Timing irregularities and glitches from the pulsar monitoring campaign at IAR

Open Access

Fig. 5.

Schematic representation of steps 1 and 2 of the algorithm described in Sect. 3.2. Example with N_min = 5. Top: ν and $\dot{ν}$ $\dot{\nu}$ are not fitted in windows W_i and $W_{i}^{'}$ $W^\prime_i$ because there are only four TOAs inside $W_{i}^{'}$ $W^\prime_i$ . Bottom: ν and $\dot{ν}$ $\dot{\nu}$ are fitted in windows W_i + 1 and $W_{i + 1}^{'}$ $W^\prime_{i+1}$ because there are at least five TOAs inside each of them.

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