Fig. B.3.
Comparison between observed average profiles of pulsar B (black) and the best fit Gaussian templates (red), as described in Sect. 3.2.3. The profiles shown have been tabulated according to orbital-phase window (columns): BP1, BP2, IP, and WP, and the MJD range (rows). The reduced chi-squared value shown for each plot has been calculated using only the off-pulse RMS (σstat) as weights.
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