Abstract
TWENTY pulsars were observed during the period May 20 to 25, 1971, using the NRAO 3-element interferometer. The principal aims of the observations were (1) to obtain accurate position measurements independent of pulse timing considerations; (2) to determine the flux densities of pulsars at 2.7 GHz and also, for the strongest ones, at 8.1 GHz; and (3) to detect (or place upper limits on) any continuous, non-pulsed radio emission from regions of small angular size near the pulsars.
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HUGUENIN, G., TAYLOR, J., HJELLMING, R. et al. Interferometric Observations of Pulsars at 2.7 and 8.1 GHz. Nature Physical Science 234, 50–51 (1971). https://doi.org/10.1038/physci234050a0
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DOI: https://doi.org/10.1038/physci234050a0
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