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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 7.

Left: periodogram of the frequency variations of 4U1608-522 as derived from the MLEs of the QPO frequency on a timescale of 16 s. The best power-law fit is shown with a dashed line (index 1.8 ± 0.2). Right: broadening of the QPO with increasing integration time of the fitted PDS. As expected from a random walk, the broadening goes like . The best fit is shown with a dot-dashed line. Such analysis enables us to derive the intrinsic QPO width to be 3.2 Hz, corresponding to a quality factor of 259 ± 5 at a frequency of 829 Hz.

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