**Table 2:** Summary of the luminosity from representative regions in RX J1713.7-3946
Region	Area	$\Gamma$	$N_{\rm H}$	$F_{{\rm 1-10~keV}}$	$L_{\rm X}$
	(arcmin²)		$(10^{22}~{\rm cm}^{-2})$	${\rm (erg~s^{-1}~cm^{-2})}$	${\rm (erg~s^{-1})}$
NWb	125	$2.28\pm0.02$	$0.72\pm0.01$	$7.3\times 10^{-11}$	$8.7\times10^{33}d_{1}^{2}$
NWd	64	$2.12\pm0.04$	$0.68\pm0.02$	$2.8\times 10^{-11}$	$3.4\times10^{33}d_{1}^{2}$
SWb	125	$2.38\pm0.03$	$0.83\pm0.01$	$6.2\times 10^{-11}$	$7.4\times10^{33}d_{1}^{2}$
SWd	77	$2.54\pm0.04$	$0.68\pm0.02$	$1.9\times 10^{-11}$	$2.3\times10^{33}d_{1}^{2}$
Interior	500	2.39^a	0.46^a	$5.4\times 10^{-11}$	$6.5\times10^{33}d_{1}^{2}$

Note. $F_{{\rm 1-10~keV}}$ is the unabsorbed flux in the 1-10 keV band; d₁ is the distance to the source
normalized to 1 kpc; ^a average values with totally 20 squires of 5 $^\prime$ $\times~$ 5 $^\prime$ .

Source LaTeX | All tables | In the text

	1 Introduction
	2 Observation and data reduction
	3 Analysis and results
	4 Discussion
	5 Conclusion
	References