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Table 3

Solar abundances model: tbabs× phabs× ∑ vapec.

Name NHlocal $\[\mathrm{N}_{\mathrm{H}}^{\text {local }}\]$ (1022 cm−2) kT (keV) Norm χν2$\[\chi_\nu^2\]$ or Prob (χ2/dof) FX[ FXISMcor]$\[\mathrm{F}_X\left[\mathrm{~F}_{\mathrm{X}}^{\mathrm{ISMcor}}\right]\]$ (erg cm−2 s−1) LX[ LXISMcor ]$\[\mathrm{L}_X\left[\mathrm{~L}_{\mathrm{X}}^{\text {ISMcor }}\right]\]$ (erg s−1)
A 4.18−0.49+0.51$\[4.18_{-0.49}^{+0.51}\]$ 0.11−0.01+0.02$\[0.11_{-0.01}^{+0.02}\]$ (0.08−0.07+0.25$\[0.08_{-0.07}^{+0.25}\]$)e2 1.05(296.39/283) (1.68−0.1+0.01$\[1.68_{-0.1}^{+0.01}\]$[2.51])e−13 (3.59−0.22+0.02$\[3.59_{-0.22}^{+0.02}\]$[5.37])e32
0.76−0.09+0.06$\[0.76_{-0.09}^{+0.06}\]$ (1.94−0.42+0.69$\[1.94_{-0.42}^{+0.69}\]$)e−3
3.8−1.0+1.1$\[3.8_{-1.0}^{+1.1}\]$ (1.57−0.36+0.84$\[1.57_{-0.36}^{+0.84}\]$)e−4
B 3.14−0.38+0.49$\[3.14_{-0.38}^{+0.49}\]$ 0.77−0.12+0.11$\[0.77_{-0.12}^{+0.11}\]$ (3.4−0.92+1.89$\[3.4_{-0.92}^{+1.89}\]$)e−4 1.11(162.61/146) (5.81−0.44+0.03$\[5.81_{-0.44}^{+0.03}\]$[7.92])e−14 (1.24−0.09+0.01$\[1.24_{-0.09}^{+0.01}\]$[1.7])e32
5.3−1.2+1.7$\[5.3_{-1.2}^{+1.7}\]$ (5.7−1.0+1.5$\[5.7_{-1.0}^{+1.5}\]$)e−5
U (a) 1.88−0.36+0.51$\[1.88_{-0.36}^{+0.51}\]$ 0.66−0.16+0.3$\[0.66_{-0.16}^{+0.3}\]$ (2.33−0.82+2.32$\[2.33_{-0.82}^{+2.32}\]$)e−4 1.05(102.76/98) (3.07−0.42+0.01$\[3.07_{-0.42}^{+0.01}\]$[5.65])e−14 (6.58−0.9+0.02$\[6.58_{-0.9}^{+0.02}\]$[12.09])e31
2.53−0.53+2.53$\[2.53_{-0.53}^{+2.53}\]$ (0.4−0.24+0.21$\[0.4_{-0.24}^{+0.21}\]$)e−4
L 2.96−0.95+1.62$\[2.96_{-0.95}^{+1.62}\]$ 0.53−0.25+0.47$\[0.53_{-0.25}^{+0.47}\]$ (18−13+235$\[18_{-13}^{+235}\]$)e−5 0.90(59.99/67) (2.18−0.56+0.01$\[2.18_{-0.56}^{+0.01}\]$[3.1])e−14 (4.66−1.2+0.02$\[4.66_{-1.2}^{+0.02}\]$[6.63])e31
2.49−0.54+1.61$\[2.49_{-0.54}^{+1.61}\]$ (0.47−0.24+0.16$\[0.47_{-0.24}^{+0.16}\]$)e−4
F(b) 6.7−2.3+3.7$\[6.7_{-2.3}^{+3.7}\]$ 0.08−0.03+0.07$\[0.08_{-0.03}^{+0.07}\]$ (0.92−0.92+592.67$\[0.92_{-0.92}^{+592.67}\]$)e2 1.19(54.73/46) (3.23−0.75+0.01$\[3.23_{-0.75}^{+0.01}\]$[3.77])e−14 (6.91−1.6+0.02$\[6.91_{-1.6}^{+0.02}\]$[8.08])e31
0.62−0.4+0.82$\[0.62_{-0.4}^{+0.82}\]$ (15−13+376$\[15_{-13}^{+376}\]$)e−5
5.7−2.2+3.2$\[5.7_{-2.2}^{+3.2}\]$ (4.26−0.99+2.48$\[4.26_{-0.99}^{+2.48}\]$)e−5
O(c) 1.58−0.98+1.37$\[1.58_{-0.98}^{+1.37}\]$ 0.53−0.15+0.2$\[0.53_{-0.15}^{+0.2}\]$ (4.5−3.3+16.7$\[4.5_{-3.3}^{+16.7}\]$)e−5 0.94(18.78/20) (1.03−0.89+0.25$\[1.03_{-0.89}^{+0.25}\]$[1.6])e−14 (2.21−1.9+0.53$\[2.21_{-1.9}^{+0.53}\]$[3.43])e31
>9.2 (8.0−2.1+1.5$\[8.0_{-2.1}^{+1.5}\]$)e−6
*N 20.3−5.6+4.7$\[20.3_{-5.6}^{+4.7}\]$ 0.1−0.03+0.04$\[0.1_{-0.03}^{+0.04}\]$ (27−27+1040$\[27_{-27}^{+1040}\]$)e2 0.1(79.85/65) (1.4−0.71+0.01$\[1.4_{-0.71}^{+0.01}\]$[1.53])e−14 (2.99−1.52+0.02$\[2.99_{-1.52}^{+0.02}\]$[3.29])e31
2.17−0.58+1.08$\[2.17_{-0.58}^{+1.08}\]$ (1.06−0.56+0.86$\[1.06_{-0.56}^{+0.86}\]$)e−4
*W 21.5−7.8+17.9$\[21.5_{-7.8}^{+17.9}\]$ 0.25±0.1 (8.7−8.5+219.4$\[8.7_{-8.5}^{+219.4}\]$)e−2 0.25(48.78/43) (0.97−0.58+0.01$\[0.97_{-0.58}^{+0.01}\]$[1.06])e−14 (2.08−1.24+0.02$\[2.08_{-1.24}^{+0.02}\]$[2.28])e31
4.6−2.6+3.2$\[4.6_{-2.6}^{+3.2}\]$ (0.27−0.1+0.65$\[0.27_{-0.1}^{+0.65}\]$)e−4
*J 6.8−3.9+10.7$\[6.8_{-3.9}^{+10.7}\]$ 0.18−0.16+0.31$\[0.18_{-0.16}^{+0.31}\]$ (7.5−7.5+396.9$\[7.5_{-7.5}^{+396.9}\]$)e−3 0.06(58.54/43) (6.68−3.54+0.10$\[6.68_{-3.54}^{+0.10}\]$[7.67])e−15 (1.43−0.76+0.02$\[1.43_{-0.76}^{+0.02}\]$[1.64])e31
5.4−3.4+6.2$\[5.4_{-3.4}^{+6.2}\]$ (1.1−0.35+3.69$\[1.1_{-0.35}^{+3.69}\]$)e−5
*R(d) 15.7−7.5+10.3$\[15.7_{-7.5}^{+10.3}\]$ 0.28−0.13+0.23$\[0.28_{-0.13}^{+0.23}\]$ (1.2−1.2+21.8$\[1.2_{-1.2}^{+21.8}\]$)e−2 0.8(27.89/35) (6.14−5.31+0.10$\[6.14_{-5.31}^{+0.10}\]$[6.9])e−15 (1.31−1.14+0.02$\[1.31_{-1.14}^{+0.02}\]$[1.48])e31
3.3−1.5+3.9$\[3.3_{-1.5}^{+3.9}\]$ (1.22−0.70+2.43$\[1.22_{-0.70}^{+2.43}\]$)e−5
*X 6.0−2.3+3.2$\[6.0_{-2.3}^{+3.2}\]$ >3.4 (8.1−2.1+6.0$\[8.1_{-2.1}^{+6.0}\]$)e−6 0.77(23.96/30) (5.52−2.22+0.16$\[5.52_{-2.22}^{+0.16}\]$[6.11])e−15 (11.82−4.75+0.34$\[11.82_{-4.75}^{+0.34}\]$[13.09])e30
*G(e) 44 3.96−0.93+1.92$\[3.96_{-0.93}^{+1.92}\]$ (3.6±1.0)e−5 0.02(47.71/30) (6.31−1.19+0.28$\[6.31_{-1.19}^{+0.28}\]$[8.0])e−15 (1.35−0.26+0.06$\[1.35_{-0.26}^{+0.06}\]$[1.71])e31
*P 32−11+24$\[32_{-11}^{+24}\]$ 4.1−2.5+5.0$\[4.1_{-2.5}^{+5.0}\]$ (2.0−1.0+9.4$\[2.0_{-1.0}^{+9.4}\]$)e−5 0.12(23.8/17) (4.66−4.66+0.01$\[4.66_{-4.66}^{+0.01}\]$[4.88])e−15 (9.98−9.98+0.02$\[9.98_{-9.98}^{+0.02}\]$[10.44])e30
*I 35−11+12$\[35_{-11}^{+12}\]$ 0.1−0.04+0.03$\[0.1_{-0.04}^{+0.03}\]$ (3.4−3.4+117.6$\[3.4_{-3.4}^{+117.6}\]$)e4 0.15(19.45/14) (3.53−3.39+0.01$\[3.53_{-3.39}^{+0.01}\]$[3.78])e−15 (7.56−7.26+0.02$\[7.56_{-7.26}^{+0.02}\]$[8.09])e30
5.1−2.7+6.4$\[5.1_{-2.7}^{+6.4}\]$ (0.13−0.05+0.22$\[0.13_{-0.05}^{+0.22}\]$)e−4
*Q 8.4−3.6+5.3$\[8.4_{-3.6}^{+5.3}\]$ >2.7 (6.9−2.7+8.0$\[6.9_{-2.7}^{+8.0}\]$)e−6 0.28(17.69/15) (3.8−3.25+0.02$\[3.8_{-3.25}^{+0.02}\]$[4.16])e−15 (8.14−6.97+0.04$\[8.14_{-6.97}^{+0.04}\]$[8.9])e30
*D 62−41+29$\[62_{-41}^{+29}\]$ >1.0 (2.2−2.2+10$\[2.2_{-2.2}^{+10}\]$)e−4 0.73(10.47/14) (2.75−2.75+0.01$\[2.75_{-2.75}^{+0.01}\]$[2.88])e−15 (5.89−5.89+0.02$\[5.89_{-5.89}^{+0.02}\]$[6.16])e30
*V 99−27+43$\[99_{-27}^{+43}\]$ 0.1 (16−16+718$\[16_{-16}^{+718}\]$)e8 0.54(10.82/12) (5.01−4.95+0.01$\[5.01_{-4.95}^{+0.01}\]$[5.23])e−15 (10.73−10.59+0.02$\[10.73_{-10.59}^{+0.02}\]$[11.2])e30
1.66−0.54+4.78$\[1.66_{-0.54}^{+4.78}\]$ (0.35−0.32+2.45$\[0.35_{-0.32}^{+2.45}\]$)e−3
*E 0.06−0.06+1.84$\[0.06_{-0.06}^{+1.84}\]$ 3.0−1.4+2.4$\[3.0_{-1.4}^{+2.4}\]$ (2.43−0.76+2.76$\[2.43_{-0.76}^{+2.76}\]$)e−6 0.66(7.67/10) (1.53−0.8+0.05$\[1.53_{-0.8}^{+0.05}\]$[2.99])e−15 (3.28−1.71+0.12$\[3.28_{-1.71}^{+0.12}\]$[6.4])e30
*H 4.5−3.6+9.7$\[4.5_{-3.6}^{+9.7}\]$ 0.28−0.17+0.48$\[0.28_{-0.17}^{+0.48}\]$ (2.8−2.8+81.1$\[2.8_{-2.8}^{+81.1}\]$)e−4 0.01(19.47/7) (2.97−2.97+0.01$\[2.97_{-2.97}^{+0.01}\]$[7.21])e−16 (6.35−6.35+0.02$\[6.35_{-6.35}^{+0.02}\]$[15.44])e29
*S 2.4−2.4+6.4$\[2.4_{-2.4}^{+6.4}\]$ 1.7−1.1+13$\[1.7_{-1.1}^{+13}\]$ (2.0−2.0+3.2$\[2.0_{-2.0}^{+3.2}\]$)e-6 0.61(2.72/4) (5.1−5.1+0.08$\[5.1_{-5.1}^{+0.08}\]$[7.1])e-16 (1.1−1.1+0.02$\[1.1_{-1.1}^{+0.02}\]$[1.5])e30

Notes. Sources that are fitted with the wstat statistic are marked with an asterisk; the null hypothesis probability is reported instead of the χν2$\[\chi_\nu^2\]$. We show the absorbed 0.5–8.0 keV flux, the corresponding luminosity, and in brackets the ISM-corrected values (not corrected for local absorption). Errors are not reported for parameters that were kept frozen (Sect. 3.5.1). Abundances of specific elements that were varied: (a)S=1.39±0.50 (b)Ar=8.7−7.7+11.3$\[\mathrm{Ar}{=}8.7_{-7.7}^{+11.3}, \mathrm{Ca}{=}21_{-14}^{+26}\]$, Ca=21−14+26$\[\mathrm{Ar}{=}8.7_{-7.7}^{+11.3}, \mathrm{Ca}{=}21_{-14}^{+26}\]$ (c)S:9.77 Ar:28.08. (d)A Gaussian line was added in the model ( lineE =5.21−0.11+0.15 keV, norm = (6.7−4.4+5.6)×10−8)$\[\left(\text { lineE }{=}5.21_{-0.11}^{+0.15} ~\mathrm{keV} \text {, norm }{=}\left(6.7_{-4.4}^{+5.6}\right) \times 10^{-8}\right)\]$ (e)A model of the form tbabs× pcfabs× ∑vapec was used in this particular case with the parameter for the covering fraction frozen at 0.95.

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