Abstract
THE Westerbork Synthesis Radio Telescope (WSRT) has been used to observe a pulsar for a period of twelve hours at 1,415 MHz. This long, continuous observation gave information on the pulsar mean intensity as well as a measure of the longer term fluctuations in intensity due to interstellar scintillations. The resultant sky map illustrates the source properties in a synthesis observation.
This is a preview of subscription content, access via your institution
Access options
References
Ryle, M., Elsmore, B., and Neville, A. C., Nature, 207, 1024 (1965).
Lyne, A. G., and Rickett, B. J., Nature, 219, 1340 (1968).
Downs, G. S., Morris, G. A., jun., and Reichley, P. E., Nature, 222, 1257 (1969).
Reichley, P. E., Downs, G. S., and Morris, G. A., Astrophys. J. Lett., 159, L35 (1970).
Rickett, B. J., Mon. Not. Roy. Astron. Soc., 150, 67 (1970).
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
COLE, T., WEILER, K. Pulsar CP 0328 at 1,420 MHz. Nature Physical Science 230, 114–115 (1971). https://doi.org/10.1038/physci230114a0
Received:
Issue date:
DOI: https://doi.org/10.1038/physci230114a0
