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Table 2.

Best-fitting spectral parameters for the averaged and phase-resolved spectra of 4U 0115+63.

Parameter Obs1 Obs2 Obs2016 Averaged ϕ1 ϕ2 ϕ3 ϕ4
CObs1 1 . 14 0.14 + 0.22 $ 1.14^{+0.22}_{-0.14} $ 1.14 (fixed) 1.14 (fixed) 1.14 (fixed) 1.14 (fixed)
CObs2 1 (fixed) 1 (fixed) 1 (fixed) 1 (fixed) 1 (fixed)
CObs2016 0 . 73 0.09 + 0.13 $ 0.73^{+0.13}_{-0.09} $ 0.73 (fixed) 0.73 (fixed) 0.73 (fixed) 0.73 (fixed)
NH (1022 cm−2) 0.9 (fixed) 0.9 (fixed) 0.9 (fixed) 0.9 (fixed) 0.9 (fixed) 0.9 (fixed) 0.9 (fixed) 0.9 (fixed)
kTBB (keV) 0 . 44 0.10 + 0.02 $ 0.44^{+0.02}_{-0.10} $ 0 . 49 0.06 + 0.06 $ 0.49^{+0.06}_{-0.06} $ 0 . 43 0.02 + 0.02 $ 0.43^{+0.02}_{-0.02} $ 0 . 44 0.01 + 0.01 $ 0.44^{+0.01}_{-0.01} $ 0 . 47 0.06 + 0.08 $ 0.47^{+0.08}_{-0.06} $ 0 . 45 0.04 + 0.03 $ 0.45^{+0.03}_{-0.04} $ 0 . 47 0.03 + 0.03 $ 0.47^{+0.03}_{-0.03} $ 0 . 39 0.05 + 0.05 $ 0.39^{+0.05}_{-0.05} $
RBB (km) 0 . 39 0.04 + 0.07 $ 0.39^{+0.07}_{-0.04} $ 0 . 30 0.05 + 0.11 $ 0.30^{+0.11}_{-0.05} $ 0 . 32 0.03 + 0.03 $ 0.32^{+0.03}_{-0.03} $ 0 . 36 0.03 + 0.04 $ 0.36^{+0.04}_{-0.03} $ 0 . 26 0.06 + 0.10 $ 0.26^{+0.10}_{-0.06} $ 0 . 41 0.06 + 0.09 $ 0.41^{+0.09}_{-0.06} $ 0 . 42 0.05 + 0.08 $ 0.42^{+0.08}_{-0.05} $ 0 . 35 0.07 + 0.17 $ 0.35^{+0.17}_{-0.07} $
Flux (10−13 erg cm−2 s−1) 2 . 38 0.14 + 0.15 $ 2.38^{+0.15}_{-0.14} $ 2 . 09 0.18 + 0.13 $ 2.09^{+0.13}_{-0.18} $ 1.53 0.01 + 0.01 $ ^{+0.01}_{-0.01} $ 2 . 10 0.23 + 0.15 $ 2.10^{+0.15}_{-0.23} $ 1 . 47 0.34 + 0.34 $ 1.47^{+0.34}_{-0.34} $ 2 . 84 0.37 + 0.37 $ 2.84^{+0.37}_{-0.37} $ 3 . 95 0.43 + 0.43 $ 3.95^{+0.43}_{-0.43} $ 1 . 05 0.22 + 0.22 $ 1.05^{+0.22}_{-0.22} $
LX (1032 erg s−1) 7 . 3 0.4 + 0.5 $ 7.3^{+0.5}_{-0.4} $ 6 . 4 0.7 + 0.4 $ 6.4^{+0.4}_{-0.7} $ 4.8 0.3 + 0.3 $ ^{+0.3}_{-0.3} $ 6 . 4 0.7 + 0.5 $ 6.4^{+0.5}_{-0.7} $ 4 . 5 0.8 + 1.0 $ 4.5^{+1.0}_{-0.8} $ 8 . 7 1.0 + 1.1 $ 8.7^{+1.1}_{-1.0} $ 12 . 1 1.2 + 1.3 $ 12.1^{+1.3}_{-1.2} $ 3 . 2 0.6 + 0.7 $ 3.2^{+0.7}_{-0.6} $

C-statistic/d.o.f. 86.1/86 28.1/37 229.6/202 343.4/326 33.0/29 58.5/59 86.3/74 26.6/26

Notes. Unabsorbed X-ray fluxes and luminosities are calculated in the 0.3−10 keV energy range. The blackbody emission radius RBB was estimated by assuming an isotropic source at a distance of 5.0 kpc.

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