PPT-1 Inner detector

upgrade IBL Activities on cooling circuits LAPP LAPP team Jacky Ballansat Patrick BaudinPierreYves David Pierre Delebecque Nicolas MassolThibaut Rambure Theodore . 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. 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, . Further developments of detectors with resistive electrodes:. R. Oliveira. 1. , V. Peskov. 1,2. , F. Pietropaolo. 3. , P. Picchi. 4. 1. CERN, Geneva, Switzerland. 2. NAM, Mexico. 3. INFN Padova, Ialy. 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, . Brian . Kross. – mechanical design and construction / gas systems. Seungjoon. Lee – advanced image recon algorithms / mechanical / detectors. John . McKisson. – software / data acquisition / electronics. 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 . 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 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 . Mike Sullivan. EICUG 2019. July 22-26. Paris, France . 1. Outline. Introduction. Detector Issues. Machine Issues. Unique features of the EIC. Some general questions for the detector and accelerator teams.