De_Angelis_Alessandro.pdf

More documents

Recommendations

Info

World-wide Collaboration 25 countries 132 institutes >800 scientists 10 fold sensitivity of current instruments 10 fold energy range improved angular resolution two sites (North / South) operated as observatory The future in VHE gamma ray astronomy:
Page 1 and 2: • • • 1
Page 3 and 4: • - • - - • - μ μ
Page 5 and 6: hadronic cascades p + (>>TeV) matte
Page 7: edshift z 30 GeV 100 GeV > 1 regio
Page 10: c ~ 1º e Threshold @ sl: 21 MeV Ma
Page 13 and 14: VERITAS: 4 telescopes (~12m) in Ari
Page 15 and 16: • • •
Page 17 and 18: W51: gamma rays come from a molecul
Page 19 and 20: Alessandro De Angelis 19
Page 21 and 22: - - • - • • •
Page 27 and 28: (t) obs 3 2 E E s2 2 1 H0
Page 29 and 30: • -, - • • Alessandro
Page 31 and 32: • • • • Alessandro
Page 33 and 34: • LHC may find candidates but can
Page 35 and 36: 2 arrays: north+south all-sky cove
Page 37 and 38: • - - - • • • - -
Page 39 and 40: 39
Page 41 and 42: Marvel 1961 • • 4
Page 43 and 44: Colours: 0.2 - 6 keV (Chandra) Cont
Page 45 and 46: • • dN dE 1 2 dN dE
Page 47 and 48: • - • - - - 50
Page 49: Alessandro De Angelis Chandra
Page 53 and 54: Carbon-fibre structure 27.8 m foc
Page 55 and 56: Multi-Anode PMT camera option Under
Page 57 and 58: +30 -30 Warning: map not quite acc
Page 59 and 60: * Readout Electronics: fast, low di
Page 61 and 62: HESS map of the Gal.plane, total ex
Page 63 and 64: • • • - • ( - •
Page 65 and 66: La = ga E ( B )a * • •
Page 67 and 68: Alessandro De Angelis HESS, PKS 215
Page 69 and 70: • • • (t) obs E
Page 71 and 72: • - - - 74
Page 73 and 74: v = H p 1 m2 2p 2 + p E P c 2 p 2
Page 75 and 76: GRH depends on the -ray path and th
Page 77 and 78: detection of -rays from GC by Canga
Page 79 and 80: 84

De_Angelis_Alessandro.pdf

Create successful ePaper yourself

Delete template?

Save as template?