Multiwavelength observations of the TeV blazar MRK 501 in March 1996. The first report of the detection by EGRET

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Scientific paper

We present the results of a multiwavelength campaign for Mrk 501 performed in March 1996 with ASCA, EGRET, Whipple, and optical telescopes. We report here for the first time the detection of a GeV gamma-ray flux from Mrk 501 with EGRETwith 3.5 sigma significance (E > 100 MeV). A higher flux was also observed in April/May 1996, with 4.0sigma significance for E > 100 MeV, and 5.2 sigma significance for E > 500 MeV. We find that the multiband spectrum in March 1996 is consistent with that calculated from a one-zone SSC model, except for the extremely `flat' TeV spectrum. We show that the discrepancy cannot be explained by either second order Comptonization or the contribution of the `seed' IR photons from the host galaxy.

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