15-GHz flux density of V

Astronomy and Astrophysics – Astronomy

Scientific paper

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Radio, Transients, Variables, Stars

Scientific paper

Following measurements of the radio flux density of V407 Cyg (see ATEL #2506, #2511), the object was observed with the AMI Large Array in Cambridge (UK) for two short periods on 2010 Mar 26 at 15 GHz (3.5 GHz bandwidth, centred on 15.7 GHz). The first observation was 11h49m to 12h20m UT and the mean flux density was 14.5 mJy; the second was 12h25m to 12h44m, and the mean flux density was 12.0 mJy.

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