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CHARACTERIZING INTERMITTENCY OF 4-Hz QUASI-PERIODIC OSCILLATION IN XTE J1550–564 USING HILBERT–HUANG TRANSFORM

  • Authors: Yi-Hao Su, Yi Chou, Chin-Ping Hu, and Ting-Chang Yang

2015 The Astrophysical Journal 815 74.

  • Provider: AAS Journals

Caption: Figure 9.

(a) rms amplitude-flux relation for the ∼4-Hz intermittent oscillations. (b) Frequency-flux relation for the ∼4-Hz intermittent oscillations. The correlation coefficients for non-rebinned points (blue dots) are 0.213 and 0.13, respectively. After binning on mean count rate (red stars), the linear relationships become more clear and their correlation coefficients are 0.51 and 0.41, respectively.

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