OCRA monitoring of V407 Cyg at 30GHz

Details OCRA monitoring of V407 Cyg at 30GHz OCRA monitoring of V407 Cyg at 30GHz

Oct 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atel.2905....1p&link_type=abstract

The Astronomer's Telegram, #2905

Astronomy and Astrophysics

Astronomy

2

Radio, Novae, Transients, Variables

Scientific paper

We have made measurements of the 30GHz radio emission from V407 Cyg using the OCRA-p receiver on the Torun telescope between 24 March and 3 October 2010. These follow from the optical and Fermi-LAT detections of the nova outburst (AAVSO Alert 419 / Special Notice 201, ATEL #2487; also see ATEL #2498) and its detections at radio frequency (ATELs #2506, #2511, #2514, #2529, #2536 and #2741). Following from our initial measurements of ~20mJy at 30GHz in late April 2010 (see ATEL #2511), the source brightened to a peak of ~50mJy in mid June before fading to sub-20mJy levels by the end of June.

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