Optical follow-up of S5 1803+78

Details Optical follow-up of S5 1803+78 Optical follow-up of S5 1803+78

May 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011atel.3323....1n&link_type=abstract

The Astronomer's Telegram, #3323

Physics

1

Optical, Blazar

Scientific paper

Following the announcement of a Gamma-ray flare of the blazar S5 1803+78 (ATel #3322) on May 2 2011, I observed the source on May 4 2011 at 22:35 UT with the 23 cm telescope on top the Department of Physics of La Sapienza University with an R_C filter and an Apogee U2 CCD camera. Comparison stars were taken from Nesci et al. (2002, AJ 124, 53). The source appeared at R=15.6 ±0.1, an average value for this source, whose large optical flares are at R~14.

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