Table 3: Fit parameters with a double $\beta $ model.

Name		 S01 (10-6 cts/s/pixel2) S02 (10-6 cts/s/pixel2) $\beta_1$ $\beta_2$ $r_{\rm c1}$ (kpc) $r_{\rm c2}$ (kpc) $\chi^2_{\rm s}$ $\chi^2_{\rm d}$

A0085		 $27.01 \pm0.99 $ $1.70 \pm 0.24 $ $ 0.60 \pm0.03$ $0.73 \pm0.03$ $58 \pm 3$ $ 385\pm 28 $ 5.32 1.90
A0119 $ 0.50 \pm0.03 $ $0.16 \pm 0.03 $ $ 0.76 \pm0.11$ $1.46 \pm0.24$ $99 \pm45$ $1511\pm 207 $ 1.75 1.47
A0133 $23.96 \pm0.82 $ $0.87 \pm 0.06 $ $ 0.65 \pm0.02$ $0.78 \pm0.02$ $42 \pm 1$ $ 321\pm 13 $ 4.14 1.71
A0401 $ 3.93 \pm0.30 $ $0.51 \pm 0.30 $ $ 0.69 \pm0.08$ $0.66 \pm0.03$ $39 \pm23$ $ 525\pm 93 $ 1.19 1.17
A0478 $37.46 \pm1.30 $ $4.02 \pm 0.71 $ $ 0.68 \pm0.04$ $0.71 \pm0.02$ $72 \pm 4$ $ 253\pm 14 $ 3.53 1.50
A0496 $37.20 \pm1.87 $ $1.40 \pm 0.33 $ $ 0.59 \pm0.05$ $0.69 \pm0.04$ $30 \pm 3$ $ 257\pm 31 $ 3.97 1.07
A1367 $ 0.30 \pm0.01 $ $0.22 \pm 0.01 $ $ 0.96 \pm0.10$ $1.51 \pm0.06$ $91 \pm23$ $ 976\pm 31 $ 1.51 1.14
A1644 $ 1.16 \pm0.24 $ $0.18 \pm 0.06 $ $ 0.83 \pm0.30$ $2.38 \pm0.81$ $74 \pm92$ $2169\pm 532 $ 0.97 0.89
A1651 $ 7.39 \pm0.47 $ $2.17 \pm 0.24 $ $ 0.75 \pm0.07$ $0.76 \pm0.02$ $20 \pm11$ $ 356\pm 17 $ 1.46 1.10
A1795 $41.44 \pm0.60 $ $1.75 \pm 0.16 $ $ 0.72 \pm0.02$ $0.89 \pm0.02$ $79 \pm 2$ $ 432\pm 19 $ 10.04 1.99
A2029 $55.67 \pm1.98 $ $5.81 \pm 1.16 $ $ 0.63 \pm0.03$ $ 0.65 \pm0.02$ $62 \pm 3$ $ 213\pm 15 $ 2.61 1.40
A2052 $23.26 \pm1.43 $ $3.78 \pm 0.46 $ $ 2.10 \pm1.02$ $0.66 \pm0.02$ $84 \pm25$ $ 140\pm 12 $ 2.70 1.45
A2063 $ 4.71 \pm0.00 $ $0.51 \pm 0.00 $ $ 0.49 \pm0.00$ $2.02 \pm0.00$ $55 \pm 0$ $ 640\pm 0 $ 1.97 1.17
A2142 $19.59 \pm0.69 $ $0.86 \pm 0.19 $ $ 0.67 \pm0.04$ $1.01 \pm0.13$ $40 \pm 8$ $ 893\pm 130 $ 2.55 1.39
A2255 $ 0.35 \pm0.05 $ $0.56 \pm 0.05 $ $ 1.15 \pm0.32$ $0.90 \pm0.03$ $69 \pm93$ $ 778\pm 31 $ 1.38 1.36
A2589 $ 3.45 \pm0.28 $ $0.51 \pm 0.23 $ $ 0.66 \pm0.10$ $0.74 \pm0.07$ $95 \pm13$ $ 311\pm 56 $ 1.38 1.23
A2634 $ 0.42 \pm0.04 $ $0.13 \pm 0.01 $ $ 0.47 \pm0.03$ $1.89 \pm0.18$ $80 \pm10$ $1189\pm 77 $ 1.77 1.25
A2657 $ 2.34 \pm0.00 $ $0.25 \pm 0.00 $ $ 0.89 \pm0.00$ $1.27 \pm0.00$ $48 \pm 0$ $ 796\pm 0 $ 3.05 1.68
A3112 $41.34 \pm2.59 $ $3.11 \pm 1.41 $ $ 0.63 \pm0.06$ $0.62 \pm0.03$ $51 \pm 5$ $ 164\pm 24 $ 1.62 1.44
A3266 $ 1.24 \pm0.05 $ $0.76 \pm 0.04 $ $ 1.20 \pm0.11$ $1.27 \pm0.03$ $50 \pm29$ $1162\pm 28 $ 2.62 1.76
A3391 $ 0.87 \pm0.16 $ $0.66 \pm 0.08 $ $ 0.50 \pm0.06$ $0.66 \pm0.03$ $71 \pm19$ $ 335\pm 24 $ 1.30 1.26
A3526 $ 8.97 \pm0.79 $ $0.34 \pm 0.07 $ $ 0.57 \pm0.03$ $0.70 \pm0.05$ $33 \pm 3$ $ 272\pm 32 $ 1.22 1.11
A3558 $ 3.13 \pm0.05 $ $0.20 \pm 0.04 $ $ 0.68 \pm0.03$ $1.17 \pm0.11$ $32 \pm 8$ $1198\pm 119 $ 3.66 2.90
A3562 $ 2.84 \pm0.10 $ $0.07 \pm 0.03 $ $ 0.52 \pm0.02$ $1.26 \pm0.27$ $03 \pm 6$ $1341\pm 273 $ 2.10 1.78
A3571 $ 5.00 \pm0.40 $ $4.39 \pm 0.22 $ $ 0.82 \pm0.13$ $0.68 \pm0.01$ $94 \pm13$ $ 256\pm 6 $ 1.72 1.13
A3667 $ 2.10 \pm0.04 $ $0.20 \pm 0.01 $ $ 0.89 \pm0.03$ $1.70 \pm0.09$ $02 \pm12$ $2375\pm 95 $ 2.53 1.63
A4038 $10.37 \pm0.58 $ $0.49 \pm 0.29 $ $ 0.58 \pm0.04$ $0.70 \pm0.12$ $53 \pm 4$ $ 241\pm 69 $ 1.27 1.18
A4059 $ 8.67 \pm0.46 $ $0.43 \pm 0.18 $ $ 0.64 \pm0.06$ $0.90 \pm0.19$ $82 \pm 7$ $ 438\pm 112 $ 1.32 1.06
COMA $ 1.13 \pm0.54 $ $1.35 \pm 0.52 $ $ 0.57 \pm0.05$ $0.90 \pm0.23$ $29 \pm66$ $ 444\pm 104 $ 1.09 1.09
HYDRA-A $40.63 \pm1.40 $ $5.67 \pm 0.43 $ $ 1.84 \pm0.42$ $0.73 \pm0.01$ $98 \pm14$ $ 183\pm 8 $ 6.24 1.81
MKW3S $12.40 \pm0.92 $ $3.84 \pm 0.62 $ $ 1.42 \pm0.41$ $0.68 \pm0.02$ $91 \pm17$ $ 152\pm 13 $ 2.07 1.54
S1101 $34.57 \pm1.35 $ $0.58 \pm 0.30 $ $ 0.79 \pm0.08$ $0.96 \pm0.16$ $66 \pm 6$ $ 381\pm 104 $ 1.67 1.33
A0539 $ 1.53 \pm0.19 $ $0.41 \pm 0.08 $ $ 0.53 \pm0.09$ $0.75 \pm0.08$ $42 \pm 9$ $ 313\pm 40 $ 1.77 1.19
A1413 $10.29 \pm0.59 $ $1.11 \pm 0.20 $ $ 0.80 \pm0.07$ $0.91 \pm0.05$ $55 \pm12$ $ 559\pm 47 $ 1.73 1.45
A1689 $23.46 \pm1.39 $ $2.53 \pm 0.82 $ $ 0.88 \pm0.14$ $0.91 \pm0.05$ $52 \pm19$ $ 471\pm 56 $ 1.73 1.24
A1775 $ 1.48 \pm0.08 $ $0.18 \pm 0.04 $ $ 2.05 \pm0.69$ $1.70 \pm0.53$ $40 \pm14$ $1443\pm 382 $ 1.62 1.46
A2319 $ 3.59 \pm0.23 $ $0.76 \pm 0.19 $ $ 1.06 \pm0.19$ $0.82 \pm0.06$ $83 \pm48$ $ 874\pm 120 $ 1.34 1.24
A2877 $ 0.28 \pm0.02 $ $0.15 \pm 0.01 $ $ 3.58 \pm0.89$ $1.23 \pm0.07$ $23 \pm47$ $ 606\pm 28 $ 2.79 2.04
A3532 $ 0.91 \pm0.11 $ $0.27 \pm 0.09 $ $ 0.74 \pm0.24$ $1.09 \pm0.21$ $93 \pm48$ $ 761\pm 161 $ 1.31 1.12
A3888 $ 3.90 \pm0.22 $ $0.30 \pm 0.15 $ $ 1.39 \pm0.19$ $1.71 \pm0.39$ $03 \pm47$ $1341\pm 271 $ 0.90 0.90
AWM7 $ 2.53 \pm0.22 $ $0.56 \pm 0.11 $ $ 0.78 \pm0.11$ $0.88 \pm0.05$ $25 \pm16$ $ 406\pm 39 $ 1.40 1.33
HCG 94 $ 2.26 \pm0.09 $ $0.41 \pm 0.04 $ $ 0.53 \pm0.01$ $0.58 \pm0.01$ $59 \pm 3$ $ 199\pm 10 $ 2.43 2.20
NGC 507 $ 1.20 \pm0.30 $ $3.37 \pm 0.34 $ $0.76 \pm 0.04 $ $4.29 \pm1.21$ $41 \pm 4$ $ 73\pm 11 $ 2.41 2.40
NGC 5846 $10.88 \pm0.97 $ $1.48 \pm 0.18 $ $ 0.51 \pm0.01$ $4.78 \pm1.07$ $ 3 \pm 0$ $ 55\pm 7 $ 1.78 1.53
OPHIUCHU $ 4.86 \pm0.24 $ $0.35 \pm 0.10 $ $ 1.04 \pm0.11$ $1.40 \pm0.22$ $28 \pm26$ $1190\pm 177 $ 1.41 1.37
PKS 0745 $53.06 \pm1.73 $ $2.02 \pm 0.39 $ $ 0.70 \pm0.02$ $0.65 \pm0.01$ $72 \pm 2$ $ 235\pm 16 $ 1.17 1.06
RXJ 2344 $ 1.41 \pm0.20 $ $1.41 \pm 0.14 $ $ 0.72 \pm0.13$ $0.92 \pm0.04$ $28 \pm27$ $ 400\pm 20 $ 1.76 1.70
TRIANGUL $ 3.36 \pm0.09 $ $0.66 \pm 0.06 $ $ 0.71 \pm0.03$ $0.80 \pm0.02$ $48 \pm 9$ $ 700\pm 30 $ 1.57 1.28
ZwCl 1742 $ 3.50 \pm0.57 $ $0.58 \pm 0.33 $ $ 0.83 \pm0.21$ $0.93 \pm0.16$ $94 \pm45$ $ 547 \pm 135 $ 1.11 1.11
Note: $\chi^2_{\rm s}$ and $\chi^2_{\rm d}$ are the reduced $\chi^2$ values for the single $\beta $ model and the double $\beta $ model, respectively.
S1 and S2 are the surface brightness. Note  $1 \hbox{$^\prime$ }=120$ pixels.

Source LaTeX | All tables | In the text