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Home All issues Volume 504 / No 1 (September II 2009) A&A, 504 1 (2009) 185-197 Full HTML
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Table 6:

X-ray spectral analysis of the INS candidates (excluding XMM J1046).

Candidate		 OBSID $t_{\rm exp}$a d.o.f. kT $f_{\rm X,14}$b C Goodnessc $\Gamma$ $f_{\rm X,14}$ C Goodness
    (ks)   (eV) (erg s-1 cm-2)   (%)   (erg s-1 cm-2)   (%)
XMM J1210 204710101 2.1 22 $\rm 253^{+53}_{-40}$ $\rm 3.6^{+0.8}_{-0.7}$ 14 4.6 2.0(4) $\rm 4.6^{+1.0}_{-0.9}$ 17 9.9
XMM J0106 150870201 1.7 5 $\rm 247^{+116}_{-60}$ $\rm 2.6^{+0.9}_{-0.7}$ 5 18.4 1.5(8) $\rm 4.6^{+1.4}_{-1.3}$ 5 19.8
XMM J0435 307001301 7.3 24 $\rm 200^{+29}_{-24}$ $\rm 2.00^{+0.3}_{-0.29}$ 22 26.8 2.4(4) 2.8(4) 21 22.7
XMM J0314 201750901 11.6 17 $\rm 229^{+58}_{-44}$ 1.7(3) 24 76.7 2.1(4) 2.5(5) 21 60.0
XMM J2140 008830101 10.5 15 $\rm 144^{+14}_{-12}$ $\rm 2.00^{+0.22}_{-0.24}$ 17 58.5 $\rm 2.94^{+0.24}_{-0.23}$ $\rm 2.59^{+0.3}_{-0.25}$ 9 6.8
XMM J1259 203020101 9.8 26 $\rm 176^{+21}_{-18}$ $\rm 2.15^{+0.26}_{-0.25}$ 44 96.7 $\rm 2.43^{+0.23}_{-0.22}$ 3.1(3) 35 79.4
XMM J1250 303561001 7.8 11 $\rm 186^{+34}_{-27}$ $\rm 1.30^{+0.26}_{-0.24}$ 6 6.7 2.6(4) 1.7(3) 6 7.0
a Exposure times are filtered for background flares.
b Observed flux refers to range 0.15-3 keV in units of 10-14 erg s-1 cm-2.
c The ``goodness-of-fit'' is derived from a number of 1000 Monte Carlo simulated spectra.

Source LaTeX | All tables | In the text

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