engleski

Follow-up observations on serendipitous sources observed by MAGIC

Many sources have been observed by MAGIC so far. In stereoscopic mode, more than 1400 hours of data have been taken. MAGIC camera field of view has diameter of 3.5 degrees, covering relatively large area in the sky observed for all sources in total. The idea is to use the data the MAGIC has already observed, in order to look for new FERMI sources observed in the same FOV. All MAGIC stereo observations have been checked, taking in account their wobble positions . Total observed time in dark and Moonlight conditions was checked, for galactic sources, extragalactic sources, and dark patches. Coordinates of MAGIC observations were compared with coordinates of FERMI objects (in 2FGL, and still unpublished 3FGL catalogue) in order to find potential candidates. 71 sources from still unpublished 3FGL catalogue were found in our observed FOV, within 1.2 deg from the primary sources observed by MAGIC. Once upper limits are derived, it can serve as a starting point for estimating observing time needed for candidates that can be proposed for the next MAGIC observing cycle.

gamma rays: observations; galaxies: active

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