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Maximum Likelihood Fitting of X-Ray Power Density Spectra: Application to High-frequency Quasi-periodic Oscillations from the Neutron Star X-Ray Binary 4U1608-522

  • Authors: Didier Barret and Simon Vaughan

Barret & Vaughan 2012 The Astrophysical Journal 746 131.

  • Provider: AAS Journals

Caption: Figure 8.

Magnitude of the bias on w ( b leakage w ) as a function of time series duration T evaluated for two different values of w (1 and 5 Hz; lower and upper curves, respectively). The leakage bias was computed numerically by comparing of the Lorentzian profile before and after convolution (computed on a fine grid of frequencies, δ f = 2 −13). Roughly, the bias decays as b leakage w T −1.

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