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Fig. 9


As Fig. 7, but for stars with with relatively large proper motions centred around (μαcosδ,μδ) = ( + 20, −45) mas/yr with a radius of 15 mas/yr. Top: in 2MAst HQb5 (maximum number of objects per 0.25 × 0.25 deg2 pixel is about 60), bottom: in UCAC4 HQ (maximum of about 25). The Magellanic Clouds (MCs) are marked. The Pleiades can easily be seen in both plots. A southern 2MAst HQb5 artefact, similar in appearance to the Pleiades, is also highlighted.

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