PPT-1 DETECTOR TECHNOLOGIES Lecture 1:

Principles of detection Generalities about detectors Interaction of particles with matter 2 Goal Observation and identification of final states whatever. The LEGe detector is fabricated with a thin front and side contact The rear contact is of less than full area which gives a lower detector capacitance compared to a planar device of similar size Since preampli64257er noise increases with detector ca . INITIATIVE. Marzio Nessi, Markus . Nordberg. CERN . What is ATTRACT?. ATTRACT (. breAkThrough. . innovaTion. . pRogrAmme. for . deteCtor. / . inrAstructure. . eCosysTem. ). A . proposal for a dedicated . Xin Qian. BNL. 1. 2015 Sambamurti Lecture: Xin Qian. Outline. The Big Question: . W. hy is there much more matter than anti-matter in our universe?. Is neutrino the key to this question?. The . O. verall Strategy: . John . Vallerga. Space . Sciences Laboratory. University of California, Berkeley. UV/Vis detector(s) for a new Flagship Mission. Large telescopes with large FOVs require large detectors . (e.g. 4m f/3 with 30 arc min . Computer Vision Lecture 10: Edge Detection III. 1. Canny Edge Detector. However, usually there will still be . noise. in the array E[. Ruqayyah Askar. PHYS 689 . April 27, 2018. Outline. Introduction. General principles. Historical overview. Types of IR . detectors. Current IR . technologies. Parameters of IR Detectors. Emerging . Technologies. Markus Nordberg. Porto, October 21 . , 2016. IDEASQUARE IN BRIEF. “. Ideasquare . is . an experiment to bring . together physicists, engineers, industrial partners, early-stage researchers and cross-disciplinary teams of students to work together on detector . PARAMETERS. The . experimental apparatus includes two main detectors: a silicon vertex tracker (SVT) for . precise momentum vertex determination and . and an electromagnetic calorimeter (. ECal. ) to trigger on . DEELS 2016. DESY, 27-28 . June. 2016. Marie LABAT, Nicolas HUBERT. In-Air X-ray Detector. Image of the vertical beam profile. Hard X-rays crossing the crotch absorber behind dipoles magnets.. Design by ESRF (6 GeV) and applied at ANKA (2,5 GeV) and ALBA (3 GeV). ــــــــــــــــــــــــــــــــــــــــــــــــــــــــــــــــــــــــــــــــــــــــــــــــــــ The Desired Brand Effect Stand Out in a Saturated Market with a Timeless Brand The Desired Brand Effect Stand Out in a Saturated Market with a Timeless Brand The Desired Brand Effect Stand Out in a Saturated Market with a Timeless Brand . Hans-Jürgen . Wollersheim. e-mail: h.j.wollersheim@gsi.de. Challenges of . γ. -ray spectroscopy. efficiency vs resolution. Composite HPGe detectors. in ADD BACK mode. Emission at rest. Δ. E=2keV .