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. Choice of assembly procedure. Screwing versus . glueing. Pro’s and con’s . MMM Würzburg, 30/01/2014. P. Ponsot/J. Wotschack. 1. Glueing. or screwing ?. The purpose of this presentation is to introduce the discussion on the first choice that we have to make in order to arrive at an agreed assembly procedure. 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.. Lab Methods Day. June 25, 2013. Taylor . Myers. 2. Carbon Monoxide Concentration. % of CO, by volume, in the air. Digital readout. Analog output 0/2/4 to 20 mA. Carbon Dioxide Concentration. % of . CO2, . Lab Methods Day. June 25, 2013. Taylor . Myers. 2. Carbon Monoxide Concentration. % of CO, by volume, in the air. Digital readout. Analog output 0/2/4 to 20 mA. Carbon Dioxide Concentration. % of . CO2, . 2012/3/2. Y.Sugimoto. Background. Request for more space from DESY team. Several installation works in parallel. Depends on total allowed construction perio. d . Design of common cryogenic system. ILD, . 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. Week 3. Very few detectors will count every interaction. Each detector will have its own counting efficiency. Eff. =CPM/DPM. Can use efficiency and count rate to determine amount of material present. 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. side. Wago. 2002-1201 . Wago. 2002-3203 . Door open. 800x600x200 mm. 0.93x60 cm. 10 cm. 4.9 cm. 4.9 cm. GSM cable. Gas pipes. ~25cm. ~25cm. NSYS3D8620. Inputs. Outputs. 600. 8. 00. 200. 60cm. 90 ˚ turn. 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 . Applying G4beamline. Tom Roberts. Muons, Inc.. June 27, 2011 TJR. 1. Machine-Detector Interface 2. Outline. Quick Introduction to G4beamline. Why use it for MDI simulations. G4beamline Capabilities Relevant to MDI Simulations. Innovative silicon sensors for future trackers. N. . Cartiglia. M. . Mandurrino. INFN - Italy. Part II: Principles of operation of RSD. Single point precision and charge sharing. Signal formation. Charge sharing: RSD master formula. 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 .