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Cited article:

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A low-noise, high-dynamic-range, digital receiver for radio astronomy applications: an efficient solution for observing radio-bursts from Jupiter, the Sun, pulsars, and other astrophysical plasmas below 30 MHz

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A model for double notches and bifurcated components in radio profiles of pulsars and magnetars

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Radio Phase-Resolved Spectra of the Conal-Double Pulsar B1133+16

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Frequency dependence of orthogonal polarisation modes in pulsars

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Polarization of individual pulses of radio pulsars at the low frequencies 40, 60, and 103 MHz

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Null-induced mode changes in PSR B0809+74

A. G. J. van Leeuwen, M. L. A. Kouwenhoven, R. Ramachandran, J. M. Rankin and B. W. Stappers
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