Search for glitches in gamma-ray pulsars with deep learning

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Fig. 7.

Weighted H-test data calculated as discussed in Sect. 2, and convolved with Gaussian function (3) for three generated pulsars with glitches: (a) at 56183 MJD with Δf ≃ 4.6 × 10⁻⁸ Hz, (b) at 55045 MJD with Δf ≃ 4.2 × 10⁻⁷ Hz, and (c) at 56041 MJD with Δf ≃ 2.2 × 10⁻⁶ Hz.

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