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Wide-band, low-frequency pulse profiles of 100 radio pulsars with LOFAR

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Figure

Fig. 1. Example of pulsar profile evolution for PSR B0950 + 08, from 1400 MHz down to 30 MHz
Table 1. Pulsars for which the absolute alignment was not achieved with the refolding using the same ephemeris (see text for details).
Table 2. Pulsars for which one or more glitches occurred during the range of the ephemerides used in this paper (above the horizontal line) or near the range of validity of our ephemerides (below the horizontal line).
Fig. 2. Gaussian modelling and resulting fit residuals for the pulse profile of PSR B1133 + 16 at four frequencies, between 0.4–0.6 in pulse phase.
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