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

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

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

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AGILE counts > FermiE AGILEE>1 GeVPellizz<strong>on</strong>i et al. 2009Abdo et al. 2009

The “soft” γ-pulsar B1509-58AGILE (Pilia et al.)Fermi (Abdo et al.)

Page 1: ICREA Work
Page 6 and 7: The “soft” γ-pulsar B1509-58Pe
Page 8 and 9: AGILEMt. Pleasant(Hobart, Tasmania)
Page 10 and 11: Vela Pulsar hides nearly 100 square
Page 12 and 13: Discarding eventswithin time interv
Page 14 and 15: Vela
Page 17: l=263.1, b=0.6, 5σ, new unidentifi
Page 20 and 21: Chandra
Page 22: Flux E>100 MeV= 35x10 -8 ph/cm 2 /s
Page 25: L AGILE =4x10 33 erg/s (0.1-10 GeV)
Page 28: CMBR FIRStarlight
Page 33 and 34: 8.4 GHz
Page 35 and 36: deJager et al., 2008
Page 38 and 39: ~85 Non-Variable EGRET Unidentified
Page 40 and 41: About 40 bright (E ROT >10 35 erg/s
Page 42 and 43: HESSAharonian et al. 2006
Page 44: ICREA Work