Evidence for different accretion regimes in GRO J1008−57

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Table 3

Parameters of the best-fitting combination of models describing the spectral evolution as shown in Fig. 6.

	Γ(F_PL)	F_BB(F_PL)
	dbl-brkn log	high-brkn pow

a _X
b _X
F _brk,lo		–
F _brk,hi ^a
χ² ^b	36.41	44.81
/d.o.f.^c	0.97/84

Notes. The definitions of the models are given in the text.

^(a)

F_brk,hi has been determined by a joint fit to both correlations.

^(b)

The χ² sum over all 45 data points for each parameter evolution.

^(c)

The total goodness of the fit.

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