Table 2.
Spectral fits to XMM-Newton pointed observations of XMMSL2 J1446+68.
Date | Γ(a) | Norm (b) | Flux (0.2–2 keV) | Flux (2–10 keV) | χ2/d.o.f. |
---|---|---|---|---|---|
keV−1 cm−2 s−1 | 10−13 ergs s−1 cm−2 | 10−13 ergs s−1 cm−2 | |||
2016-09-08 | 2.56 ± 0.06 | 2.27 ± (0.10)×10−4 | 8.4 ± 0.3 | 2.6 ± 0.3 | 116/99 |
2016-09-16 | 2.59 ± 0.03 | 2.29 ± (0.07)×10−4 | 8.6 ± 0.2 | 2.5 ± 0.2 | 354/347 |
2016-10-30 | 2.58 ± 0.04 | 2.52 ± (0.08)×10−4 | 9.7 ± 0.2 | 2.8 ± 0.2 | 241/237 |
2016-11-27 | 2.55 ± 0.05 | 1.85 ± (0.06)×10−4 | 7.0 ± 0.2 | 2.2 ± 0.2 | 228/220 |
2018-04-25 |
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4.0 ± (1.0)×10−6 | 0.16 ± 0.03 |
![]() |
15/13 |
Combined (c) | 2.58 ± 0.03 | 2.20 ± (0.03)×10−4 | 8.5 ± 0.2 | 2.5 ± 0.2 | 425/410 |
Notes. Fit to the broad-band XMM-Newton spectra, from 0.3–10 keV, of a power law absorbed by the Galactic column (model TBABS, NH = 1.9 × 1020 cm−2). Errors are at the 90% confidence level. Observations of 2016-09-08, 2016-09-16, 2016-10-30, and 2016-11-27 use the EPIC-pn, MOS1, and MOS2 data; the 2018-04-25 observation only uses the EPIC-pn data.
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