PPT-AST3 detector properties

Ma Bin NAOC 20150309 2015 AST3 meetingHKU OUTLINE 1 AST3 CCD 2 CCD test results 3 Nonlinear PTC 4 Current status 1 AST3 CCD STA 1600FT 10560 10560 pixels Pixel size 9 μ m gt 1. 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 of Plastic Scintillator. Oct. 2, 2009. IP-BSM Group. 1. Schematic . Drawing . of. new Gamma Detector. 2. sandwich type calorimeter. SUS and plastic scintillation plate. wavelength-shifting fiber (WLSF) for light transmission. Bin Ma, . Peng. Wei, Yi . Hu. , . Zhaohui. Shang. NAOC. 2015.03.10. 2015 AST3 . meeting@HKU. Variables by . Lingzhi. Wang. Outline . 1 Overview of the data . 2 Image Reduction. 3 Astrometry. 4 Aperture Photometry. Brennan Thomason. Tamara Reed. Edmond Wilson. Project Goal. Design a detector for a high resolution spectrograph that provides electromagnetic radiation intensity data as a function of wavelength in the range of 400 nm to 1000 nm.. Lifan Wang. TAMU/CCAA. The Site. Dome A . Elevation 4,091 m (13,422 ft). Coordinates: -80d22m, E77d 21m . The highest peak on the Plateau. Marching toward Antarctica. A team of Pioneers led by . Yuanshen. M. Sullivan. Mini-workshop on the MEIC design. Nov 2, 2012. Introduction. Accelerator Parameters. Previous Synchrotron . R. adiation estimates. Other SR issues. Other detector backgrounds. Points of Interest. for the AST3-3 telescope for the Kunlun Infrared Sky Survey (KISS). Progress Meeting. Jon Lawrence. 14 August 2015. Project Aims and Objectives. Project Personnel. Project Roles. Jeremy . Mould (SUT) as Lead Investigator. Philip Anderson. National Sales Manager. System Sensor Canada. A hospital is like a city. Living areas. Machinery, high technology. Food prep/service. Retail, public spaces. Open spaces, parking. Wide range of application challenges. MicroTCA. platform with embedded sub-ns WR synchronization. G. .. Kasprowicz (WUT). 2. Outline. NICA . collider. & . Cosmic Ray Detector – Goals. SIPM AFE. SIPM readout chain based on Open Source HW. FCC week Washington. 23. -27 March . 2015. W. . Riegler. D. . Denisov. , H. . ten. Kate, L. . Lienssen. , F. . Lanni. , M. . Abbrescia. , R. Richter, Y. . Onel. , W. Smith, S. . C. hekanov. Exploration + Higgs as a tool for . 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 . results during isotopic analysis Traditionally it was recodetector with a full width half-maximum FWHMHowever in many cases when using large detectors or when using a short amplifier time constant thi 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). Previous work [1] studied the use of PTP and Synchronous Ethernet (. SyncE. ) for synchronization of detector data from multiple Pixie-Net modules, an earlier and smaller version of the digitizing and pulse processing electronics described here. The time resolution for coincident events reached ~10ns FWHM with PTP synchronization and 200-800ps FWHM with .