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Fig. 3.

image

Results of fitting procedure A applied to the 2010–2011 outburst of GX 339-4. The black markers are fits taken from Clavel et al. (2016) reported with their error bars when reliable, while color lines display our results: green, blue, yellow, and red for hard, hard-intermediate, soft-intermediate, and soft states, respectively (see Sect. 2). Left, from top to bottom: 3–200 keV total luminosity L3−200 (in Eddington units), the power-law luminosity fraction PLf = Lpl/L3−200, and the power-law index Γ. Right: DFLD. The hard tail proxy we used was frozen to 10%, but 1% and 3% proxies are also illustrated as red dot-dashed and dashed lines (see Paper III).

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