Abstract
THE 100-m telescope at Effelsberg has been used to determine more accurate positions and periods for seven recently discovered pulsars, using a helium cooled parametric receiver at 11 cm, at which wavelength the telescope has a circular beam-width of 4.7 arc min to half-power. Positions were determined by taking an integration at every beam area within the published error rectangles1–4. The derived positions and other quantities determined are quoted in Table 1 where these represent an improvement over previous data.
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GRAHAM, D., HUNT, G. Observations at 11 cm of Recently Discovered Pulsars. Nature Physical Science 242, 86–87 (1973). https://doi.org/10.1038/physci242086a0
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DOI: https://doi.org/10.1038/physci242086a0
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