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Table 2.

Best-fit results of GRO J1750-27 joint analysis for the joint NuSTAR and NICER (ObsID 4202350104) spectral data with different best-fit solution for the Model I (Deep and Smooth) tbabs*(bbodyrad+highecut*pow+gaussKα[+gaussbroad])*gabs, Model II tbabs*(bbodyrad+cutoffpl+gaussKα)*gabs, and Model III tbabs*(bbodyrad+bwcyc+gaussKα)*gabs (see text).

Model I
Model II Model III
Deep Smooth Cutoffpl BWcyc
CFPMA (fixed) 1 1 1 1
CFPMB
CNICER
NH [1022 cm−2]
kTBB [keV]
normBB
EKα [keV]
σKα [keV]
normKα [10−4 ph cm−2 s−1]
Γ
normΓ( * )
HighEcut [keV]
cutoffE [keV]
foldE
EGauss [keV]
σGauss [keV]
NormGauss [ph cm−2 s−1]
ξ
δ
B [1012 G] 4.62 ( ⋆ )
[1017 g s−1]
Te [keV]
r0 [m]
d [kpc] 14.0 (fixed)
normbwcyc
Ecyc [keV]
σcyc [keV]
Strengthcyc( ‡ ) (τcyc( ‡ ) [keV])
Flux ( † ) (1–60 keV)
χ2/d.o.f. 3156/3395 3308/3392 3364/3396 3435/3393
Goodness-of-fit 44% 45% 40% 45%
Null-hypothesis P 70% 85% 68% 28%

Notes. All reported errors are at 1σ c.l. and based on the MCMC chain values. ( * )In units of photons keV−1 cm−2 s−1 at 1 keV. ( ⋆ )Linked to the Ecyc parameter (see text). ( ‡ )Line depth (optical depth) as defined in XSPEC. ( † )Unabsorbed flux calculated for the entire model (in units of 10−9 erg cm−2 s−1), obtained using the cflux model from XSPEC as resulting from FPMA.

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