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WP2 Physics analysis and simulation. Ressources. People. Objectives. In few months…. Neil McCauley (AC) 2 post-docs 1(+) student. People involved. Current. Stella Bradbury (AC) Fabrice Jouvenot (PostDoc) Joachim Rose (AC) Lee Thompson (AC) Christos Touramanis (AC).
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WP2Physics analysis and simulation Ressources People Objectives
In few months… • Neil McCauley (AC) • 2 post-docs • 1(+) student People involved Current • Stella Bradbury (AC) • Fabrice Jouvenot (PostDoc) • Joachim Rose (AC) • Lee Thompson (AC) • Christos Touramanis (AC) Ressources People Objectives
Galactic latitude Galactic longitude SNR distribution νμ+νμon Earth HN model E2 x Neutrino flux [particles MeV s-1 cm-2] HE model C model HEMN model Calibration Software Energy [MeV] • Time calibration (cf. WP 3) Objectives Benchmark neutrino fluxes • Diffuse flux of galactic neutrinos • (Egret, AMS, HESS) • Accumulation of point sources SNR, GRB, AGN • (HESS, VERITAS) • Galactic dark matter Detector geometries Reconstruction & Shape recognition Ressources People Objectives
Resources Computing power • 150 - 3GHz CPU • each machine containing • 1GB RAM and 120Gb disk Ressources People Objectives