Table 2: Deduced properties of all 13 galaxy clusters. Column (1): cluster name; Col. (2): electron number density of the inner most radial bin; Col. (3): entropy at 0.2 r₅₀₀; Col. (4): inner most radial bin of the surface brightness profile; Col. (5): cooling time measured at $r_{\rm cen}$ ; Col. (6): cooling radius; Col. (7): r₅₀₀; Cols. (8-10): gas mass, total mass and gas mass fraction at r₅₀₀.
Name n_e0 S_{0.2 r₅₀₀} $r_{\rm cen}$ $t_{\rm c}$ $r_{\rm cool}$ r₅₀₀ $M_{\rm gas, 500}$ M₅₀₀ $f_{\rm gas, 500}$

10^-3 cm^-3 keV cm² kpc Gyr r₅₀₀ Mpc $10^{14}~M_{\odot}$ $10^{14}~M_{\odot}$

Abell 68 $6.4 \pm 0.3$ $487 \pm 35$ 3.55 $6.6 \pm 0.2$ 0.10 1.21 $0.68 \pm 0.07$ $6.51 \pm 1.93$ $0.105 \pm 0.060$

Abell 209 $5.7 \pm 0.2$ $370 \pm 26$ 3.74 $6.4 \pm 0.3$ 0.14 1.15 $0.77 \pm 0.08$ $5.33 \pm 1.71$ $0.146 \pm 0.089$

Abell 267 $7.4 \pm 0.4$ $365 \pm 33$ 3.29 $4.9 \pm 0.4$ 0.15 1.06 $0.47 \pm 0.04$ $4.29 \pm 1.30$ $0.109 \pm 0.060$

Abell 383 $54.6 \pm 1.5$ $303 \pm 14$ 1.98 $0.5 \pm 0.2$ 0.16 0.98 $0.33 \pm 0.04$ $3.17 \pm 0.94$ $0.104 \pm 0.061$

Abell 773 $7.4 \pm 0.4$ $434 \pm 41$ 3.15 $5.7 \pm 0.5$ 0.14 1.33 $1.05 \pm 0.12$ $8.30 \pm 2.45$ $0.126 \pm 0.070$

Abell 963 $14.3 \pm 0.8$ $393 \pm 18$ 2.14 $2.6 \pm 0.2$ 0.14 1.14 $0.62 \pm 0.07$ $5.19 \pm 1.52$ $0.120 \pm 0.066$

Abell 1689 $30.1 \pm 0.9$ $505 \pm 25$ 1.95 $1.5 \pm 0.2$ 0.13 1.44 $1.05 \pm 0.14$ $10.26 \pm 2.96$ $0.102 \pm 0.060$

Abell 1763 $6.5 \pm 0.3$ $402 \pm 47$ 4.00 $6.1 \pm 0.5$ 0.13 1.12 $0.88 \pm 0.08$ $4.96 \pm 1.46$ $0.178 \pm 0.094$

Abell 1835 $60.8 \pm 1.2$ $334 \pm 20$ 2.50 $0.6 \pm 0.3$ 0.19 1.22 $1.14 \pm 0.11$ $6.62 \pm 1.94$ $0.172 \pm 0.092$

Abell 2218 $5.8 \pm 0.2$ $444 \pm 51$ 3.26 $8.0 \pm 0.5$ 0.12 1.07 $0.62 \pm 0.06$ $4.18 \pm 1.27$ $0.147 \pm 0.085$

Abell 2390 $40.1 \pm 1.6$ $486 \pm 34$ 2.31 $0.9 \pm 0.3$ 0.14 1.29 $1.21 \pm 0.16$ $7.67 \pm 2.28$ $0.158 \pm 0.095$

Abell 2667 $40.7 \pm 1.4$ $399 \pm 27$ 2.33 $0.8 \pm 0.3$ 0.15 1.19 $0.77 \pm 0.09$ $6.02 \pm 1.74$ $0.128 \pm 0.073$

Mean -- -- -- -- -- -- -- -- $0.13 \pm 0.01$

**Table 2:** Deduced properties of all 13 galaxy clusters. Column (1): cluster name; Col. (2): electron number density of the inner most radial bin; Col. (3): entropy at 0.2 r₅₀₀; Col. (4): inner most radial bin of the surface brightness profile; Col. (5): cooling time measured at $r_{\rm cen}$ ; Col. (6): cooling radius; Col. (7): r₅₀₀; Cols. (8-10): gas mass, total mass and gas mass fraction at r₅₀₀.
Name	n_e0	S_{0.2 r₅₀₀}	$r_{\rm cen}$	$t_{\rm c}$	$r_{\rm cool}$	r₅₀₀	$M_{\rm gas, 500}$	M₅₀₀	$f_{\rm gas, 500}$
10^-3 cm^-3	keV cm²	kpc	Gyr	r₅₀₀	Mpc	$10^{14}~M_{\odot}$	$10^{14}~M_{\odot}$
Abell 68	$6.4 \pm 0.3$	$487 \pm 35$	3.55	$6.6 \pm 0.2$	0.10	1.21	$0.68 \pm 0.07$	$6.51 \pm 1.93$	$0.105 \pm 0.060$
Abell 209	$5.7 \pm 0.2$	$370 \pm 26$	3.74	$6.4 \pm 0.3$	0.14	1.15	$0.77 \pm 0.08$	$5.33 \pm 1.71$	$0.146 \pm 0.089$
Abell 267	$7.4 \pm 0.4$	$365 \pm 33$	3.29	$4.9 \pm 0.4$	0.15	1.06	$0.47 \pm 0.04$	$4.29 \pm 1.30$	$0.109 \pm 0.060$
Abell 383	$54.6 \pm 1.5$	$303 \pm 14$	1.98	$0.5 \pm 0.2$	0.16	0.98	$0.33 \pm 0.04$	$3.17 \pm 0.94$	$0.104 \pm 0.061$
Abell 773	$7.4 \pm 0.4$	$434 \pm 41$	3.15	$5.7 \pm 0.5$	0.14	1.33	$1.05 \pm 0.12$	$8.30 \pm 2.45$	$0.126 \pm 0.070$
Abell 963	$14.3 \pm 0.8$	$393 \pm 18$	2.14	$2.6 \pm 0.2$	0.14	1.14	$0.62 \pm 0.07$	$5.19 \pm 1.52$	$0.120 \pm 0.066$
Abell 1689	$30.1 \pm 0.9$	$505 \pm 25$	1.95	$1.5 \pm 0.2$	0.13	1.44	$1.05 \pm 0.14$	$10.26 \pm 2.96$	$0.102 \pm 0.060$
Abell 1763	$6.5 \pm 0.3$	$402 \pm 47$	4.00	$6.1 \pm 0.5$	0.13	1.12	$0.88 \pm 0.08$	$4.96 \pm 1.46$	$0.178 \pm 0.094$
Abell 1835	$60.8 \pm 1.2$	$334 \pm 20$	2.50	$0.6 \pm 0.3$	0.19	1.22	$1.14 \pm 0.11$	$6.62 \pm 1.94$	$0.172 \pm 0.092$
Abell 2218	$5.8 \pm 0.2$	$444 \pm 51$	3.26	$8.0 \pm 0.5$	0.12	1.07	$0.62 \pm 0.06$	$4.18 \pm 1.27$	$0.147 \pm 0.085$
Abell 2390	$40.1 \pm 1.6$	$486 \pm 34$	2.31	$0.9 \pm 0.3$	0.14	1.29	$1.21 \pm 0.16$	$7.67 \pm 2.28$	$0.158 \pm 0.095$
Abell 2667	$40.7 \pm 1.4$	$399 \pm 27$	2.33	$0.8 \pm 0.3$	0.15	1.19	$0.77 \pm 0.09$	$6.02 \pm 1.74$	$0.128 \pm 0.073$
Mean	--	--	--	--	--	--	--	--	$0.13 \pm 0.01$

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