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SciNeGHE 2012

19–22 Jun 2012
Lecce
Europe/Rome timezone

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Session

Future Projects

09
22 Jun 2012, 14:10
Lecce

Lecce

Officine Cantelmo

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  1. 7. CALET: a calorimeter for cosmic-ray measurements in space
    Dr Nicola Mori (FI)
    22/06/2012, 14:10
    The CALorimetric ELectron Telescope (CALET) is a space-station-borne experiment aimed at precise measurements of the electron+positron, ion and gamma-ray components of the cosmic-ray spectrum, in an energy range starting from tens of GeV up to tens of TeV. The heart of the detector is a deep (~27 X0) homogeneous calorimeter made by lead tungstate (PWO) scintillating bars, which can...
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  2. 9. The GAMMA-400 Space Experiment: Gammas, Electrons and Nuclei Measurements
    Dr Emiliano Mocchiutti (TS)
    22/06/2012, 14:35
    The present design of the new space gamma-ray telescope GAMMA-400 for the energy range 50 MeV - 3 TeV is presented. The proposed instrument has an angular resolution of 1-2 degrees at E(gamma) ~100 MeV and ~0.01 degrees at E(gamma) > 100 GeV and an energy resolution ~1% at E(gamma) > 100 GeV. By the mean of a deep segmented calorimeter high energy electrons flux can be studied, with a...
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  3. 51. The Cerenkov Telescope Array (CTA)
    Massimo Persic (INAF Trieste and INFN)
    22/06/2012, 15:00
    The CTA project will be reviewed.
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  4. 63. Science with the ASTRI prototype
    Nicola SARTORE (INAF - Milano)
    22/06/2012, 15:25
    ASTRI is a flagship project of the italian Ministry of Instruction, University and Research and represents the italian proposal for the development of the Small Scale Telescope (SST) system of the Cherenkov Telescope Array (CTA), which is the planned next generation observatory for very high energy gamma-rays (20 GeV - 100 TeV). The ASTRI (Astrofisica a Specchi con Tecnologia Replicante...
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  5. 22. Status and updates from the High Altitude Water Cherenkov (HAWC) Observatory
    Dr Brian Baughman (University of Maryland, College Park)
    22/06/2012, 15:40
    The High Altitude Water Cherenkov Observatory (HAWC) is currently being deployed on the slopes of Volcan Sierra Negra, Puebla, Mexico. The HAWC observatory will consist of 300 Water Cherenkov Detectors totaling approximately 22,000 m^2 of instrumented area. The water Cherenkov technique allows HAWC to have a nearly 100\% duty cycle and large field of view, making the HAWC observatory an ideal...
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  6. 61. The LHAASO project
    Cunfeng Feng (Shandong University)
    22/06/2012, 16:05
    The LHAASO project will be described
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  7. 34. An overview of the JEM-EUSO mission
    Dr Mario Edoardo Bertaina (INFN Torino)
    22/06/2012, 16:30
    JEM-EUSO will be the first observatory to explore from space the universe at ultra-high energies. Hosted on the JEM platform on board the ISS, it will use an innovative refractive optics and sophisticated focal surface to observe the UV fluorescence light emitted, in the 320-400 nm band, by extensive air showers generated by primary particles interacting in the atmosphere. The telescope...
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