Detection of an increase in the flux density at 43 GHz from blazar PKS 1510-089 since August, 2011

Details Detection of an increase in the flux density at 43 GHz from blazar PKS 1510-089 since August, 2011 Detection of an increase in the flux density at 43 GHz from blazar PKS 1510-089 since August, 2011

Dec 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011atel.3799....1b&link_type=abstract

The Astronomer's Telegram, #3799

Astronomy and Astrophysics

Astronomy

Radio, Agn, Blazar

Scientific paper

We have been performing monthly observations of PKS1510-089 at 43 GHz since 2011 January, using the Itapetinga Radio telescope (13.7 m antenna installed at Atibaia, Brazil). We already reported the variability behavior during the July gamma ray flare (ATel #3523, following the communication from Atel #3470 and Atel #3473,). In the occasion, the blazar was relatively bright at 43 GHz, but we concluded that the source behavior was not different from the observed since the beginning of the year(Atel #3523).

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