Slide 1 What the Lund/Dubna group wishes to achieve until next annual meeting produce two* close-to-final (forward) EGPA clusters requiresCsI(Tl) decided (alternatives?,doping…

Slide 1 „the perfect stopped beam experiment“ clean fragment separation   unique fragment identification  A, Z fragment position  x, y, z decay radiation…

Slide 1 Absolutely Calibrating an Energy Dispersive Detector Patrick Ross Spring Research Conference Slide 2 Why? Absolute Calibration provides more information. Applications…

Thermal Analysis: Differential Scanning Calorimetry (DSC) Professor Maria L. Auad E-mail: [email protected] Phone: 334 844-5459 Office: 103 Textile Building 2 Introduction…

Slide 1 1 Super-Kamiokande atmospheric neutrinos Results from SK-I atmospheric neutrino analysis including treatment of systematic errors Sensitivity study based on improved…

Slide 1 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: Skobeltsyn…

March 22, 2011 Mike Hildreth – ALCPG 2011, Beam Instrumentation Energy Spectrometer R&D; Plans for End Station A Test Beams Mike Hildreth University of Notre Dame ALCPG,…

PowerPoint Presentation LOLA setup simulated LOLA measurement*: no transverse beam dimensions imaging: entrance-LOLA to OTR simulated LOLA measurement*: gaussian transverse…

Energy Calibration with Compton Data June 23, 2006 Outline Revisit “Z” using DA Compton calibration SA Compton calibration Using production on carbon, lead SA gains vs…

NEMO-3 bb experiment First Results and Future Prospects Ruben Saakyan, UCL UK HEP Neutrino Forum The Cosener’s House, Abingdon Outline Why NEMO-3 ? The Detector First results…