Fig. 3.
DM time series of the selected pulsars after subtraction of the IISM component. Observations highlighted in red were taken when the Solar elongation of the source was < 50°, and the gray vertical lines mark the modified Julian dates (MJDs) of the Solar conjunctions. For the sake of visual clarity, these plots show only 95% of the most precise measurements, although all data points are used in the analysis.
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