De_Angelis_Alessandro.pdf
De_Angelis_Alessandro.pdf De_Angelis_Alessandro.pdf
edshift z ~ E -2 De Angelis, Galanti, Roncadelli 2011 with Franceschini EBL modeling ray energy (TeV) Alessandro De Angelis Selection bias? New physics ? 20
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- 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: Alessandro De Angelis 19
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- 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
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- 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
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- Page 49 and 50: Alessandro De Angelis Chandra
- Page 52 and 53: Design study phase concluded in Fal
- Page 54 and 55: 100 m 2 dish area 1.2 m mirror face
- Page 56 and 57: Wavelenght range 300 - 600 nm Mirro
- Page 58 and 59: Hardware key elements: - O(100) Tel
- Page 60 and 61: • • Fermi Alessandro De Ang
- Page 62 and 63: 65 2008 2009 2010 2011 2012 2013 2
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- Page 66 and 67: DARMA 3C279 Note: if conversion “
- Page 68 and 69: 1st order (t) obs E H0 E s1
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