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Table 4

Fits to the X-ray spectra described in the text.

Spectrum apec kT1 apec kT2 NH Flux abs. Flux unabs. Luminosity C-stat F-test
(keV) (keV) (1020 cm−2) (10−12 erg s−1 cm−2) (erg s−1) prob.
Sall 6.8 2.9 538/555
7.1 0.19 5.5 532/553 95.5
So,high 8.1 4.1 3.78 3.96 3.58 × 1031 380/430
8.5 0.22 9.2 3.82 4.29 3.88 × 1031 371/428 99.4
So,low 6.6 <3.2 2.17 2.20 1.99 × 1031 300/361
6.5 0.15 5.2 2.20 2.39 2.17 × 1031 296/359 91.0
SA 8.1 <4.7 2.72 ± 0.26 2.72 ± 0.26 2.46 × 1031 311/342
6.5 0.14 9.4 2.67 3.12 2.83 × 1031 306/340 93.6
SB 4.5 <1.6 1.40 1.40 1.26 × 1031 128/153
4.2 0.07 <35 1.46 3.7 3.36 × 1031 123/151 95.1
Sd 5.3 5.4 1.12 1.20 1.08 × 1031 291/322
5.3 Unconst. 5.8 1.11 1.19 1.08 × 1031 290/320 42.4
Sq >3.7 <9.3 0.43 0.44 4.01 × 1030 71/102
SGW,q 3.5 <8.9 0.50 0.53 6.91 × 1029 135/193

Notes. Single and double apec models were fitted to each spectrum. The absorbed and unabsorbed fluxes and unabsorbed luminosities are given in the 0.3–10 keV range. The luminosity is calculated for the assumed distance of 275 pc for SSS J122222 (Paper I) and 104 pc for GW Lib (Byckling et al. 2009). The final column gives the probability of improving the fit by including the second temperature component via the F-test.

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