NIR Flaring of the QSO CGRaBS J1700+6830

Details NIR Flaring of the QSO CGRaBS J1700+6830 NIR Flaring of the QSO CGRaBS J1700+6830

Jun 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atel.2703....1c&link_type=abstract

The Astronomer's Telegram, #2703

Astronomy and Astrophysics

Astronomy

Radio, Infra-Red, Gamma Ray, Agn, Blazars, Quasars

Scientific paper

We call attention on our recent observation of the Gamma Ray source CGRaBS J1700+6830 also known as RGB J1700+685 with the CANICA NIR camera on the 2.1m telescope at the Observatorio Astrofísico Guillermo Haro, located in Cananea, Mexico. On June 12th, 2010 (JD24555359.892), we found this blazar to be in outburst. It showed fluxes about 2.6 magnitudes brighter than previous NIR photometry. On this date the source was found to have a flux corresponding to K = 10.446 ± 0.05.

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