Discovery of a magnetic neutron star in X-ray transient IGR J01583+6713

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Table 2:

Different fits to the spectrum of IGR J01583+6713 during the outburst state.
Model	$\Gamma$ / kT	$E_{\rm cyc,0}$ (keV)	$E_{\rm cyc,1}$ (keV)	Flux (10^-10 erg cm^-2 s^-1)	reduced $\chi^2$
power+cyclabs	$2.13\pm 0.53$	$35.1\pm 2.1$	$65.8\pm 4.9$	$1.99\pm 0.42$	0.989(5 d.o.f.)
bremss+cyclabs	$35.2\pm 4.1$ keV	$35.3\pm 1.6$	$67.9\pm 4.8$	$1.98\pm 0.41$	0.828(5 d.o.f.)

Notes. Power implies a power law model, bremss implies a thermal bremsstrahlung model, cyclabs implies a resonant cyclotron absorption model. The hard X-ray fluxes in the range of 20-100 keV in different fits are also given.

Source LaTeX | All tables | In the text

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