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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 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.

(a)

Power-law slope,

(b)

power-law normalisation,

(c)

Combination of observations 1-4 (2016-09-08 – 2016-11-27), EPIC-pn data only, without filtering for periods of higher background.

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