\begin{table}%t1
%\centering
\par
\caption{Best-fit results of the spectral and spatial analysis
of the sample of galaxy clusters at redshift $>$0.4 and derived
quantities at an overdensity corresponding to $\Delta_z=500$
in a Einstein-de Sitter universe.
A Hubble constant of 70~km~s$^{-1}$~Mpc$^{-1}$ in a flat universe
with~$\Omega_{\rm m}$ equals to~0.3 is assumed.
Note: (i) RX~J1347--1145 has a clear hot enhancement to the South--East of the
main X-ray emission. A sector with position angle $90^{\circ}{-}180^{\circ}$ 
and centered
on the X-ray peak has been masked in accordance with the analysis presented in 
Allen et~al. (\cite{Allen02}). (ii) In~3C~295, the central active galactic 
nucleus and regions of enhanced emission associated to the radio lobes 
have been masked (see Allen et~al. \cite{Allen01}a). 
(iii) MS1054--0321 presents significant substructure (e.g. Jeltema et~al. 
\cite{Jeltema01}). The temperature and the best-fit of the surface brightness profile are 
estimated from the main body of the cluster once a circular region centered at 
(RA, Dec; 2000)~=~$(10^{\rm h} 56^{\rm m} 55\arcsec7,-3^{\circ} 37' 37'')$ 
and with radius of 36 arcsec is masked.
\label{tab:obj_a}}
 \begin{tabular}{l@{\hspace{.7em}} c@{\hspace{.7em}} c@{\hspace{.7em}} c@{\hspace{.7em}} c@{\hspace{.7em}} c@{\hspace{.7em}} c@{\hspace{.7em}} c@{\hspace{.7em}} c@{\hspace{.7em}} c@{\hspace{.7em}} c@{\hspace{.7em}} c@{\hspace{.7em}}}
\hline\hline  
cluster & $z$ & $1'$ & $R_{\rm spec}$ & $R_{2 \sigma}$ & $T_{\rm gas}$ & 
$r_{\rm c}$ & $\beta$ & $R_{500}$ & $L_{\rm bol}$ & $M_{\rm gas}$ & $M_{\rm tot}$ \\ 
  & & kpc & kpc & kpc & keV & kpc &  & kpc & $10^{44}$ erg s$^{-1}$ & $10^{13}~ M_{\odot}$ & $10^{14}~ M_{\odot}$  \\ 
\hline 
RX~J1416+4446 & 0.400 & $322$ & $397$ & $1088$ & $\rm 3.7_{-0.3}^{+0.2}$ & $26(\pm 4)$ & $0.438(\pm 0.012)$ & $749(\pm 26)$ & $5.43(\pm 0.19)$ & $2.84(\pm 0.47)$ & $1.35(\pm 0.14)$ \\ 
MS0302+1658 & 0.424 & $334$ & $274$ & $552$ & $\rm 3.8_{-0.2}^{+0.9}$ & $64(\pm 10)$ & $0.630(\pm 0.036)$ & $899(\pm 65)$ & $6.41(\pm 0.19)$ & $3.26(\pm 0.48)$ & $2.43(\pm 0.55)$ \\ 
MS1621+2640 & 0.426 & $335$ & $659$ & $1276$ & $\rm 6.8_{-0.5}^{+0.9}$ & $185(\pm 19)$ & $0.563(\pm 0.040)$ & $1119(\pm 74)$ & $10.92(\pm 0.30)$ & $7.18(\pm 0.76)$ & $4.70(\pm 0.94)$ \\ 
RX~J1347--1145 & 0.451 & $346$ & $533$ & $1430$ & $\rm 10.3_{-0.5}^{+0.6}$ & $38(\pm 1)$ & $0.571(\pm 0.004)$ & $1368(\pm 40)$ & $116.75(\pm 0.58)$ & $18.06(\pm 0.80)$ & $8.94(\pm 0.80)$ \\ 
RX~J1701+6421 & 0.453 & $347$ & $370$ & $889$ & $\rm 4.5_{-0.2}^{+0.4}$ & $13(\pm 2)$ & $0.396(\pm 0.007)$ & $750(\pm 24)$ & $6.42(\pm 0.58)$ & $3.36(\pm 0.45)$ & $1.48(\pm 0.15)$ \\ 
3C~295 & 0.460 & $350$ & $172$ & $895$ & $\rm 4.3_{-0.2}^{+0.3}$ & $31(\pm 2)$ & $0.553(\pm 0.007)$ & $870(\pm 26)$ & $14.07(\pm 0.19)$ & $4.35(\pm 0.29)$ & $2.33(\pm 0.21)$ \\ 
RX~J1525+0957 & 0.516 & $372$ & $372$ & $973$ & $\rm 5.1_{-0.5}^{+0.5}$ & $229(\pm 30)$ & $0.644(\pm 0.054)$ & $941(\pm 60)$ & $6.92(\pm 0.19)$ & $4.74(\pm 0.62)$ & $3.23(\pm 0.62)$ \\ 
MS0451--0305 & 0.539 & $381$ & $625$ & $1391$ & $\rm 8.0_{-0.3}^{+0.3}$ & $201(\pm 6)$ & $0.734(\pm 0.015)$ & $1263(\pm 30)$ & $50.94(\pm 8.05)$ & $14.15(\pm 0.47)$ & $8.09(\pm 0.59)$ \\ 
MS0016+1609 & 0.541 & $382$ & $626$ & $1770$ & $\rm 10.0_{-0.5}^{+0.5}$ & $237(\pm 8)$ & $0.685(\pm 0.013)$ & $1355(\pm 35)$ & $53.27(\pm 7.33)$ & $17.13(\pm 0.66)$ & $10.02(\pm 0.78)$ \\ 
RX~J1121+2326 & 0.562 & $389$ & $446$ & $702$ & $\rm 4.6_{-0.3}^{+0.5}$ & $427(\pm 85)$ & $1.180(\pm 0.276)$ & $1132(\pm 128)$ & $5.45(\pm 0.22)$ & $4.60(\pm 0.39)$ & $6.04(\pm 2.12)$ \\ 
RX~J0848+4456 & 0.570 & $391$ & $196$ & $401$ & $\rm 3.2_{-0.3}^{+0.3}$ & $97(\pm 14)$ & $0.620(\pm 0.050)$ & $723(\pm 45)$ & $1.21(\pm 0.37)$ & $1.23(\pm 0.14)$ & $1.59(\pm 0.30)$ \\ 
MS2053--0449 & 0.583 & $396$ & $357$ & $730$ & $\rm 5.5_{-0.5}^{+0.5}$ & $99(\pm 11)$ & $0.610(\pm 0.033)$ & $931(\pm 47)$ & $5.40(\pm 1.04)$ & $3.41(\pm 0.35)$ & $3.47(\pm 0.52)$ \\ 
RX~J0542--4100 & 0.634 & $411$ & $540$ & $1198$ & $\rm 7.9_{-0.8}^{+1.0}$ & $132(\pm 17)$ & $0.514(\pm 0.031)$ & $982(\pm 63)$ & $12.15(\pm 1.36)$ & $6.27(\pm 0.82)$ & $4.41(\pm 0.85)$ \\ 
RX~J1221+4918 & 0.700 & $429$ & $563$ & $972$ & $\rm 7.5_{-0.6}^{+0.7}$ & $263(\pm 22)$ & $0.734(\pm 0.047)$ & $1063(\pm 57)$ & $12.95(\pm 0.39)$ & $6.80(\pm 0.59)$ & $6.16(\pm 1.00)$ \\ 
RX~J1113--2615 & 0.730 & $436$ & $286$ & $371$ & $\rm 5.6_{-0.6}^{+0.8}$ & $89(\pm 13)$ & $0.639(\pm 0.049)$ & $866(\pm 62)$ & $4.43(\pm 0.77)$ & $2.49(\pm 0.31)$ & $3.47(\pm 0.75)$ \\ 
RX~J2302+0844 & 0.734 & $437$ & $358$ & $635$ & $\rm 6.6_{-0.6}^{+1.5}$ & $96(\pm 12)$ & $0.546(\pm 0.033)$ & $865(\pm 65)$ & $5.45(\pm 0.17)$ & $3.38(\pm 0.48)$ & $3.48(\pm 0.82)$ \\ 
MS1137+6625 & 0.782 & $447$ & $367$ & $635$ & $\rm 6.9_{-0.5}^{+0.5}$ & $111(\pm 6)$ & $0.705(\pm 0.022)$ & $964(\pm 39)$ & $15.30(\pm 0.44)$ & $4.90(\pm 0.29)$ & $5.18(\pm 0.63)$ \\ 
RX~J1317+2911 & 0.805 & $451$ & $185$ & $238$ & $\rm 4.1_{-0.8}^{+1.2}$ & $50(\pm 12)$ & $0.518(\pm 0.048)$ & $634(\pm 83)$ & $1.12(\pm 0.08)$ & $0.98(\pm 0.29)$ & $1.52(\pm 0.61)$ \\ 
RX~J1350+6007 & 0.810 & $452$ & $519$ & $801$ & $\rm 4.6_{-0.9}^{+0.7}$ & $106(\pm 37)$ & $0.479(\pm 0.056)$ & $627(\pm 65)$ & $4.41(\pm 0.39)$ & $2.24(\pm 0.79)$ & $1.48(\pm 0.46)$ \\ 
RX~J1716+6708 & 0.813 & $453$ & $371$ & $640$ & $\rm 6.8_{-0.6}^{+1.0}$ & $121(\pm 16)$ & $0.635(\pm 0.038)$ & $896(\pm 56)$ & $13.86(\pm 1.04)$ & $4.87(\pm 0.61)$ & $4.35(\pm 0.83)$ \\ 
MS1054--0321 & 0.830 & $456$ & $628$ & $900$ & $\rm 10.2_{-0.8}^{+1.0}$ & $511(\pm 36)$ & $1.375(\pm 0.124)$ & $1509(\pm 93)$ & $28.48(\pm 2.96)$ & $10.61(\pm 0.44)$ & $21.27(\pm 3.96)$ \\ 
RX~J0152--1357S & 0.830 & $456$ & $400$ & $607$ & $\rm 6.9_{-0.8}^{+2.9}$ & $96(\pm 19)$ & $0.532(\pm 0.046)$ & $824(\pm 109)$ & $7.73(\pm 0.40)$ & $3.91(\pm 0.94)$ & $3.47(\pm 1.49)$ \\ 
RX~J0152--1357N & 0.835 & $457$ & $427$ & $919$ & $\rm 6.0_{-0.7}^{+1.1}$ & $157(\pm 36)$ & $0.542(\pm 0.067)$ & $753(\pm 72)$ & $10.67(\pm 0.67)$ & $4.49(\pm 1.01)$ & $2.66(\pm 0.77)$ \\ 
WGA1226+3333 & 0.890 & $466$ & $459$ & $711$ & $\rm 11.2_{-1.5}^{+2.2}$ & $123(\pm 13)$ & $0.692(\pm 0.037)$ & $1134(\pm 95)$ & $54.63(\pm 0.83)$ & $10.54(\pm 1.33)$ & $9.80(\pm 2.55)$ \\ 
RX~J0910+5422 & 1.106 & $491$ & $201$ & $273$ & $\rm 6.6_{-1.3}^{+1.7}$ & $147(\pm 53)$ & $0.843(\pm 0.268)$ & $818(\pm 150)$ & $2.83(\pm 0.35)$ & $1.56(\pm 0.30)$ & $4.91(\pm 2.93)$ \\ 
RX~J1252--2927 & 1.235 & $500$ & $492$ & $440$ & $\rm 5.2_{-0.7}^{+0.7}$ & $77(\pm 13)$ & $0.525(\pm 0.034)$ & $532(\pm 40)$ & $5.99(\pm 1.10)$ & $1.81(\pm 0.34)$ & $1.59(\pm 0.35)$ \\ 
RX~J0849+4452 & 1.260 & $501$ & $197$ & $275$ & $\rm 5.2_{-1.1}^{+1.6}$ & $128(\pm 40)$ & $0.773(\pm 0.189)$ & $640(\pm 106)$ & $2.83(\pm 0.17)$ & $1.38(\pm 0.30)$ & $2.85(\pm 1.48)$ \\ 
RX~J0848+4453 & 1.270 & $501$ & $164$ & $173$ & $\rm 2.9_{-0.8}^{+0.8}$ & $163(\pm 70)$ & $0.972(\pm 0.431)$ & $499(\pm 115)$ & $1.04(\pm 0.73)$ & $0.56(\pm 0.21)$ & $1.37(\pm 0.98)$ \\ 
\hline 
\end{tabular}
\end{table}