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CHARACTERIZING INTERMITTENCY OF 4-Hz QUASI-PERIODIC OSCILLATION IN XTE J1550–564 USING HILBERT–HUANG TRANSFORM
2015 The Astrophysical Journal 815 74.
Caption: Figure 3.
Fourier power spectrum of the IMF c4 (blue), plotted along with the best Lorentzian model fit (red).
© 2015. The American Astronomical Society. All rights reserved.