Striani, E.E.StrianiPiano, G.G.PianoTavani, M.M.TavaniPittori, CarlottaCarlottaPittoriVerrecchia, FrancescoFrancescoVerrecchiaGiommi, PaoloPaoloGiommiSantolamazza, P.P.SantolamazzaLucarelli, FabrizioFabrizioLucarelli2020-09-172020-09-172011-04-01https://hdl.handle.net/20.500.13025/2171The Astronomer's Telegram, #3286Strongly variable gamma-ray emission above 100 MeV continues to be detected by AGILE from a source positionally consistent with the Crab Nebula. After a telemetry gap that AGILE experienced on April 14, 2011 (in partial coincidence with the strong gamma-ray flare reported by Fermi-LAT in ATel # 3284) the AGILE-GRID detected the following gamma-ray flux above 100 MeV (pulsar plus nebula) MJD=55666.44-55667.44, 2011-04-15 10 40 UT - 2011-04-16 10 38 UT, F = (19.6 3.7) 10^{-6} ph/cm2/sec.Gamma RayNeutron StarSupernova RemnantTransientPulsarhttp://adsabs.harvard.edu/abs/2011ATel.3286....1S2011ATel.3286....1S