Table 3.
X-ray spectral fit results.
Source | Obs. | Model | Photon |
![]() |
![]() |
![]() |
dof | Fobserved (a) | L (b) |
---|---|---|---|---|---|---|---|---|---|
name | ID | index | (1021 cm−2) | (1021 cm−2) | (erg cm−2 s−1) | (erg s−1) | |||
J0453 | 0804550201 | PL |
![]() |
0.85 |
![]() |
1.0 | 13 |
![]() |
6.5 × 1034 |
J0457 | 0804550101 | PL | 0.64 ± 0.03 | 0.85 | < 0.17 | 0.98 | 388 | 1.83 ± 0.05 × 10−12 | 5.6 × 1035 |
J0457 | 0841660301 | PL | 0.63 ± 0.05 | 0.85 | < 0.47 | 1.07 | 212 | 0.97 ± 0.03 × 10−12 | 2.9 × 1035 |
J0457 | combined | PL | 0.64 ± 0.03 | 0.85 | < 0.14 | 1.01 | 602 | – | – |
J0524 | 0841320201 | PL |
![]() |
0.54 |
![]() |
1.24 | 248 |
![]() |
3.9 × 1035 |
J0524 (c) | 0841320201 | highecut |
![]() |
0.54 |
![]() |
1.06 | 246 |
![]() |
3.9 × 1035 |
J0524 (d) | 0841320201 | fdcut |
![]() |
0.54 |
![]() |
1.07 | 246 |
![]() |
4.0 × 1035 |
J0524 (e) | 0841320201 | PL+BB |
![]() |
0.54 |
![]() |
1.02 | 246 |
![]() |
4.8 × 1035 |
Notes. Best-fit parameters using a model with absorbed power-law emission. Errors indicate 90% confidence ranges.
Source luminosities (0.2–10.0 keV) corrected for absorption, assuming a distance of 50 kpc (Pietrzyński et al. 2013). The Galactic foreground column density was taken from Dickey & Lockman (1990). Fluxes and luminosities are taken as mean of the values from the different EPIC instruments.
The PL is modified by an exponential cutoff (highecut in XSPEC) with cut-off energy at 6.5 keV, and a folding energy of 4.1
keV.
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