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Fig. 6


Figure 6a shows the reconstructed light curve ϕ for SGR 1900+14. The grey rectangles indicate the operational down times of the instrument. Figure 6b: snapshot of the entire reconstruction between ≈80 s and ≈91 s. For t ≳ 88 the instrument had an operational down time, leading to zero counts in this time interval. Figure 6c and Figure 6d: reconstructed power spectra as well as their uncertainties, using a smoothness-enforcing prior with σsm = 5 × 105 and σsm = 105, respectively. The plots have the same volumes and sampling rate as in Fig. 1.

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