NIR Flaring of S4 1030+61.

Details NIR Flaring of S4 1030+61. NIR Flaring of S4 1030+61.

May 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atel.2625....1c&link_type=abstract

The Astronomer's Telegram, #2625

Astronomy and Astrophysics

Astronomy

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

Scientific paper

We call attention on our recent observation of the Gamma Ray source 1FGL J1033.8+6048 with the CANICA NIR camera on the 2.1m telescope at the Observatorio Astrofísico Guillermo Haro, located in Cananea, Mexico. We found this blazar to be in outburst. It shows fluxes about 2.7 magnitudes brighter than previous NIR photometry listed in the 2MASS catalog of point sources. Our photometric results in the H Band for the date JD2455335.6830, yield a value of H=13.298 ± 0.05.

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