Broad-band properties of the hard X-ray cataclysmic variables IGR J00234+6141 and 1RXS J213344.1+510725

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Table 5:

Spectral parameters of the best-fit models to the average spectra of RX J2133. Errors are given at the $90\%$ confidence level.
		$N_{{\rm H}}$ ^a	$N_{{\rm H}}$ ^b	$C_{\rm F}$ ^c	$k T_{{\rm BB}}$	$C_{{\rm BB}}$ ^d	A_Z^e	$\alpha$ ^f	k T₁	C₁^g	k T₂	C₂^h	k T₃ⁱ	C₃^j	EW^k	$\chi_{\nu}^2$
					(eV)				(keV)		(keV)		(keV)		(eV)	( $\chi^2$ / d.o.f.)
	1	$1.7_{\rm -0.2}^{+0.1}$	$1.3_{\rm -0.1}^{+0.2}$	$0.56_{\rm -0.04}^{+0.03}$	$94_{\rm -2}^{+3}$	$5.8_{\rm -1.1}^{+0.8}$	$0.6_{\rm -0.1}^{+0.2}$	$0.9_{\rm -0.1}^{+0.2}$					$55_{\rm -15}^{+21}$	$3.5 \pm 0.4$	$159 \pm 22$	0.98 (1416/1444)
A	2	1.7 (fixed)	$1.1 \pm 0.2$	$0.58_{\rm -0.04}^{+0.03}$	$97_{\rm -1}^{+2}$	$4.9_{\rm -0.5}^{+0.4}$	$0.6_{\rm -0.1}^{+0.2}$	$0.9 \pm 0.2$					$45_{\rm -10}^{+23}$	$3.5 \pm 0.6$	$149_{\rm -31}^{+16}$	1.05 (819/780)
	3	1.7 (fixed)	$1.06 \pm 0.07$	$0.48_{\rm -0.02}^{+0.01}$	$102 \pm 1$	$3.7 \pm 0.2$	$0.8 \pm 0.1$	1 (fixed)					$82_{\rm -10}^{+13}$	$3.80_{\rm -0.08}^{+0.09}$	$181 \pm 10$	1.12 (2907/2608)
	1	$1.7_{\rm -0.08}^{+0.12}$	$1.4 \pm 0.2$	$0.52_{\rm -0.02}^{+0.04}$	$98 \pm 2$	$4.9_{\rm -0.6}^{+1.0}$	$0.5 \pm 0.1$				$1.4_{\rm -0.2}^{+0.4}$	$0.9_{\rm -0.3}^{+0.5}$	$27_{\rm -6}^{+4}$	$1.70_{\rm -0.07}^{+0.05}$	$168_{\rm -24}^{+23}$	0.99 (1431/1443)
B	2	1.7 (fixed)	$1.2 \pm 0.2$	$0.59 \pm 0.04$	$103 \pm 2$	$4.3_{\rm -0.4}^{+0.5}$	$0.7_{\rm -0.2}^{+0.3}$				$4.6_{\rm -1.0}^{+1.9}$	$5.1_{\rm -1.7}^{+1.9}$	$36_{\rm -8}^{+13}$	$1.3 \pm 0.2$	$140 \pm 30$	1.06 (822/779)
	3	1.7 (fixed)	$1.03 \pm 0.07$	$0.46_{\rm -0.01}^{+0.02}$	$107 \pm 1$	$3.1 \pm 0.1$	$0.9_{\rm -0.1}^{+0.2}$				$7.3_{\rm -1.1}^{+0.6}$	$3.6_{\rm -0.9}^{+0.8}$	> 71	$1.46_{\rm -0.06}^{+0.07}$	$173 \pm 9$	1.08 (2818/2606)
	1	$1.7 \pm 0.1$	$1.3 \pm 0.2$	$0.54 \pm 0.03$	$96_{\rm -2}^{+3}$	$5.4_{\rm -0.9}^{+0.8}$	$0.7 \pm 0.2$		$1.1_{\rm -0.2}^{+0.3}$	$4.1_{\rm -1.7}^{+3.3}$	$4.8_{\rm -0.9}^{+3.2}$	$3.3_{\rm -0.5}^{+1.5}$	$39_{\rm -9}^{+11}$	$1.46_{\rm -0.18}^{+0.09}$	$156_{\rm -21}^{+22}$	0.97 (1403/1441)
C	2	1.7 (fixed)	$1.1 \pm 0.2$	$0.57 \pm 0.04$	$99 \pm 2$	$4.7 \pm 0.5$	$0.7_{\rm -0.2}^{+0.3}$		$1.0_{\rm -0.2}^{+0.3}$	$4.5_{\rm -2.3}^{+3.6}$	5.4_1.4^+1.7	$4.7_{\rm -1.7}^{+2.4}$	$39_{\rm -8}^{+12}$	$1.3_{\rm -0.2}^{+0.1}$	$142_{\rm -30}^{+31}$	1.04 (805/777)
	3	1.7 (fixed)	$1.10 \pm 0.09$	$0.45_{\rm -0.02}^{+0.01}$	$100_{\rm -3}^{+2}$	$4.7_{\rm -0.8}^{+1.0}$	$0.9_{\rm -0.1}^{+0.2}$		$0.9_{\rm -0.1}^{+0.2}$	$1.6_{\rm -0.6}^{+0.9}$	$6.6 \pm 1.0$	$3.5_{\rm -0.9}^{+1.0}$	> 61	$1.50_{\rm -0.05}^{+0.07}$	$170 \pm 9$	1.07 (2794/2603)

^a Column density of the total absorber in units of $10^{21}~{\rm cm}^{-2}$ ; ^b column density of the partial absorber in units of $10^{23}~{\rm cm}^{-2}$ ; ^c covering fraction of the partial absorber; ^d normalization constant of the BBODY component in units of 10^-4; ^e metal abundance; ^f index of power-law emissivity function of the CEMEKL component; ^g normalization constant of the first optically thin plasma component in units of 10^-4; ^h normalization constant of the second optically thin plasma component in units of 10^-3; ⁱ in model A this the maximum temperature of the CEMEKL; ^j normalization constant of the third optically thin plasma component (CEMEKL in model A) in units of 10^-2; ^k equivalent width of the 6.4 keV Fe line.

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