Right Ascension Measures for Ten Pulsars

Abstract
Improved right ascensions have been measured for ten pulsars using the East–West arm of the Bologna ‘Northern Cross’ radio telescope at 408 MHz. Each pulsar in the list was observed at transit on a number of occasions of relative activity. For each object the positions corresponding to the centres of the observed pulse trains were averaged to obtain the final right ascension. Systematic pointing errors were eliminated by frequent observations of bright radio sources of accurately known position. The measured right ascensions for epoch 1950 are given in Table I.

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