'Track direction' presentation slideshows

Introducing MINER n A

Introducing MINER n A. Kevin McFarland University of Rochester 30 March 2006. MINERvA in a Nutshell. MINERvA is a dedicated neutrino cross-section experiment operating in the NuMI near hall in a unique position to provide critical input for world neutrino oscillation program

943 views • 72 slides

Speed: 3D sensors, current amplifiers

Speed: 3D sensors, current amplifiers. Cinzia Da Via Manchester University Giovanni Anelli, Matthieu Despeisse 1 , Pierre Jarron CERN Christopher Kenney, Jasmine Hasi, SLAC Angela Kok SINTEF Sherwood Parker University of Hawaii Initial work and calculations with Julie Segal

663 views • 56 slides

In Search of the Rings

In Search of the Rings. (not the session-chair). Approaches to Cherenkov Ring Finding and Reconstruction in HEP. Guy Wilkinson, Oxford University RICH 2007, Trieste, October 2007. First some excuses, admissions and warnings.

376 views • 37 slides

Lecture 5: Asteroid Discovery and Characterization Using Stellar Occultation

Lecture 5: Asteroid Discovery and Characterization Using Stellar Occultation. 1. On the Idea Of Shadows.

283 views • 19 slides

Gamma-ray Large Area Space Telescope

Gamma-ray Large Area Space Telescope. TKR Distributions Michael Kuss INFN Pisa LAT CU Beam Test Kick-Off Workshop 20 March 2006. Requirements. Existing Information. full description on the LAT IA group web page (or the workbook) digi root file : almost everything from the XxxDigi TDS

167 views • 16 slides

Offline tau reconstruction overview

Offline tau reconstruction overview. M. Pilar Casado (IFAE & UAB). Introduction tauRec tau1P3P AOD and ESD Conclusion. t Decays. ~35%, but they belong to another story. t decay modes Leptonic decay modes t ? n t + n e + e (17.4%)

217 views • 14 slides

Impact Parameter Tag

238 views • 12 slides

Future prospects for large area ground & space-based neutrino detectors

Future prospects for large area ground & space-based neutrino detectors. Peter Gorham JPL Tracking & Applications Section 335 RADHEP 2000. UHE/EHE Neutrino Detector Possibilities. Of order 10^43 nucleons if we want ~100 GZK nu events per year at >10^18 eV

198 views • 8 slides