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Table 2

First ten entries of the X-ray-selected group/cluster sample (185 systems) from the 2XMMi/SDSS Galaxy Cluster Survey with X-ray parameters based on the given flux in the 2XMMi-DR3 catalogue.

Detida Namea RAa Deca Obsida z b Scale R 500 F cat a,c ± eFcat L cat d ± eLcat L 500 e ± eL500 M 500 f ± eM500 T 500 ± eT500
IAUNAME (deg) (deg) kpc/′′ (kpc) (keV) (keV)
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12) (13) (14) (15) (16) (17) (18)

006511 2XMM J004205.5-093613 10.52296 –9.60375 0065140201 0.3256 4.71 582.39 3.30 0.47 11.51 1.63 29.35 4.66 7.87 1.67 1.84 0.45
007481 2XMM J004259.7-092634 10.74900 –9.44286 0065140201 0.4151 5.49 678.59 7.97 1.21 49.11 7.44 106.34 20.98 13.80 2.93 2.65 0.63
011071 2XMM J005608.0+004103 14.03365 0.68427 0303110401 0.4607 5.84 588.27 2.71 0.60 21.40 4.74 51.85 13.25 9.48 2.18 2.12 0.53
014038 2XMM J010606.8+004926 16.52863 0.82407 0150870201 0.2564 3.98 680.44 13.69 1.54 27.55 3.11 60.33 7.82 11.62 2.34 2.30 0.55
014050 2XMM J010610.0+005110 16.54201 0.85302 0150870201 0.2566 3.99 689.89 15.44 1.42 31.12 2.86 65.80 7.60 12.12 2.41 2.36 0.56
021043 2XMM J015558.5+053159 28.99394 5.53329 0153030701 0.4312 5.62 671.20 5.82 0.85 39.27 5.76 105.58 20.88 13.61 2.90 2.64 0.63
021688 2XMM J020056.5-092119 30.23615 –9.35526 0203840201 0.3381 4.83 549.44 2.29 0.24 8.72 0.92 21.37 2.51 6.70 1.40 1.67 0.41
023255 2XMM J021447.5-005425 33.69817 –0.90720 0201020201 0.2650 4.08 484.82 0.88 0.12 1.91 0.27 7.50 0.78 4.24 0.93 1.23 0.32
030889 2XMM J023458.7-085055 38.74463 –8.84868 0150470601 0.2484 3.89 603.14 4.15 0.53 7.77 1.00 27.63 4.52 8.02 1.70 1.83 0.45
033092 2XMM J024810.2+311511 42.04268 31.25311 0111490401 0.3871 5.27 532.12 2.17 0.39 11.31 2.03 20.99 4.49 6.44 1.46 1.64 0.42
034341 2XMM J030212.0+001108 45.55036 0.18583 0041170101 0.6523 6.94 413.91 0.43 0.08 7.91 1.49 12.12 2.98 4.15 1.01 1.33 0.35
006511 1237652947993297563 10.51514 –9.60060 0.3256 0.0000 0 photo-z 138.56
007481 1237652630713795354 10.75138 –9.43350 0.4151 0.0000 0 photo-z 191.29 CXO J004259.9-092704 1
011071 1237663204920328298 14.04250 0.68188 0.4607 0.0000 0 photo-z 192.67
014038 1237663204921376994 16.52926 0.81949 0.2515 0.2564 4 spec-z 68.21 SDSS CE J016.528793+00.817471 2, 3, 4, 5, 6
014050 1237663785278374092 16.54324 0.85569 0.2492 0.2566 5 spec-z 42.90 MaxBCG J016.54324+00.85569 4, 7, 8
021043 1237678663047250389 28.98754 5.53073 0.4312 0.0000 0 photo-z 143.57
021688 1237652900224303421 30.23274 –9.35660 0.3472 0.3381 1 spec-z 62.93
023255 1237680000377684204 33.69949 –0.90894 0.2649 0.2650 1 spec-z 32.01
030889 1237653500970270877 38.74547 –8.84926 0.2484 0.0000 0 photo-z 13.80
033092 1237670458043073373 42.04490 31.25411 0.3871 0.0000 0 photo-z 39.90
034341 1237663784217346252 45.54822 0.18751 0.6516 0.6523 1 spec-z 67.99 BLOX J0302.2+0010.5 9

Notes. The full catalogue is available at CDS and contains the information given in Cols. (1)−(28) in Table 2.

(a)

All these parameters are extracted from the 2XMMi-DR3 catalogue.

(b)

The cluster redshift is from Col. (23) otherwise from Col. (22).

(c)

The given flux in the 2XMMi-DR3 Fcat [0.5−2.0] keV and its errors in units of 10-14 erg cm-2 s-1.

(d)

The computed X-ray luminosity Lcat [0.5−2.0] keV and its errors in units of 1042 erg s-1.

(e)

X-ray bolometric luminosity L500 and its error in units of 1042 erg s-1.

(f)

The cluster mass M500 and its error in units of 1013  M.

(g)

These parameters are obtained from our detection algorithm in the optical band.

Reference. 1 − Evans et al. (2010); 2 − Goto et al. (2002); 3 − Lopes et al. (2004); 4 − Barkhouse et al. (2006); 5 − Wen et al. (2009); 6 − Hao et al. (2010); 7 − Koester et al. (2007); 8 − Bahcall et al. (2003); 9 − Dietrich et al. (2007); 10 − Gunn et al. (1986); 11 − Knobel et al. (2009); 12 − Olsen et al. (2007); 13 − Finoguenov et al. (2007); 14 − Gal et al. (2003); 15 − McConnachie et al. (2009); 16 − Merchán & Zandivarez (2005); 17 − Boschin (2002); 18 − Kolokotronis et al. (2006); 19 − Horner et al. (2008); 20 − Zwicky et al. (1961); 21 − Falco et al. (1999); 22 − Burenin et al. (2007); 23 − Yoon et al. (2008); 24 − Romer et al. (2000); 25 − White et al. (1999).

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