ICREA Workshop on the High Energy Emission from pulsars and their ...

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In the 30-100 MeV AGILEsensitivity is competitive(500 cm 2 eff. Area for timing).The 1 GeV Fermi sensitivity ismuch better than the AGILE one.
Page 1: ICREA Work
Page 5 and 6: The “soft” γ-pulsar B1509-58AG
Page 7 and 8: Bright Gamma-ray Pulsars (E>50 MeV)
Page 9 and 10: 40000 pulsed countscollected from V
Page 11 and 12: Discarding eventswithin time interv
Page 13 and 14: Discarding eventswithin time interv
Page 15: ph/cm 2 /s/sr0.25x0.25 deg bins
Page 19 and 20: l=263.9, b=-3.2, 6σ
Page 21 and 22: HESSAharonian et al. 2006X-rays-GeV
Page 24 and 25: EGRET U.L.
Page 27 and 28: deJager et al., 2008
Page 31: VELA X in radio (Hales et al., 2004
Page 34 and 35: CMBR FIRStarlightE ph =1 eV
Page 36: Sardinia Radio Telescope (64 m dish
Page 39 and 40: Unidentified gamma-ray sources:PWNe
Page 41 and 42: HESSRADIOAharonian et al. 2006
Page 43 and 44: HESSAharonian et al. 2006

ICREA Workshop on the High Energy Emission from pulsars and their ...

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