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Table 5.

Journal of the X-ray modes of J1109 from the simultaneous XMM-Newton EPIC and NuSTAR data sets, and results of the spectral fits.

Mode Instrument Net exposure Net count rate Γ Absorbed flux Unabsorbed flux Luminosity χ red 2 $ \chi _{{\rm{red}}}^2 $ (d.o.f.)
(ks) (counts s−1) (10−12 erg cm−2 s−1) (10−12 erg cm−2 s−1) ( 10 34 d 4 2 $ {10^{34}} d_4^2 $ erg s−1)
EPIC pn 1.0 1.54  ±  0.04
EPIC MOS 1 1.0 0.44  ±  0.02
Flare EPIC MOS 2 1.0 0.51  ±  0.02 1.68  ±  0.04 10.7  ±  0.5 27  ±  2 5.2  ±  0.4 0.89 (75)
FPMA 0.4 0.13  ±  0.02
FPMB 0.4 0.13  ±  0.02

EPIC pn 31.0 0.728  ±  0.006
EPIC MOS 1 31.3 0.216  ±  0.003
High EPIC MOS 2 30.8 0.248  ±  0.003 1.61  ±  0.01 5.42  ±  0.06 14.2  ±  0.3 2.72  ±  0.06 1.19 (437)
FPMA 19.9 0.081  ±  0.002
FPMB 20.0 0.073  ±  0.002

EPIC pn 5.7 0.063  ±  0.008
EPIC MOS 1 5.8 0.016  ±  0.002
Low EPIC MOS 2 5.7 0.018  ±  0.002 1.5  ±  0.1 0.56  ±  0.09 1 . 6 0.4 + 0.5 $ 1.6^{+0.5}_{-0.4} $ 0 . 31 0.08 + 0.10 $ 0.31^{+0.10}_{-0.08} $ 1.05 (26)
FPMA 4.2 0.007  ±  0.002
FPMB 4.2 0.005  ±  0.002

Notes. The net count rates refer to the 0.3–10 keV energy band for XMM-Newton data and to the 3–79 keV energy range for NuSTAR data. Spectra were fitted with an absorbed power law model with column density fixed to the average value, NH = 5.3  ×  1021 cm−2. Fluxes and luminosities are quoted over the 0.3–79 keV energy band. Luminosities were computed assuming a distance of D = 4 kpc and isotropic emission.

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