Fig. 2
Full resolution image of the Crab pulsar obtained from uniformly weighted data. The image has a peak flux density of 8.3 mJy/beam and an rms noise of 0.3 mJy/beam. The synthesised (restoring) beam is 19.9 × 2.2 mas, oriented at a PA = 83°. The extreme ellipticity of the restoring beam results from a very limited East-West uv-coverage on baselines ≥ 10 Mλ.
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