Fig. B.1
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Lag-frequency spectrum of observation O106 between energy bands 0.5–1 keV and 1–10 keV independently computed with the code used in this paper (implemented in IDL and used e.g. in De Marco et al. 2015b, 2017), with the GeneralHigh-Energy Aperiodic Timing Software (GHATS; used e.g. in Belloni et al. 2005), and with Stingray (developed by Huppenkothen et al. 2019a,b and publicly available). The scatter in the data is due to slight differences in the extraction and binning. These lags are compared to those reported in Kara et al. (2019) for the same observation.
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