1 Super-Kamiokande atmospheric neutrinos Results from SK-I atmospheric neutrino analysis including treatment of systematic errors Sensitivity study based.
Space fluorescence detectors TUS/KLYPVE for study of UHECR. 18 October 2005 B. A. KHRENOV 18 October 2005 B. A. KHRENOV for TUS/KLYPVE collaboration of:
Constraining the EoS and Symmetry Energy from HI collisions Statement of the problem Demonstration: symmetric matter EOS Laboratory constraints on the.
Energy Spectrometer R&D; Plans for End Station A Test Beams
LOLA setup simulated LOLA measurement*: no transverse beam dimensions imaging: entrance-LOLA to OTR simulated LOLA measurement*: gaussian transverse shape.
Outline: Introduction Some experimental remarks Extra Dimensions (ADD, TeV -1 , RS, UED, BH)
07-29-05PrimEx collaboration meeting Energy calibration of the Hall B bremsstrahlung tagging system using magnetic pair spectrometer S. Stepanyan (JLAB)
Framework
Overview of Energy Spectrometers
RECONSTRUCTION ALGORITHM CALIBRATION OBJECT ESD STRUCTURE ONGOING TASKS
NEMO-3 experiment First Results and Future Prospects Ruben Saakyan, UCL UK HEP Neutrino Forum The Cosener’s House, Abingdon.
Auger New Results G. Matthiae Universita’ e Sezione INFN di Roma “Tor Vergata”
