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Fig. 5.

image

Spectral energy distribution of IGR J19294+1816 obtained with the Swift/XRT and NuSTAR telescopes during the high (black dots) and low (blue and green dots) intensity states. The data from the two NuSTAR units are added together for plotting (but not for actual fit). Solid lines represent best-fit models for each observation including fundamental line only (see text).

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