Pulsar Associated with the Supernova Remnant IC 443

Computer Science

Scientific paper

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Scientific paper

DURING the period July 26 to September 21, 1972, the Jodrell Bank Mark IA radio telescope has been engaged in a systematic search for pulsars at a frequency of 408 MHz. The technique is that used by Davies, Large and Pickwick1 in 1970, but adapted in a way that allows the analysis to be carried out in real time on the Argus data processing computer.

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