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Table 4:

The same as Table 3, but for the spectrum of IGR J08408-4503 obtained by using the total available exposure time of the XMM-Newton observation.

Model 		BB+CUTOFFPL MKL+CUTOFFPL BMC

$N_{\rm H}$ (1022 cm-2) 		$\rm0.9^{+0.2}_{-0.1}$ $\rm0.7^{+0.1}_{-0.2}$ $\rm 1.0^{+0.1}_{-0.2}$

$\Gamma$ 		1.6 $\pm$ 0.1 1.4 $\pm$ 0.1 2.0 $\pm$ 0.1

$kT_{\rm BB}$(keV) 		$\rm0.082^{+0.007}_{-0.004}$ -- --

$R_{\rm BB}$a (km) 		$\rm 100^{+126}_{-47}$ -- --

$kT_{\rm MKL}$(keV) 		-- $\rm0.22^{+0.04}_{-0.02}$ --

$N_{\rm MKL}$(10-3) 		-- $\rm 1.3_{-0.8}^{+1.1}$ --

$kT_{\rm BMC}$(keV) 		-- -- $\rm0.075^{+0.007}_{-0.006}$

$\log(A)$ 		-- -- $\rm --2.5^{+0.3}_{-0.2}$

$N_{\rm BMC}$ (10-3) 		-- -- $\rm 2.0^{+2.8}_{-1.3}$

$F_{\rm0.5{-}1.5~keV}$b 		$\rm 1.2_{-0.8}^{+0.1}$ $\rm 1.2_{-0.7}^{+0.1}$ $\rm 1.2_{-0.8}^{+0.2}$

$F_{\rm 1.5{-}10~keV}$b 		$\rm 6.3_{-1.4}^{+0.7}$ $\rm 6.3_{-1.0}^{+0.7}$ $\rm 6.4_{-3.7}^{+0.9}$

$F_{\rm0.5{-}10~keV}$b 		$\rm 7.5_{-2.1}^{+0.6}$ $\rm 7.5_{-1.5}^{+0.8}$ $\rm 7.5_{-4.0}^{+1.1}$

$\chi^2_{\rm red}$/d.o.f. 		0.99/99 1.05/99 1.02/99

EXP. (ks)c 		26 26 26

Notes.  (a) For a distance of 3 kpc. (b) Observed flux in units of 10-13 erg cm-2 s-1. (c) Exposure time.


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