**Table 2:** Best fit model parameters and inferred physical system parameters. Here C_F is the partial covering coefficient, F_3-100 the observed X-ray flux in the 3-100 keV band, F_0.1-100 the unabsorbed X-ray flux in the 0.1-100 keV band, both in 10^-11 erg cm^-2 s^-1 units. The distances for V405 Aur, V709 Cas, PQ Gem and V2400 Oph are assumed.
Name	$M_{\rm wd}$ ,	C_F	$N_{\rm H}$ ,	F_3-100	F_0.1- 100	$\dot M$	$L_{\rm x}$ , 10³³	d	$\chi^2$ (d.o.f.)
	$M_{\odot}$		10²² cm^-2			10¹⁶ g s^-1	erg s^-1	pc
V1223 Sgr	$0.95\pm0.05$	1.0^a	$3.7\pm1$	4.2	7.3	12.6	24.3	527¹	105.4(63)
		$0.57\pm0.05$	$28\pm3$
FO Aqr	$0.60\pm 0.05$	$0.9\pm0.1$	$36\pm4$	1.5	4.9	10.2	9.4	400²	62.1(65)
EX Hya	$0.50 \pm 0.05$	1.0	$0.6\pm1.0$	1.5	3.4	0.25	0.17	64.5³	85.3(65)
AO Psc	$0.65\pm0.05$	$0.95\pm0.1$	$10\pm5$	1.3	2.5	4.7	4.9	420⁴	55.8(65)
TVCol	$0.84\pm0.06$	$0.81\pm0.3$	$21\pm5$	1.7	3.5	3.4	5.7	368⁵	63.4(65)
GK Per	$0.59\pm0.05$	1.0^a	$20\pm2$	12.5	88.6	81.5	156	340⁶	110.5(63)
		$0.75\pm0.05$	$125\pm10$
V709 Cas	$0.90\pm0.10$	$0.5\pm 0.1$	$29\pm5$	2.3	3.7	5.76	11.1	(500)	56.3(65)
PQ Gem	$0.65\pm 0.2$	1.0	$5\pm1$	0.80	1.3	3.7	3.9	(500)	38.7(65)
V2400 Oph	$0.59\pm0.05$	$0.4\pm0.1$	$29\pm10$	2.43	5.6	18.7	16.75	(500)	78.5(65)
BG CMi	$0.85\pm0.12$	$0.70\pm0.05$	$25\pm6$	0.77	1.54	5.3	9.0	700⁷	57.4(65)
V405 Aur	$0.90\pm0.10$	$0.6\pm0.1$	$39\pm3$	0.9	1.7	2.65	5.09	(500)	51.6(65)
V1062 Tau	$1.00\pm0.20$	$0.6\pm0.1$	$21\pm7$	1.1	1.8	2.2	5.4	500⁸	45.6(65)
DO Dra	$0.75\pm0.05$	$0.4\pm0.1$	$20\pm5$	7.8	14.4	3.1	4.1	155⁹	69.7(65)
TX Col	$0.70\pm0.30$	<0.4	<60	0.32	0.58	1.8	2.1	550¹⁰	52.6(65)

^a - For the systems V1223 Sgr and GK Per which have very high mass accretion rates we used two absorbers.

References to distance estimates: 1. Beuermann et al. (2004); 2. McHardy et al. (1987); 3. Beuermann et al. (2003); 4. Hellier et al. (1991); 5. McArthur et al. (2001); 6. Warner (1987); 7. Berriman (1987); 8. Szkody & Silber (1996); 9. Mateo et al. (1991); 10. Buckley & Tuohy (1989).

	1 Introduction
	2 The model
	3 Observations and data reduction
	4 Results
	5 Conclusions
	References