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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 5.

Biases of fitted QPO amplitude ( R) with min(χ 2) (blue filled squares) and MLE (black filled circles) fitting for different M, from 4 to 64, in steps of 4. Error bars on the MLEs are plotted but are in many cases smaller than the plot symbols. 4096 averages of M PDS were fitted by the two methods. The bias of the MLEs of R is lower than 0.3% ( M = 4). At the opposite, biases of the R estimates from min(χ 2) fitting can be as large as ~30% for M = 4 and remain as large as ~2.5% for M = 64. This figure alone demonstrates that MLE should always be preferred, when averaging a very large number of PDS is not possible.

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