Table 3: XSPEC best-fit parameters for the X-ray spectrum of XMMU J013636.5+155036 in 2002 February, from the combined XMM-Newton EPIC dataset. The foreground line-of-sight absorption column density $n_{\rm {H,~Gal}}$ has been fixed at $0.5 \times 10^{21}$ cm ^-2. See http://heasarc.gsfc.nasa.gov/docs/xanadu/xspec for a full description of the XSPEC spectral models.
model: wabs $_{\rm Gal}$ $\times$ wabs $\times$ power-law

$n_{\rm H}~(\times 10^{21}$ cm^-2) $\rm 1.3^{+0.6}_{-0.5}$

$\Gamma$ $\rm 1.91^{+0.21}_{-0.17}$

$K_{\rm pl}~(\times 10^{-5})$ $\rm 4.0^{+0.9}_{-0.7}$

$\chi_\nu^2$ (d.o.f.) 0.86 (36)

$L_{\rm {0.3-12}}~(\times 10^{39}$ erg s^-1) $\rm 1.6^{+0.1}_{-0.3}$

**Table 3:** XSPEC best-fit parameters for the X-ray spectrum of XMMU J013636.5+155036 in 2002 February, from the combined *XMM-Newton* EPIC dataset. The foreground line-of-sight absorption column density $n_{\rm {H,~Gal}}$ has been fixed at $0.5 \times 10^{21}$ cm ^-2. See http://heasarc.gsfc.nasa.gov/docs/xanadu/xspec for a full description of the XSPEC spectral models.
model: wabs $_{\rm Gal}$ $\times$ wabs $\times$ power-law
$n_{\rm H}~(\times 10^{21}$ cm^-2)	$\rm 1.3^{+0.6}_{-0.5}$
$\Gamma$	$\rm 1.91^{+0.21}_{-0.17}$
$K_{\rm pl}~(\times 10^{-5})$	$\rm 4.0^{+0.9}_{-0.7}$
$\chi_\nu^2$ (d.o.f.)	0.86 (36)
$L_{\rm {0.3-12}}~(\times 10^{39}$ erg s^-1)	$\rm 1.6^{+0.1}_{-0.3}$

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