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Table 1.

Central values and confidence levels based on the marginalized parameter distribution of the Bayesian model comparison for the broadband fit of combined XMM-Newton and NuSTAR observation of NGC300 ULX-1 for phase-averaged (FULL) and phase-resolved spectra (ON- and OFF-pulse).

MCAE model dBB soft
dBB hot
PL tail
Gaussian line
Phase nH kTdisk Kdisk kThot Khot Γ KPL Egabs σgabs Kgabs
(1021 cm−2) keV keV (×10−3) (×10−5) keV keV
Full (no line) 0.82 0.30 ± 0.013 9.2 2.39 6.81 ± 0.40 0.92 1.8
Full 0.76 0.32 ± 0.02 7.09 2.74 4.37 1.09 0.97 12.0 3.2 2.9
ON-pulse 0.88 0.33 ± 0.03 8.77 3.41 4.74 1.11 0.27 13.6 4.4 9.0
OFF-pulse 0.62 0.31 ± 0.02 5.34 2.82 1.33 2.52 0.002 11.2 2.30 4.3

AC model dBB soft
Cutoff PL
Gaussian line
Phase nH kTdisk Kdisk Efold Γ KcPL Egabs σgabs Kgabs
(1021 cm−2) keV keV (×10−5) keV keV

Full (no line) 0.86 0.29 ± 0.02 11.2 4.17 0.53 48.8
Full 0.83 0.30 9.63 5.66 0.65 46.3 13.1 ± 0.4 3.7 ± 0.3 5.1 ± 1.0
ON-pulse 1.10 0.26 22.5 6.05 0.78 98.3 13.8 3.26 ± 0.24 5.3
OFF-pulse 0.62 0.31 ± 0.02 5.60 4.01 0.36 13.2 11.6 2.4 4.8

Notes. The continuum was fit separately with the MCAE and the AC models. In both cases a Gaussian absorption line was used to model the possible CRSF. All errors are in the 90% confidence range. Kdisk is the normalization parameter for the diskbb component. Namely, Kdisk = (Rdisk/D10 kpc)2 cosi, where Rdisk is the inner radius of the disk in km, D10 kpc is the distance in units of 10 kpc, and i is the inclination. Khot is the same as Kdisk, but for the hot MCD component. KcPL and KPL are the power-law normalization parameters in units of photons/keV/cm2/s at 1 keV. Kgabs is the line depth. The optical depth at line center is .

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