X-ray emission from magnetized neutron star atmospheres at low mass-accretion rates - I. Phase-averaged spectrum

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Table 1.

Parameters of the best-fit models of the pulse-averaged spectra shown in Fig. 7.

Parameter	Best-fit
N_H [10²² cm⁻²]	1.1 (fixed)
log 10(Ṁ/[g s⁻¹])
r₀ [m]
E_cyc [keV]
f_cyc
z	0.24 (fixed)
C_FPMA^(a)	1 (fixed)
C_FPMB^(a)	1.00 ± 0.04
C_XRT^(a)

Cash/d.o.f.	276.03/221 = 1.25

Notes. The indicated uncertainties are at 1.6σ (90%) confidence level.

^(a)

Detector cross-calibration constants with respect to FPMA.

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