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J16021+3326: New Multi-Frequency Observations of a Complex Source

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arxiv 1001.5423 v1 pith:IQGA2GDA submitted 2010-01-29 astro-ph.CO

S.E. Tremblay , G.B. Taylor , J.L. Richards , A.C.S. Readhead , J.F. Helmboldt , R.W. Romani , S.E. Healey This is my paper
classification astro-ph.CO
keywords blazarobservationsj16021sourcealignedalmostalongappear
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We present multifrequency Very Long Baseline Array (VLBA) observations of J16021+3326. These observations, along with variability data obtained from the Owens Valley Radio Observatory (OVRO) candidate gamma-ray blazar monitoring program, clearly indicate this source is a blazar. The peculiar characteristic of this blazar, which daunted previous classification attempts, is that we appear to be observing down a precessing jet, the mean orientation of which is aligned with us almost exactly.

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