Fig. 4.
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Sample of 19 pulsars observed with I-LOFAR and REALTA. Each of these observations is 6 min in duration and were taken on 4–5 March 2020 using the HBA antennas (110–190 MHz ). The data were processed using the method described in Sect. 3.3 and plotted using PSRCHIVE. The x-axis in each plot is the pulse phase in radians, while the y-axis is flux density in arbitrary units.
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