Fig. 2
Spectra for three pulsars in the frequency range 100−200 MHz. Errors bars correspond to a 10% uncertainty in the pulsar flux estimation. The best fit power law curves are also displayed. For PSR B1133+16, a broken power-law provides a closer fit to the measured fluxes. The flux in the RFI-affected band centred at 163.5 MHz is not included for PSR B1133+16.
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