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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 4.

Results of fitting simulated data with a constant and a Lorentzian QPO model. Each of the four panels shows the histogram of the estimates for one of the four model parameters (top left, a; bottom left, ν 0; top right, w; bottom right, R). The parameters were estimated using the MLE (black line) and the min(χ 2) method (blue line) by fitting the average of M = 4 periodograms (4096 samples). For min(χ 2) fitting, outliers in the parameter distribution (e.g., fitted R ⩾ 100) were removed before building the histograms (about 2% of the total sample are outliers). The vertical dashed line indicates the true parameter values for the simulations. Clearly, the MLEs show no strong biases, but the min(χ 2) results underestimate both the Poisson level and the QPO amplitude. The estimates have generally larger spreads from min(χ 2) fitting than from the MLE.

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