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Table 1

X-ray temperatures (68% uncertainties), ROSAT 0.1–2.4 keV fluxes, and redshifts of the 73 X-ray clusters used in the present work.

Cluster z T X a s X b Ref.c
NGC 4552 0.001 0.8 19.1 1, 1
NGC 4343GROUP 0.004 0.9 39.7 5, 2
VIRGOCLUSTER 0.004 2.28 761.6 3, 3
VIRGOS 0.004 1.13 18.51 1, 4
NGC 1399GROUP 0.005 1.56 86.8 2, 2
NGC 5044GROUP 0.008 1.22 58.1 5, 6
ABELL3526 0.011 3.92 271.89 1, 6
NGC 1550GROUP 0.012 1.34 31.2 5, 8
RXCJ0419.6+0224 0.012 1.29 40.1 9, 6
ABELL1060 0.013 3.15 99.5 2, 16
ABELL0262 0.016 2.25 93.5 2, 4
NGC 0507GROUP 0.019 1.44 20 5, 2
MKW04 0.02 1.78 22.7 11, 4
ABELL1367 0.022 3.55 60.5 2, 4
ABELL1656 0.023 8.25 344.4 12, 4
ABELL3581 0.023 1.83 33.4 2, 4
ABELL0400 0.024 2.43 27.8 2, 4
MKW08 0.027 3.29 25.1 2, 2
RXJ0341.3+1524 0.029 2.17 20.1 13, 2
ABELL2199 0.03 4.37 106.4 10, 4
RXC J2347.7-2808 0.03 2.61 56.9 14, 4
ABELL2634 0.031 3.45 24.1 2, 4
ABELL0496 0.033 4.12 83.3 14, 4
UGC 03957CLUSTER 0.034 2.6 19.7 14, 4
ABELL2052 0.035 3.12 47.1 2, 4
ABELL2063 0.035 3.57 42.3 14, 4
2A0335+096 0.035 3.64 91.6 2, 4
ABELL2147 0.035 4.34 55.2 2, 4
ABELL3571 0.039 6.81 120.9 14, 4
ABELL0576 0.039 3.68 30.1 14, 4
EXO0422-086 0.04 2.84 30.8 14, 4
ABELL2657 0.04 3.62 25.3 14, 4
ABELL2107 0.041 4 19.4 15, 16
ABELL2589 0.041 3.38 25.9 2, 4
ABELL0119 0.044 5.4 40.5 17, 4
MKW03S 0.045 3.45 33.0 11, 4
ABELL3376 0.046 4.48 24.5 19, 4
Cluster z T X a s X b Ref.c
ABELL1736 0.046 2.95 35.4 14, 4
ABELL1644 0.047 4.86 40.3 17, 4
ABELL3558 0.048 4.78 67.2 17, 4
ABELL4059 0.048 4.25 31.7 14, 4
ABELL3562 0.049 4.31 29.3 14, 4
IC1365 0.049 3.93 19.0 7, 2
ABELL3391 0.051 5.39 22.2 14, 4
ABELL3395SW 0.051 4.42 20.1 11, 2
ABELL3395 0.051 5.1 31.4 14, 14
ABELL0754 0.054 8.93 33.7 17, 4
ABELL0780 0.054 3.42 47.8 10, 4
ABELL0085 0.055 5.78 74.3 17, 4
ABELL3667 0.056 6.33 72.0 14, 4
RXC J0102.7-2152 0.057 4.01 21.2 14, 4
ABELLS1101 0.058 2.59 24.8 19, 4
ABELL2256 0.058 6.4 52.2 17, 20
ABELL3266 0.059 7.46 58.1 17, 4
ABELL3158 0.06 5 37.9 17, 4
ABELL1795 0.062 6.12 62.7 21, 4
ABELL0399 0.072 7.95 32.5 18, 4
ABELL2065 0.073 5.36 25.0 17, 4
ABELL0401 0.074 6.37 52.8 18, 4
ZWCL1215.1+0400 0.075 6.45 21.8 17, 4
ABELL3112 0.075 5.02 31.0 17, 4
ABELL3822 0.076 5.12 19.3 2, 4
ZWCL1742.1+3306 0.076 3.59 18.7 7, 2
ABELL2029 0.077 7.7 69.4 17, 4
ABELL2061 0.078 4.3 18.6 7, 22
ABELL2255 0.081 5.79 20.2 17, 4
ABELL1650 0.084 5.11 24.0 17, 4
ABELL2597 0.085 4.05 22.1 5, 4
ABELL1651 0.085 6.26 25.4 18, 4
ABELL0478 0.088 7.3 51.5 18, 4
ABELL2142 0.091 8.65 62.4 23, 4
ABELL2244 0.097 5.37 21.2 14, 4
ABELL3827 0.098 6.19 19.8 17, 2

Notes.

(a)

Temperature in keV and 68% uncertainties.

(b)

Flux provided by BAX in 10-12 erg/s/cm2 in the 0.1−2.4 keV ROSAT band.

(c)

The first reference is for temperature, the second for the luminosity.

Reference. (1) Fukazawa et al. (2004); (2) Ikebe et al. (2002); (3) Matsumoto et al. (2000); (4) Reiprich & Böhringer (2002); (5) Hudson et al. (2010); (6) Böhringer et al. (2004); (7) Shang & Scharf (2009); (8) Kawaharada et al. (2003); (9) Yoshioka et al. (2004); (10) Simionescu et al. (2009); (11) Rasmussen & Ponman (2007); (12) Arnaud et al. (2001); (13) Sun et al. (2009); (14) Vikhlinin et al. (2009a); (15) Fujita et al. (2006); (16) Jones & Forman (1999); (17) Planck Collaboration XI (2011); (18) Cavagnolo et al. (2008); (19) de Plaa et al. (2007); (20) Fusco-Femiano et al. (2005); (21) Vikhlinin et al. (2006); (22) Marini et al. (2004); (23) De Grandi & Molendi (2002).

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