An AGN Observation Catalogue for the MAGIC Cherenkov Telescope

Physics

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Scientific paper

The 17m diameter MAGIC telescope will become operational in mid-2003. Active Galactic Nuclei (AGN) known to be T eV γ -ray emitters will be observed by the telescope in its initial phase. But, due to the high sensitivity measuring fluxes and low Energy Threshold, MAGIC will be able to observe very high redshifted AGNs which have remained undetected by the present Cherenkov telescopes. The EGRET AGNs and Constamante-Ghisellini T eV BL Lacs candidates are taken as a reference to perform a study of source observability by evaluating their fluxes at the MAGIC energy detection range.

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