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Fig. A.1.
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Histograms of the centroid frequencies of the QPOs found around 67 Hz in the data from GRS 1915+105, as reported in Belloni & Altamirano (2013b). The solid black line is the best Gaussian fit to the histogram, which yields a centroid frequency of 67.712 Hz and an FWHM of 2.056 Hz.
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