Title: Leonidas K. Resvanis NESTOR Institute for Astroparticle Physics National Observatory of Athens and Physics Department University of Athens ISCRA / Erice
1Leonidas K. ResvanisNESTOR Institute for
Astroparticle PhysicsNational Observatory of
AthensandPhysics DepartmentUniversity of
AthensISCRA / Erice July 2008
2ANSWERS TO QUESTIONS ON THE FIRST LECTURE
3(No Transcript)
4(No Transcript)
5(No Transcript)
6(No Transcript)
7DELTA-BERENIKE
-
- DEPLOYMENT PLATFORM WHICH WILL ALSO CARRY THE
SCINTILLATOR - SURFACE ARRAY (1500m2) FOR THE ABSOLUTE
CALIBRATION USING AIR SHOWERS
8(No Transcript)
9SECOND LECTURE. BAIKAL
10(No Transcript)
11(No Transcript)
12(No Transcript)
13(No Transcript)
14(No Transcript)
15(No Transcript)
16(No Transcript)
17(No Transcript)
18NESTOR
19(No Transcript)
20(No Transcript)
21(No Transcript)
22(No Transcript)
232003
Successful deployment of one NESTOR star with 12
Optical Modules to 4000m using the cableship
RAYMOND CROZE (FranceTelecom) 29th of March
The first deep sea muon data transmitted
to shore
24(No Transcript)
25(No Transcript)
26(No Transcript)
27Run 81_72 Event 236
c
28(No Transcript)
29SEE ASTROPARTICLE PHYSICS 23(2005), 377-392 NIM
A 552(2005) 420-439
30NEMO
31(No Transcript)
32(No Transcript)
33(No Transcript)
34(No Transcript)
35ANTARES
36(No Transcript)
37(No Transcript)
38(No Transcript)
39(No Transcript)
40J. CARR NEUTRINO 2008
41J. CARR NEUTRINO 2008
42J. CARR NEUTRINO 2008
43ICECUBE AMANDA
44(No Transcript)
45(No Transcript)
46(No Transcript)
47Albrecht Karle, March 2008
48(No Transcript)
49(No Transcript)
50Carefully model optics of ice!
Dark and transparent environment for Cherenkov
light detection Polar ice ??abs (blue)
100-200 m leff. scat 25 m
IceCube new strings compared to string 48
dust layer
muon energy loss in the detector
50
51(No Transcript)
52IceCube 9 (data)
sigma
- IceCube 9 String Configuration June 2006 --
November 2006 137.4 days livetime - With Quality Cuts
- Real Data 233 neutrino event candidates
- Atmospheric neutrino rate 1.7 per day
- median angular resolution 2.0
Albrecht Karle March 2008
53Albrecht Karle March 2008
54Albrecht Karle March 2008
55Diffuse fluxes
Where do we stand? diffuse fluxes
Albrecht Karle March 2008
WB about 50 events/km2/year above 300 TeV
56(No Transcript)
57(No Transcript)
58(No Transcript)
59(No Transcript)
60(No Transcript)
61(No Transcript)
62Albrecht Karle March 2008
63KM3NeT
Conceptual Design Report
64(No Transcript)
65(No Transcript)
66(No Transcript)
67(No Transcript)
68(No Transcript)
69(No Transcript)
70(No Transcript)
71(No Transcript)
72(No Transcript)
73(No Transcript)
74(No Transcript)
75(No Transcript)
76(No Transcript)
77(No Transcript)
78My personal preferences (distances may change)
79(No Transcript)
80(No Transcript)
81(No Transcript)
82(No Transcript)
83NUBE
84Neutrino Burst Experiment (NuBE) The NESTOR
collaboration U.C.Berkeley/Space Sciences
Lab SUNYSB
85(No Transcript)
86(No Transcript)
87(No Transcript)
88(No Transcript)
89(No Transcript)
90(No Transcript)
91(No Transcript)
92(No Transcript)
93(No Transcript)
94DEPLOYMENTS
95DELTA-BERENIKE
-
- DEPLOYMENT PLATFORM WHICH WILL ALSO CARRY THE
SCINTILLATOR - SURFACE ARRAY (1500m2) FOR THE ABSOLUTE
CALIBRATION USING AIR SHOWERS
96(No Transcript)
97ANTARES J. CARR NEUTRINO 2008
98(No Transcript)
99(No Transcript)
100(No Transcript)
101(No Transcript)
102(No Transcript)