847 ClG 12 06 12.2 -08 48 02           ~ 246 0
30 ZwCl 1215+0400 ClG 12 17 43.62 +03 38 51.5           ~ 153 0
31 ACO 1576 ClG 12 36 59.5 +63 11 18           ~ 108 0
32 BAX 193.6700-29.2254 ClG 12 54 40.6 -29 13 44           ~ 61 0
33 ACO 1644 ClG 12 57 11.6 -17 24 34           ~ 366 1
34 ACO 3532 ClG 12 57 19.2 -30 22 13           ~ 168 2
35 ACO 1650 ClG 12 58 42.0 -01 45 45           ~ 304 0
36 ACO 1651 ClG 12 59 22.43 -04 11 47.1           ~ 290 0
37 ACO 1689 ClG 13 11 29.5 -01 20 28           ~ 1125 0
38 ACO 3558 ClG 13 27 54.8 -31 29 32           ~ 442 2
39 ACO 1763 ClG 13 35 20.1 +41 00 04           ~ 312 0
40 ACO 1795 ClG 13 48 50.48 +26 35 07.4           ~ 1267 0
41 ACO 1914 ClG 14 26 03.32 +37 49 58.7           ~ 314 0
42 ACO 2034 ClG 15 10 12.96 +33 29 53.2           ~ 215 1
43 ACO 2029 ClG 15 10 56.2 +05 44 42           ~ 943 0
44 ACO 2065 ClG 15 22 29.3 +27 42 22           ~ 374 0
45 ACO 2163 ClG 16 15 46.1 -06 08 50           ~ 562 0
46 ACO 2204 ClG 16 32 45.7 +05 34 43           ~ 436 0
47 ACO 2218 ClG 16 35 54.0 +66 13 00           ~ 809 1
48 ACO 2219 ClG 16 40 22.1 +46 42 20           ~ 359 0
49 ACO 2256 ClG 17 03 09.4 +78 39 36           ~ 885 1
50 ACO 2255 ClG 17 12 50.04 +64 03 10.6           ~ 568 0
51 ClG J1720+2638 ClG 17 20 09.6 +26 37 35           ~ 255 0
52 ACO 2261 ClG 17 22 26.9 +32 07 58           ~ 342 0
53 ACO 2390 ClG 21 53 37.4 +17 41 46           ~ 688 2
54 ACO 3827 ClG 22 01 49.1 -59 57 15           ~ 159 0
55 ACO 3854 ClG 22 17 45.72 -35 43 31.4           ~ 67 0
56 ACO 3856 ClG 22 18 45.2 -38 53 57           ~ 79 2
57 BAX 337.1433+20.6131 ClG 22 28 32.6 +20 37 08           ~ 117 0
58 ACO 3888 ClG 22 34 23.0 -37 43 29           ~ 138 1
59 ClG J2243-0935 ClG 22 43 21.1 -09 35 43           ~ 78 0
60 ACO 3911 ClG 22 46 22.6 -52 44 21           ~ 64 0
61 ACO S 1063 ClG 22 48 45.4 -44 31 42           ~ 320 0
62 ACO 3921 ClG 22 49 59.0 -64 25 48           ~ 150 1

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