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Table 9.

Significance values of the observed periods using either the local or the global method with respect to the monthly and weekly γ-ray light curves of PG 1553+113 and PKS 0447−489, respectively.

Source Simulation Monthly
Weekly
algorithm PSD-slope Local Global PSD-slope Local Global
βm significance significance βw significance significance
PG 1553+113 Timmer & Koenig βmin = 0.75 5.33σ 2.46σ βmin = 0.55 5.32σ 3.06σ
βm⟩ = 0.88 3.89σ 2.14σ βw⟩ = 0.66 3.70σ 2.07σ
βmax = 1.01 3.72σ 1.86σ βmax = 0.77 2.90σ 0.93σ
Emmanoulopoulos βmin = 0.76 5.33σ 2.40σ βmin = 0.56 5.32σ 3.10σ
βm⟩ = 0.90 3.89σ 2.06σ βw⟩ = 0.67 3.83σ 2.16σ
βmax = 1.04 3.48σ 1.75σ βmax = 0.78 2.79σ 0.79σ
PKS 0447−439 Timmer & Koenig βmin = 0.91 3.12σ 1.06σ βmin = 0.66 3.32σ 1.74σ
βm⟩ = 1.06 2.87σ 1.00σ βw⟩ = 0.79 3.02σ 1.28σ
βmax = 1.21 2.67σ 0.46σ βmax = 0.92 2.53σ 0.64σ
Emmanoulopoulos βmin = 0.94 3.11σ 1.04σ βmin = 0.67 3.30σ 1.69σ
βm⟩ = 1.07 2.94σ 1.16σ βw⟩ = 0.80 3.03σ 1.25σ
βmax = 1.20 2.71σ 0.54σ βmax = 0.93 2.47σ 0.65σ

Notes. The significance levels were evaluated via MC-Simulation using Timmer & Koenig (1995) and Emmanoulopoulos et al. (2013) algorithms with 50 000 trials. The mean slopes ⟨βm⟩ were obtained from fitting the γ-ray power spectra with a simple power-law model, and the corresponding success fractions were calculated based on the PSRESP method (Uttley et al. 2002). βmin and βmin represents the minimum and maximum of the 1σ error bars resulting from fitting Gaussians to each of the slope profiles.

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