NIR flaring of the Gamma ray source PKS1550-242

Details NIR flaring of the Gamma ray source PKS1550-242 NIR flaring of the Gamma ray source PKS1550-242

Jul 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atel.2726....1c&link_type=abstract

The Astronomer's Telegram, #2726

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 1FGLJ1553.4-2425 also known as PKS1550-242 with the CANICA NIR camera on the 2.1m telescope at the Observatorio Astrofísico Guillermo Haro, located in Cananea, Mexico. On June 16th, 2010 (JD24555363.741), we found this blazar to be in outburst. It showed fluxes about 1.6 magnitudes brighter than our previous NIR photometry. On this date the source was found to have a flux corresponding to H = 14.615 ± 0.04.

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