Detection of optical activity in the radio source B2 0619+33

Details Detection of optical activity in the radio source B2 0619+33 Detection of optical activity in the radio source B2 0619+33

Sep 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atel.2831....1s&link_type=abstract

The Astronomer's Telegram, #2831

Astronomy and Astrophysics

Astronomy

Optical, >Gev, Agn, Blazars

Scientific paper

In response to ATEL #2829, optical observations were obtained on September 7, 2010 for the radio source B2 0619+33 (RA: 06h22m52.221945s, Dec: +33d26m10.41027s, J2000; Kovalev et al. 2007, AJ 133, 1236) with the 1.54m Kuiper Telescope on Mt. Bigelow, Arizona using the SPOL spectropolarimeter. Comparison to two spectrophotometric standard stars yields a V magnitude of 18.48+/-0.03 for the object. This is substantially brighter than seen in the second Digitized Sky Survey (DSS2) plate, where the object is not visible.

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