Table 2: Spectroscopy of XB1832-330 with the same model adopted for the two observations (RGS1+RGS2+pn+MOS1+MOS2 data) consisting of a power-law model together with a blackbody, both equally absorbed by a variable absorption model, VPHABS in XSPEC.
Parameters Obs I Obs II

$N_{\rm H}$ (10²² cm^-2) $0.058 \pm{0.006}$ $0.094 \pm{0.006}$

$kT_{\rm bb}$ (keV) $0.62 \pm{0.01}$ $0.61 \pm{0.01}$

$R_{\rm bb}$ (km) $3.1 \pm{0.1}$ $3.5 \pm{0.1}$

$\Gamma$ $1.58 \pm{0.02}$ $1.52 \pm{0.02}$

Flux (10^-11 erg cm^-2 s^-1) 1.6 1.5

$L_{\rm X}$ (0.5-10 keV) (10³⁶ erg s^-1) 1.6 1.5

red. $\chi ^{2}$ (d.o.f.) 1.154 (2363) 1.044 (2712)

**Table 2:** Spectroscopy of XB1832-330 with the same model adopted for the two observations (RGS1+RGS2+pn+MOS1+MOS2 data) consisting of a power-law model together with a blackbody, both equally absorbed by a variable absorption model, VPHABS in XSPEC.
Parameters	Obs I	Obs II
$N_{\rm H}$ (10²² cm^-2)	$0.058 \pm{0.006}$	$0.094 \pm{0.006}$
$kT_{\rm bb}$ (keV)	$0.62 \pm{0.01}$	$0.61 \pm{0.01}$
$R_{\rm bb}$ (km)	$3.1 \pm{0.1}$	$3.5 \pm{0.1}$
$\Gamma$	$1.58 \pm{0.02}$	$1.52 \pm{0.02}$
Flux (10^-11 erg cm^-2 s^-1)	1.6	1.5
$L_{\rm X}$ (0.5-10 keV) (10³⁶ erg s^-1)	1.6	1.5
red. $\chi ^{2}$ (d.o.f.)	1.154 (2363)	1.044 (2712)

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