| Name . | BF model . | NH . | Γ . | N unabs/N abs . | R . | E g . | EW . | F 2-10 keV . | |$L_{\,{\rm 2-10}\,{\rm keV}}^{\,\mbox{intr}}$| . | χ2/d.o.f. . |
|---|---|---|---|---|---|---|---|---|---|---|
| (1) . | (2) . | (3) . | (4) . | (5) . | (6) . | (7) . | (8) . | (9) . | (10) . | (11) . |
| XBSJ013240.1−133307 | aPL+scatt+line | 3.|$22^{+0.40}_{-0.49}$| | 1.|$47^{+0.09}_{-0.13}$| | 0.05 ± 0.02 | – | 6.|$25^{+0.09}_{-0.08}$| | 108|$^{+80}_{-68}$| | |$3.81^{+0.28}_{-0.31}$| | |$4.39^{+0.27}_{-0.29}$| | 135.8/128 |
| XBSJ113148.7+311358 | aPL+scatt+refl | 4.|$05^{+2.39}_{-1.84}$| | 1.|$59^{+0.39}_{-0.40}$| | 0.|$07^{+0.06}_{-0.04}$| | 0.|$98^{+0.02}_{-0.66}$| | – | – | |$1.17^{+1.20}_{-0.60}$| | |$1.01^{+1.83}_{-0.41}$| | 14.9/16 |
| XBSJ160645.9+081525 | aPL+scatt | 29.|$62^{+9.63}_{-8.01}$| | 2.|$02^{+0.56}_{-0.52}$| | <0.05 | – | – | – | |$1.77^{+3.84}_{-1.20}$| | |$5.87^{+12.96}_{-3.98}$| | 16.6/25 |
| Name . | BF model . | NH . | Γ . | N unabs/N abs . | R . | E g . | EW . | F 2-10 keV . | |$L_{\,{\rm 2-10}\,{\rm keV}}^{\,\mbox{intr}}$| . | χ2/d.o.f. . |
|---|---|---|---|---|---|---|---|---|---|---|
| (1) . | (2) . | (3) . | (4) . | (5) . | (6) . | (7) . | (8) . | (9) . | (10) . | (11) . |
| XBSJ013240.1−133307 | aPL+scatt+line | 3.|$22^{+0.40}_{-0.49}$| | 1.|$47^{+0.09}_{-0.13}$| | 0.05 ± 0.02 | – | 6.|$25^{+0.09}_{-0.08}$| | 108|$^{+80}_{-68}$| | |$3.81^{+0.28}_{-0.31}$| | |$4.39^{+0.27}_{-0.29}$| | 135.8/128 |
| XBSJ113148.7+311358 | aPL+scatt+refl | 4.|$05^{+2.39}_{-1.84}$| | 1.|$59^{+0.39}_{-0.40}$| | 0.|$07^{+0.06}_{-0.04}$| | 0.|$98^{+0.02}_{-0.66}$| | – | – | |$1.17^{+1.20}_{-0.60}$| | |$1.01^{+1.83}_{-0.41}$| | 14.9/16 |
| XBSJ160645.9+081525 | aPL+scatt | 29.|$62^{+9.63}_{-8.01}$| | 2.|$02^{+0.56}_{-0.52}$| | <0.05 | – | – | – | |$1.77^{+3.84}_{-1.20}$| | |$5.87^{+12.96}_{-3.98}$| | 16.6/25 |
Note. Fluxes and luminosities refer to the MOS calibration. Errors are quote at 90 per cent confidence level.
Col. (1): source name in the XBS sample. Col. (2): best-fitting model: aPL = absorbed power law; scatt = scattering component (additional unabsorbed power law with the same photon index as the primary one); refl = neutral Compton reflection (continuum + Fe and Ni lines; the pexmon model in xspec, with the same photon index as the primary power law); line = narrow Gaussian line. Col. (3): intrinsic column density; in units of 1022 cm−2. Col. (4): source photon index. Col. (5): scattering fraction, defined as the ratio of the unabsorbed and the direct power-law normalizations. Col. (6): reflection scaling factor of the pexmon component. Col. (7): line energy. Col. (8): line EW. Col. (9): observed flux (deabsorbed by our Galaxy) in the 2-10 keV energy band, in units of 10−13 ergcm−2s−1. Col. (10): luminosity of the direct component (deabsorbed by intrinsic and Galactic NH) in the 2-10 keV energy band, in units of 1044 ergs−1. Col. (11): χ 2 and number of degree of freedom.
| Name . | BF model . | NH . | Γ . | N unabs/N abs . | R . | E g . | EW . | F 2-10 keV . | |$L_{\,{\rm 2-10}\,{\rm keV}}^{\,\mbox{intr}}$| . | χ2/d.o.f. . |
|---|---|---|---|---|---|---|---|---|---|---|
| (1) . | (2) . | (3) . | (4) . | (5) . | (6) . | (7) . | (8) . | (9) . | (10) . | (11) . |
| XBSJ013240.1−133307 | aPL+scatt+line | 3.|$22^{+0.40}_{-0.49}$| | 1.|$47^{+0.09}_{-0.13}$| | 0.05 ± 0.02 | – | 6.|$25^{+0.09}_{-0.08}$| | 108|$^{+80}_{-68}$| | |$3.81^{+0.28}_{-0.31}$| | |$4.39^{+0.27}_{-0.29}$| | 135.8/128 |
| XBSJ113148.7+311358 | aPL+scatt+refl | 4.|$05^{+2.39}_{-1.84}$| | 1.|$59^{+0.39}_{-0.40}$| | 0.|$07^{+0.06}_{-0.04}$| | 0.|$98^{+0.02}_{-0.66}$| | – | – | |$1.17^{+1.20}_{-0.60}$| | |$1.01^{+1.83}_{-0.41}$| | 14.9/16 |
| XBSJ160645.9+081525 | aPL+scatt | 29.|$62^{+9.63}_{-8.01}$| | 2.|$02^{+0.56}_{-0.52}$| | <0.05 | – | – | – | |$1.77^{+3.84}_{-1.20}$| | |$5.87^{+12.96}_{-3.98}$| | 16.6/25 |
| Name . | BF model . | NH . | Γ . | N unabs/N abs . | R . | E g . | EW . | F 2-10 keV . | |$L_{\,{\rm 2-10}\,{\rm keV}}^{\,\mbox{intr}}$| . | χ2/d.o.f. . |
|---|---|---|---|---|---|---|---|---|---|---|
| (1) . | (2) . | (3) . | (4) . | (5) . | (6) . | (7) . | (8) . | (9) . | (10) . | (11) . |
| XBSJ013240.1−133307 | aPL+scatt+line | 3.|$22^{+0.40}_{-0.49}$| | 1.|$47^{+0.09}_{-0.13}$| | 0.05 ± 0.02 | – | 6.|$25^{+0.09}_{-0.08}$| | 108|$^{+80}_{-68}$| | |$3.81^{+0.28}_{-0.31}$| | |$4.39^{+0.27}_{-0.29}$| | 135.8/128 |
| XBSJ113148.7+311358 | aPL+scatt+refl | 4.|$05^{+2.39}_{-1.84}$| | 1.|$59^{+0.39}_{-0.40}$| | 0.|$07^{+0.06}_{-0.04}$| | 0.|$98^{+0.02}_{-0.66}$| | – | – | |$1.17^{+1.20}_{-0.60}$| | |$1.01^{+1.83}_{-0.41}$| | 14.9/16 |
| XBSJ160645.9+081525 | aPL+scatt | 29.|$62^{+9.63}_{-8.01}$| | 2.|$02^{+0.56}_{-0.52}$| | <0.05 | – | – | – | |$1.77^{+3.84}_{-1.20}$| | |$5.87^{+12.96}_{-3.98}$| | 16.6/25 |
Note. Fluxes and luminosities refer to the MOS calibration. Errors are quote at 90 per cent confidence level.
Col. (1): source name in the XBS sample. Col. (2): best-fitting model: aPL = absorbed power law; scatt = scattering component (additional unabsorbed power law with the same photon index as the primary one); refl = neutral Compton reflection (continuum + Fe and Ni lines; the pexmon model in xspec, with the same photon index as the primary power law); line = narrow Gaussian line. Col. (3): intrinsic column density; in units of 1022 cm−2. Col. (4): source photon index. Col. (5): scattering fraction, defined as the ratio of the unabsorbed and the direct power-law normalizations. Col. (6): reflection scaling factor of the pexmon component. Col. (7): line energy. Col. (8): line EW. Col. (9): observed flux (deabsorbed by our Galaxy) in the 2-10 keV energy band, in units of 10−13 ergcm−2s−1. Col. (10): luminosity of the direct component (deabsorbed by intrinsic and Galactic NH) in the 2-10 keV energy band, in units of 1044 ergs−1. Col. (11): χ 2 and number of degree of freedom.
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