Table B.2: XSPEC best-fit parameters for the two brightest supersoft sources. (An asterisk indicates that we could not determine an error for that fit parameter.)
parameter No. 68 No. 96
     
model: wabs $_{\rm Gal}$ $\times$ wabs $\times$ blackbody
$n_{\rm H}~(\times 10^{21}$ cm-2) $\rm 1.4^{+1.4}_{-0.5}$ $\rm 4.7^{+2.3}_{-1.0}$
$T_{\rm bb}$ (keV) $\rm0.065^{+0.014}_{-0.013}$ $\rm0.058^{+0.032}_{-0.023}$
$K_{\rm bb}~(\times 10^{-6})$ $\rm 2.3^{+0.3}_{-0.4}$ $\rm 48^{+35}_{-25}$
$\chi_\nu^2$ (d.o.f.) 1.01 (7) 0.51 (5)
$L_{\rm {0.3-8}}~(\times 10^{38}$ erg s-1) $\rm0.9^{+3.4}_{-0.4}$ [>1]
model: wabs $_{\rm Gal}$ $\times$ wabs $\times$ raymond-smith
$n_{\rm H}~(\times 10^{21}$ cm-2) $\rm 1.9^{+1.5}_{-1.2}$ $\rm 4.5^{+150}_{-4.5}$
$T_{\rm rs}$ (keV) $\rm0.087^{+0.033}_{-0.027}$ $\rm0.082^{+0.007}_{-0.013}$
Z (metal ab.) $\rm0.01^{+0.04}_{-0.01}$ $\rm0.02^{+0.14}_{-0.02}$
$K_{\rm rs}~(\times 10^{-3})$ $\rm 7.7^{+8.0}_{-4.5}$ $\rm 59^{+*}_{-*}$
$\chi_\nu^2$ (d.o.f.) 1.08 (6) 0.41 (4)
$L_{\rm {0.3-8}}~(\times 10^{38}$ erg s-1) $\rm 2.0^{+10.2}_{-1.5}$ [>1]


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