2013A&A...550A.130P


C.D.S. - SIMBAD4 rel 1.7 - 2020.07.04CEST01:54:09

2013A&A...550A.130P - Astronomy and Astrophysics, volume 550A, 130-130 (2013/2-1)

Planck intermediate results. IV. The XMM-Newton validation programme for new Planck galaxy clusters.

PLANCK COLLABORATION, ADE P.A.R., AGHANIM N., ARNAUD M., ASHDOWN M., AUMONT J., BACCIGALUPI C., BALBI A., BANDAY A.J., BARREIRO R.B., BARTLETT J.G., BATTANER E., BENABED K., BENOIT A., BERNARD J.-P., BERSANELLI M., BIKMAEV I., BOEHRINGER H., BONALDI A., BOND J.R., BORGANI S., BORRILL J., BOUCHET F.R., BROWN M.L., BURIGANA C., BUTLER R.C., CABELLA P., CARVALHO P., CATALANO A., CAYON L., CHAMBALLU A., CHARY R.-R., CHIANG L.-Y., CHON G., CHRISTENSEN P.R., CLEMENTS D.L., COLAFRANCESCO S., COLOMBI S., COULAIS A., CRILL B.P., CUTTAIA F., DA SILVA A., DAHLE H., DAVIS R.J., DE BERNARDIS P., DE GASPERIS G., DE ZOTTI G., DELABROUILLE J., DEMOCLES J., DESERT F.-X., DIEGO J.M., DOLAG K., DOLE H., DONZELLI S., DORE O., DOUSPIS M., DUPAC X., ENSSLIN T.A., ERIKSEN H.K., FINELLI F., FLORES-CACHO I., FORNI O., FRAILIS M., FRANCESCHI E., FROMMERT M., GALEOTTA S., GANGA K., GENOVA-SANTOS R.T., GIRAUD-HERAUD Y., GONZALEZ-NUEVO J., GONZALEZ-RIESTRA R., GORSKI K.M., GREGORIO A., GRUPPUSO A., HANSEN F.K., HARRISON D., HEMPEL A., HENROT-VERSILLE S., HERNANDEZ-MONTEAGUDO C., HERRANZ D., HILDEBRANDT S.R., HIVON E., HOBSON M., HOLMES W.A., HORNSTRUP A., HOVEST W., HUFFENBERGER K.M., HURIER G., JAFFE A.H., JAGEMANN T., JONES W.C., JUVELA M., KNEISSL R., KNOCHE J., KNOX L., KUNZ M., KURKI-SUONIO H., LAGACHE G., LAMARRE J.-M., LASENBY A., LAWRENCE C.R., LE JEUNE M., LEACH S., LEONARDI R., LIDDLE A., LILJE P.B., LINDEN-VORNLE M., LOPEZ-CANIEGO M., LUZZI G., MACIAS-PEREZ J.F., MAINO D., MANDOLESI N., MANN R., MARIS M., MARLEAU F., MARSHALL D.J., MARTINEZ-GONZALEZ E., MASI S., MASSARDI M., MATARRESE S., MAZZOTTA P., MEI S., MEINHOLD P.R., MELCHIORRI A., MELIN J.-B., MENDES L., MENNELLA A., MITRA S., MIVILLE-DESCHENES M.-A., MONETI A., MORGANTE G., MORTLOCK D., MUNSHI D., NASELSKY P., NATI F., NATOLI P., NORGAARD-NIELSEN H.U., NOVIELLO F., OSBORNE S., PAJOT F., PAOLETTI D., PERDEREAU O., PERROTTA F., PIACENTINI F., PIAT M., PIERPAOLI E., PIFFARETTI R., PLASZCZYNSKI S., PLATANIA P., POINTECOUTEAU E., POLENTA G., POPA L., POUTANEN T., PRATT G.W., PRUNET S., PUGET J.-L., REINECKE M., REMAZEILLES M., RENAULT C., RICCIARDI S., ROCHA G., ROSSET C., ROSSETTI M., RUBINO-MARTIN J.A., RUSHOLME B., SANDRI M., SAVINI G., SCOTT D., SMOOT G.F., STANFORD A., STIVOLI F., SUDIWALA R., SUNYAEV R., SUTTON D., SUUR-USKI A.-S., SYGNET J.-F., TAUBER J.A., TERENZI L., TOFFOLATTI L., TOMASI M., TRISTRAM M., VALENZIANO L., VAN TENT B., VIELVA P., VILLA F., VITTORIO N., WADE L.A., WANDELT B.D., WELIKALA N., WELLER J., WHITE S.D.M., YVON D., ZACCHEI A. and ZONCA A.

Abstract (from CDS):

We present the final results from the XMM-Newton validation follow-up of new Planck galaxy cluster candidates. We observed 15 new candidates, detected with signal-to-noise ratios between 4.0 and 6.1 in the 15.5-month nominal Planck survey. The candidates were selected using ancillary data flags derived from the ROSAT All Sky Survey (RASS) and Digitized Sky Survey all-sky maps, with the aim of pushing into the low SZ flux, high-z regime and testing RASS flags as indicators of candidate reliability. Fourteen new clusters were detected by XMM-Newton, ten single clusters and two double systems. Redshifts from X-ray spectroscopy lie in the range 0.2 to 0.9, with six clusters at z>0.5. Estimated masses (M500) range from 2.5x1014 to 8x1014M. We discuss our results in the context of the full XMM-Newton validation programme, in which 51 new clusters have been detected. This includes four double and two triple systems, some of which are chance projections on the sky of clusters at different redshifts. We find that association with a source from the RASS-Bright Source Catalogue is a robust indicator of the reliability of a candidate, whereas association with a source from the RASS-Faint Source Catalogue does not guarantee that the SZ candidate is a bona fide cluster. Nevertheless, most Planck clusters appear in RASS maps, with a significance greater than 2σ being a good indication that the candidate is a real cluster. Candidate validation from association with SDSS galaxy overdensity at z>0.5 is also discussed. The full sample gives a Planck sensitivity threshold of Y500∼4x10–4arcmin2, with indication for Malmquist bias in the YX-Y500 relation below this threshold. The corresponding mass threshold depends on redshift. Systems with M500>5x1014M at z>0.5 are easily detectable with Planck. The newly-detected clusters follow the YX-Y500 relation derived from X-ray selected samples. Compared to X-ray selected clusters, the new SZ clusters have a lower X-ray luminosity on average for their mass. There is no indication of departure from standard self-similar evolution in the X-ray versus SZ scaling properties. In particular, there is no significant evolution of the YX/Y500 ratio.

Abstract Copyright:

Journal keyword(s): cosmology: observations - galaxies: clusters: general - galaxies: clusters: intracluster medium - cosmic background radiation - X-rays: galaxies: clusters

Status at CDS:   Examining the need for a new acronym.

Simbad objects: 33

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Number of rows : 33

N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2020
#notes
1 PLCKESZ G113.1-74.4 ClG 00 41 -11.7           ~ 2 0
2 PSZ1 G205.07-62.94 ClG 02 46 22 -20 31.6           ~ 12 0
3 PLCKESZ G277.75-51.73 ClG 02 54 23 -58 57.8           ~ 30 0
4 PSZ1 G171.96-40.64 ClG 03 12 55 +08 22.8           ~ 29 0
5 PSZ1 G193.29-46.13 ClG 03 35 51.40 -06 58 32.8           ~ 8 0
6 PSZ1 G286.27-38.39 ClG 03 59 12 -72 04.0           ~ 9 0
7 XMMXCS J043818.0-541917.5 ClG 04 38 17.70 -54 19 20.7           ~ 51 0
8 PSZ1 G200.95-28.16 ClG 04 50 20.90 -02 56 57.6           ~ 8 0
9 PSZ1 G286.60-31.23 ClG 05 31 22.3 -75 09 50           ~ 17 0
10 PSZ1 G241.11-28.70 ClG 05 43 04 -36 01.3           ~ 7 0
11 SPT-CL J0549-6205 ClG 05 49 16 -62 05.2           ~ 26 0
12 PLCKESZ G234.2-20.5 ClG 06 11 01.20 -27 35 31.7           ~ 3 0
13 PSZ1 G268.52-28.12 ClG 06 11 18.90 -59 37 23.2           ~ 8 0
14 PLCKESZ G226.1-16.9 ClG 06 12 33 -19 02.4           ~ 2 0
15 PSZ1 G266.56-27.31 ClG 06 15 56.2665 -57 45 50.508           ~ 36 0
16 PSZ1 G284.97-23.69 ClG 07 23.2 -73 27           ~ 13 0
17 PSZ1 G210.64+17.09 ClG 07 48 46.60 +09 40 10.6           ~ 6 0
18 PSZ1 G285.62-17.23 ClG 08 43 49 -71 11.4           ~ 8 0
19 PSZ1 G235.57+23.29 ClG 08 56 05.90 -07 43 15.3           ~ 7 0
20 PLCKESZ G214.6+36.9 ClG 09 08 49 +14 38.5           ~ 4 0
21 PSZ1 G250.02+24.15 ClG 09 32 10 -17 38.8           ~ 8 0
22 PSZ1 G262.24+34.47 ClG 10 34 36.20 -17 21 40.2           ~ 6 0
23 PSZ1 G272.85+48.78 ClG 11 33 14 -09 28.7           ~ 8 0
24 PSZ1 G287.00+32.90 ClG 11 50 49.20 -28 04 36.5           ~ 53 0
25 PSZ1 G292.53+21.97 ClG 12 01 08.18 -39 54 33.0           ~ 9 0
26 PSZ1 G019.12+31.23 ClG 16 36 29.80 +03 08 37.5           ~ 8 0
27 PLCKESZ G018.7+23.6 ClG 17 02 13 -01 00.2           ~ 8 0
28 PLCKESZ G060.1+15.6 ClG 18 41 08.50 +30 55 03.4           ~ 6 0
29 PLCKESZ G004.5-19.5 ClG 19 16 54 -33 30.5           ~ 14 0
30 PLCKESZ G343.4-43.4 ClG 21 20 35 -53 37.9           ~ 2 0
31 PLCKESZ G070.8-21.5 ClG 21 25 38 +19 56.5           ~ 2 0
32 PLCKESZ G100.2-30.4 ClG 23 22 21 +28 33.8           ~ 4 0
33 PLCKESZ G317.4-54.1 ClG 23 40 59 -61 02.3           ~ 2 0

    Equat.    Gal    SGal    Ecl

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2020.07.04-01:54:09

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