ORIGAMIX CURRENT STATE OF A TECHNOLOGY TRANSFER PROJECT FROM SPACE GRADE HIGH ENERGY SPECTRO-IMAGER TO COMMERCIAL GRADE GAMMA CAMERA
|
|
|
- Sabrina Warren
- 5 years ago
- Views:
Transcription
1 ORIGAMIX CURRENT STATE OF A TECHNOLOGY TRANSFER PROJECT FROM SPACE GRADE HIGH ENERGY SPECTRO-IMAGER TO COMMERCIAL GRADE GAMMA CAMERA Pierre-Anne BAUSSON CEA Saclay DRF/Irfu B. 709 p. 27 B. 141 p. 104 CEA OCTOBER 31, 2012 PAGE 1 MAY 24TH 2016 CEA SACLAY
2 SUMMARY ORIGAMIX Personal & project introduction Existing CALISTE technology Project tasks & organization Compton-effect based algorithm development Embedded modular system design Space technology downgrading Tests, results and current state of project Remaining steps & Perspectives Conclusion Pierre-Anne Bausson - DRF/Irfu/SAp May PAGE 2
3 PERSONAL INTRODUCTION 25 years old INSA Lyon electronics engineer 1 year finished term finished 3 weeks ago Now : Permanent same research institute but a more technical department Pierre-Anne Bausson - DRF/Irfu/SAp May PAGE 3
4 PROJECT INTRODUCTION ANR : French National funding Agency for Research RSNR : Radioprotection & Nuclear Safety Research projects call ORIGAMIX Stands for : localisation de la Radioactivité par Imageurs GAMma pixellisés pixelated GAMma Imager for Radioactivity location Pierre-Anne Bausson - DRF/Irfu/SAp May PAGE 4
5 PROJECT INTRODUCTION Main goal : Design a new generation of gamma imager Specifications : Smaller / Easier-to-use system Better spectroscopic resolution Higher energy range Innovative Compton effect-based source location algorithm Pierre-Anne Bausson - DRF/Irfu/SAp May PAGE 5
6 PROJECT ORGANIZATION Consortium : CEA : DRF/Irfu DRT/LIST DEN/MAR 3Dplus Areva Canberra IRSN GIE INTRA CEA DRF/Irfu roles : Third generation 3G gamma camera prototype development Embedded modular system design Acquisition chain electronics design Compton effect based location algorithm CALISTE space technology downgrading / cost optimization Pierre-Anne Bausson - DRF/Irfu/SAp May PAGE 6
7 PROJECT INTRODUCTION So how to do this? Pierre-Anne Bausson - DRF/Irfu/SAp May PAGE 7
8 HIGH ENERGY PHYSICS DETECTION Higher energy Shorter wavelength High energy physics OR Nuclear safety energy domains Pierre-Anne Bausson - DRF/Irfu/SAp May PAGE 8
9 FROM ASTROPHYSICS TO DETECTOR SPECS Compact Objects Point sources Continuum spectra Gamma Ray Bursts Point sources Light curves Continuum spectra Space applications Wide field imaging High angular resolution Wide energy band High energy resolution Time resolution Supernovae remnants Line spectra Point or diffuse sources ( 44 Ti, 57 Co, 56 Fe, ) Diffuse Emission Fine spectroscopy ( 26 Al, 511 kev) Extended sources
10 CALISTE-HD TECHNOLOGY Caliste HD design and technology IDeF-X HD ASIC 32 analog channels CdTe 256-pixel detector (625 µm pitch, 1 or 2 mm thick, Al Scho ky) + (Pt entrance electrode) Moun ng on PCB 8 ASIC stacking perpendicular to the detec on surface Caliste-HD camera Top surface prepara on Electrical body with a 4 x 4 pin grid array Pierre-Anne Bausson - DRF/Irfu/SAp May PAGE 10
11 COMPTON EFFECT The Compton effect : Significant effects for E0 > 100 kev Deposited entirely inside the detector shortly after scattering θ Φ Klein-Nishina formula : Pierre-Anne Bausson - DRF/Irfu/SAp May PAGE 11
12 LOCATION ALGORITHM PRINCIPLE Source is at the circles junction Compton diffusion E 1 e - absorption in CdTe Scattered lower-energy photon E 2 photoelectric absorption in CdTe Pierre-Anne Bausson - DRF/Irfu/SAp May PAGE 12
13 RESULTS WITH MACSI Detector plane Located source «Ghost source» Detector axis Ceiling Ground In front of the detector Behind the detector Pierre-Anne Bausson - DRF/Irfu/SAp May PAGE 13
14 CUBE CORNER CONFIGURATION Detector planes in corner cube : Corner cube system assembly: Simulation results : Pierre-Anne Bausson - DRF/Irfu/SAp May PAGE 14
15 EMBEDDED MODULAR SYSTEM DESIGN Flexible PCB Pierre-Anne Bausson - DRF/Irfu/SAp May PAGE 15
16 INNER PARTS Pierre-Anne Bausson - DRF/Irfu/SAp May PAGE 16
17 FIRST BATCH INTEGRATION Pierre-Anne Bausson - DRF/Irfu/SAp May PAGE 17
18 BONDINGS Pierre-Anne Bausson - DRF/Irfu/SAp May PAGE 18
19 FIRST BATCH INTEGRATION Pierre-Anne Bausson - DRF/Irfu/SAp May PAGE 19
20 WIX MODULE SCALE Pierre-Anne Bausson - DRF/Irfu/SAp May PAGE 20
21 FIRST WIX MODULE READY Pierre-Anne Bausson - DRF/Irfu/SAp May PAGE 21
22 ENVIRONMENT CONTROL STATION Pierre-Anne Bausson - DRF/Irfu/SAp May PAGE 22
23 ISOLATION CLAMPING Pierre-Anne Bausson - DRF/Irfu/SAp May PAGE 23
24 TESTS AT CEA LIST NOV 20, 2015 Coded mask configuration Pierre-Anne Bausson - DRF/Irfu/SAp May PAGE 24
25 Nov. 20, Pierre-Anne Bausson - DRF/Irfu/SAp May PAGE 25
26 Pierre-Anne Bausson - DRF/Irfu/SAp May PAGE 26
27 WIX SPECTRAL RESPONSE Nov. 20, MBq 241 Am Tacq ~ 2min Low energy absorbed by steel encapsulation of the source 930 ev FWHM 60keV In 2 minutes Pierre-Anne Bausson - DRF/Irfu/SAp May PAGE 27
28 WIX SPECTRAL RESPONSE Tacq ~ 8s 600 single events Pierre-Anne Bausson - DRF/Irfu/SAp May PAGE 28
29 WIX SPECTRAL RESPONSE Tacq ~ 800ms 60 singles Pierre-Anne Bausson - DRF/Irfu/SAp May PAGE 29
30 WIX SPECTRAL RESPONSE Tacq ~ 400ms 30 singles Pierre-Anne Bausson - DRF/Irfu/SAp May PAGE 30
31 ORIGAMIX FINAL SYSTEM DESIGN Pierre-Anne Bausson - DRF/Irfu/SAp May PAGE 31
32 ORIGAMIX FINAL SYSTEM DESIGN Xilinx Zynq System on Chip (SoC) Pierre-Anne Bausson - DRF/Irfu/SAp May PAGE 32
33 ORIGAMIX DATA FLOW Pierre-Anne Bausson - DRF/Irfu/SAp May PAGE 33
34 CALISTE-O INDUSTRIAL GRADE DETECTOR 800µm pixel pitch 400µm between two pixel pixel size 16x16 physical pixels Same IDeF-X HD ASIC use inside Optimization of industrial manufacturing process Use of non-space qualified industrial technologies and parts when possible New CALISTE-O detector design s response validated by simulation Pierre-Anne Bausson - DRF/Irfu/SAp May PAGE 34
35 CONCLUSION ORIGAMIX First modules are ready and functional First tests are a good proof of concept Compton configuration tests coming soon Caliste-O : Cost optimized CALISTE design in progress Final system design and acquisition chain releases soon! What s next? Modular and flexible Hardware & Software architectures are ready for further developments and optimizations! On site demonstration campaign at CEA Marcoule nuclear center planned during this September. Pierre-Anne Bausson - DRF/Irfu/SAp May PAGE 35
36 ACKNOWLEDGEMENTS Thank you to all the ORIGAMIX project team : H. Bervas DRF/Irfu/SEDI C. Blondel DRF/Irfu/SAp F. Bouyjou DRF/Irfu/SEDI F. Carrel DRT/LIST/DM2I G. Daniel DRF/Irfu/SAp C. Delisle DRF/Irfu/SAp L. Dumaye DRF/Irfu/SAp C. Force DRT/LIST/DM2I O. Gevin DRF/Irfu/SEDI A. Gros DRF/Irfu/SAp S. Herve DRF/Irfu/SEDI D. Huynh DRF/Irfu/SAp P. Laurent DRF/Irfu/SAp H. Lemaire DRT/LIST/DISC O. Limousin DRF/Irfu/SAp J. Martignac DRF/Irfu/SAp Y. Menesguen DRT/LIST/DM2I A. Meuris DRF/Irfu/SAp T. Orduna DRF/Irfu/SAp F. Pinsard DRF/Irfu/SAp D. Renaud DRF/Irfu/SAp S. Schanne DRF/Irfu/SAp V. Schoepff DRT/LIST/DM2I MC. Vassal 3Dplus And many curious people Pierre-Anne Bausson - DRF/Irfu/SAp May PAGE 36
37 THANK YOU FOR YOUR ATTENTION Pierre-Anne Bausson - DRF/Irfu/SAp May PAGE 37
ORIGAMIX, A CDTE-BASED SPECTRO-IMAGER DEVELOPMENT FOR NUCLEAR APPLICATIONS
ORIGAMIX, A CDTE-BASED SPECTRO-IMAGER DEVELOPMENT FOR NUCLEAR APPLICATIONS Sébastien Dubos 1 Hermine Lemaire 2 Frédérick Carrel 2 Olivier Limousin 1 Aline Meuris 1 Stéphane Schanne 1 Vincent Schoepff 2
CALISTE and its applications
CALISTE and its applications Daniel Maier 1, P.A. Bausson 2, C. Blondel 1, F. Carrel 3, G. Daniel 1, C. Force 3, O. Gevin 2, H. Lemaire 3, O. Limousin 1, D. Renaud 1, J. Martignac 1, A. Meuris 1, V. Schoepff
Development of High-Z Semiconductor Detectors and Their Applications to X-ray/gamma-ray Astronomy
Development of High-Z Semiconductor Detectors and Their Applications to X-ray/gamma-ray Astronomy Taka Tanaka (SLAC/KIPAC) 9/19/2007 SLAC Advanced Instrumentation Seminar Outline Introduction CdTe Diode
Compton Camera. Compton Camera
Diagnostic Imaging II Student Project Compton Camera Ting-Tung Chang Introduction The Compton camera operates by exploiting the Compton Effect. It uses the kinematics of Compton scattering to contract
New trends in CdTe detectors for X and γ-ray applications
New trends in CdTe detectors for X and γ-ray applications Olivier Limousin CEA Saclay / DSM / DAPNIA Service d Astrophysique France New developments in photodetection, Beaune 2002 / Solid state detectors
Semi conductor detectors for soft gamma-ray astrophysics
Semi conductor detectors for soft gamma-ray astrophysics François Lebrun APC (UMR 7164), CEA-Saclay ISGRI PI IWORID 2005 Grenoble High-energy astronomy specific telescopes X-rays and gamma rays radio,
Application of Nuclear Physics
Application of Nuclear Physics Frontier of gamma-ray spectroscopy 0.1 IR visible light UV soft X-ray X-ray hard X-ray gamma-ray 1 10 100 1e3 1e4 1e5 1e6 energy [ev] Photoelectric effect e - Compton scattering
IPNDV Working Group 3: Technical Challenges and Solutions Nuclear Material (3) Technology Data Sheet
Nuclear Material (NM) Technology Name: Gamma-Ray Imaging Physical Principle/Methodology of Technology: Gamma-ray imaging provides the location and shape information of gamma-ray emitting radionuclides.
A NEW GENERATION OF GAMMA-RAY TELESCOPE
A NEW GENERATION OF GAMMA-RAY TELESCOPE Aleksandar GOSTOJIĆ CSNSM, Orsay, France 11 th Russbach School on Nuclear Astrophysics, March 2014. Introduction: Gamma-ray instruments GROUND BASED: ENERGY HIGHER
Development and characterization of 3D semiconductor X-rays detectors for medical imaging
Development and characterization of 3D semiconductor X-rays detectors for medical imaging Marie-Laure Avenel, Eric Gros d Aillon CEA-LETI, DETectors Laboratory marie-laure.avenel@cea.fr Outlines Problematic
Maximum-Likelihood Deconvolution in the Spatial and Spatial-Energy Domain for Events With Any Number of Interactions
IEEE TRANSACTIONS ON NUCLEAR SCIENCE, VOL. 59, NO. 2, APRIL 2012 469 Maximum-Likelihood Deconvolution in the Spatial and Spatial-Energy Domain for Events With Any Number of Interactions Weiyi Wang, Member,
The Path From COSI to COSI-X
The Path From COSI to COSI-X Andreas Zoglauer, UC Berkeley for the COSI / COSI-X collaboration Instruments & Campaigns COSI Balloon-borne Compton telescope Energy range: 0.2 5.0 MeV 12 high-purity Ge double-sided
Performance of the Gamma-ray Imaging Detector with Micro-TPC
Performance of the Gamma-ray Imaging Detector with Micro-TPC Cosmic-Ray Group Dept. of Physics, Graduate School of Science, Kyoto University R.Orito Orito,H.Kubo,K.,H.Kubo,K.Miuchi,T.Nagayoshi, A.Takada,A.Takeda,T.Tanimori
Development of a new MeV gamma-ray camera
Development of a new MeV gamma-ray camera ICEPP Symposium February 16, 2004 Hakuba, Nagano, Japan Kyoto University Atsushi Takeda H. Kubo, K. Miuchi, T. Nagayoshi, Y. Okada, R. Orito, A. Takada, T. Tanimori,
X- & γ-ray Instrumentation
X- & γ-ray Instrumentation Used nuclear physics detectors Proportional Counters Scintillators The Dark Ages Simple collimators HEAO A1 & A2: 2 x 8 degree field of view Confusion limit is about 200 sources
Status of the TRACE array
Status of the TRACE array D. Mengoni University of the West of Scotland, Paisley - U.K. INFN - Sezione di Padova, Padova - Italy SPES workshop, LNL - Italy Nov 15 th 17 th, 2010 Outline 1 Introduction
Detector R&D at KIPAC. Hiro Tajima Kavli InStitute of Particle Astrophysics and Cosmology
Detector R&D at KIPAC Hiro Tajima Kavli InStitute of Particle Astrophysics and Cosmology Detector R&D Overview Si detector ASIC Integration GLAST GeV Gamma-ray Observatory ASIC DAQ Next generation X-ray
Development of a Hard X-Ray Polarimeter for Solar Flares and Gamma-Ray Bursts
Development of a Hard X-Ray Polarimeter for Solar Flares and Gamma-Ray Bursts M.L. McConnell, D.J. Forrest, J. Macri, M. McClish, M. Osgood, J.M. Ryan, W.T. Vestrand and C. Zanes Space Science Center University
Position Sensitive Germanium Detectors for the Advanced Compton Telescope
Position Sensitive Germanium Detectors for the Advanced Compton Telescope R.A. Kroeger 1, W.N. Johnson 1, J.D. Kurfess 1, B.F. Phlips, P.N. Luke 3, M. Momayezi 4, W.K. Warburton 4 1 Naval Research Laboratory,
X-ray polarimetry and new prospects in high-energy astrophysics
X-ray polarimetry and new prospects in high-energy astrophysics Carmelo Sgrò INFN Pisa carmelo.sgro@pi.infn.it Frascati, March 31, 2016 A new exploration window: X-Ray polarimetry Spectroscopy, imaging
Soft Gamma-ray Detector (SGD) for the NeXT mission and beyond Astro-E2 Tadayuki Takahashi
T.Takahashi, Astronomy with Radioactivies IV,2003 Soft Gamma-ray Detector (SGD) for the NeXT mission and beyond Astro-E2 Tadayuki Takahashi Institute of Space and Astronautical Science (ISAS, Japan) 2005
arxiv: v1 [physics.ins-det] 11 Dec 2015
![arxiv: v1 [physics.ins-det] 11 Dec 2015](/thumbs/94/119833631.jpg "arxiv: v1 [physics.ins-det] 11 Dec 2015")
Energy calibration via correlation Originally published in Nuclear nstruments and Methods in Physics Research Section A, 206 (DO: 0.06/j.nima.205..49) Daniel Maier, Olivier Limousin CEA Saclay, DSM/rfu/Service
hν' Φ e - Gamma spectroscopy - Prelab questions 1. What characteristics distinguish x-rays from gamma rays? Is either more intrinsically dangerous?
Gamma spectroscopy - Prelab questions 1. What characteristics distinguish x-rays from gamma rays? Is either more intrinsically dangerous? 2. Briefly discuss dead time in a detector. What factors are important
The Compton Spectrometer and Imager A balloon- borne gamma- ray spectrometer, polarimeter, and imager
The Compton Spectrometer and Imager A balloon- borne gamma- ray spectrometer, polarimeter, and imager John Tomsick UC Berkeley/Space Sciences Lab for the COSI collaboration The COSI Collaboration: S.E.
CANDELA, a setup to study a stacked detector configuration and the way to ASTRO-H , Daniel Maier, P.160
CANDELA, a setup to study a stacked detector configuration and the way to ASTRO-H 14.04.2015, Daniel Maier, P.160 Overview CANDELA setup Statistics on polarization measurements Perspective: ASTRO-H 2 Daniel
Modular Survey Spectrometer and Compton Imager
1 Modular Survey Spectrometer and Compton Imager Audrey MacLeod Ionizing Radiation Standards Measurement Science and Standards National Research Council Canada On behalf of the SCoTSS collaboration (Silicon
Gamma-Ray Polarimetry in the Pair Production Regime
Gamma-Ray Polarimetry in the Pair Production Regime Peter F. Bloser (NASA/GSFC) S. D. Hunter (NASA/GSFC) G. O. Depaola (National University of Córdoba) F. Longo (INFN) Gamma-Ray Polarimetry Polarimetry
A novel design of the MeV gamma-ray imaging detector with Micro-TPC
Elsevier Science 1 Journal logo A novel design of the MeV gamma-ray imaging detector with Micro-TPC R.Orito *,H.Kubo,K.Miuchi,T.Nagayoshi,A.Takada,T.Tanimori,M.Ueno Department of Physics,Graduate School
Special SLS Symposium on Detectors
Special SLS Symposium on Detectors Tuesday, December 12, 2017 9:30 to 12:15, WBGB/019 09:30 - What are hybrid pixel detectors? - An introduction with focus on single photon counting detectors Erik Fröjdh
Development of semiconductor imaging detectors for a Si/CdTe Compton camera
SLAC-PUB-12926 October 27 Development of semiconductor imaging detectors for a Si/CdTe Compton camera Shin Watanabe a,, Shin ichiro Takeda a,b, Shin-nosuke Ishikawa a,b, Hirokazu Odaka a,b, Masayoshi Ushio
High-Sensitivity Gamma-Ray Imaging With Double Sided Strip Detectors
High-Sensitivity Gamma-Ray Imaging With Double Sided Strip Detectors Thomas Niedermayr, Morgan Burks, Lucian Mihailescu, Karl Nelson, David Lange, John Valentine, Kai Vetter Lawrence Livermore National
New perspectives in X-ray detection of concealed illicit materials brought by CdTe/CdZnTe spectrometric detectors
New perspectives in X-ray detection of concealed illicit materials brought by CdTe/CdZnTe spectrometric detectors Jean-Marc Dinten, Jean-Louis Amans, Loïck Verger, Olivier Peyret CEA-LETI, MINATEC, Recherche
INTEGRAL observations of -ray polarized sources
INTEGRAL observations of -ray polarized sources Philippe Laurent, Christian Gouiffès, Diego Götz, J. Rodriguez Service d Astrophysique, CEA Saclay, France Andy Shearer, Eoin O Connor, Paul Moran Centre
CCD readout of GEM-based neutron detectors
Nuclear Instruments and Methods in Physics Research A 478 (2002) 357 361 CCD readout of GEM-based neutron detectors F.A.F. Fraga a, *, L.M.S. Margato a, S.T.G. Fetal a, M.M.F.R. Fraga a, R. Ferreira Marques
Detector R&D in KAPAC
Detector R&D in KAPAC Hiroyasu Tajima Stanford Linear Accelerator Center Kavli Institute for Particle Astrophysics and Cosmology Outline Compton Camera SOI detector Scintillator Polarimeter Cherenkov Camera
Polaris 3-D CdZnTe (CZT) Gamma-Ray Imaging Spectrometers
Polaris 3-D CdZnTe (CZT) Gamma-Ray Imaging Spectrometers Zhong He ISOE-ALARA Symposium, January 12, 2015 Acknowledgements: DOD, DOE and DHS John M. Palms Outstanding Innovation Began in early 1960s Thank
Detection and measurement of gamma-radiation by gammaspectroscopy
Detection and measurement of gamma-radiation by gammaspectroscopy Gamma-radiation is electromagnetic radiation having speed equal to the light in vacuum. As reaching a matter it interact with the different
Warsaw University of Technology, Faculty of Physics. Laboratory of Nuclear Physics & Technology. Compton effect
Warsaw University of Technology, Faculty of Physics Laboratory of Nuclear Physics & Technology Compton effect Author: MSc. Eng. Dariusz Aksamit, Dariusz.Aksamit@pw.edu.pl, Faculty of Physics on the basis
PoS(Extremesky 2011)067
telescopes, INAF/IASF-Bologna Via Gobetti 101, I-40129 Bologna, Italy E-mail: caroli@iasfbo.inaf.it Rui M. Curado da Silva LIP, Universidade de Coimbra, P-3004-516 Coimbra, Portugal E-mail: ruisilva@saturno.fis.uc.pt
1. Motivation & Detector concept 2. Performance 3. Applications 4. Summary
A. Takada, T. Tanimori, H. Kubo, K. Miuchi, J. D. Parker, T. Mizumoto, Y. Mizumura, T. Sawano, Y. Matsuoka, S. Komura, S. Nakamura, M. Oda, S. Iwaki, K. Nakamura, S. Sonoda, D. Tomono (Kyoto Univ.) 1.
Detecting high energy photons. Interactions of photons with matter Properties of detectors (with examples)
Detecting high energy photons Interactions of photons with matter Properties of detectors (with examples) Interactions of high energy photons with matter Cross section/attenution length/optical depth Photoelectric
Studying microquasars with X-ray polarimetry
Studying microquasars with X-ray polarimetry XIPE extp IXPE Andrea Marinucci From quiescence to ouburst: when microquasars go wild! Ile de Porquerolles 25 September 2017 Outline - Introduction - Polarimetry
E. Caroli(1), R. M. Curado da Silva(2), J.B. Stephen(1), F. Frontera(1,3), A. Pisa (3), S. Del Sordo (4)
E. Caroli(1), R. M. Curado da Silva(2), J.B. Stephen(1), F. Frontera(1,3), A. Pisa (3), S. Del Sordo (4) 1. INAF/IASF-Bologna, Italia 2. Departamento de Fisica, Univerisidade de Combra, Portugal 3. Dipartimento
Gamma Ray Burst Polarimeter POLAR
Gamma Ray Burst Polarimeter POLAR Hualin Xiao, Wojtek Hajdas, R. Marcinkowski, R. Kramert, Ken Egli, P. Socha, P. Zhang Paul Scherrer Institute On behalf of POLAR collobration PSI, Switzerland NCBJ, Poland
Compton suppression spectrometry
Compton suppression spectrometry In gamma ray spectrometry performed with High-purity Germanium detectors (HpGe), the detection of low intensity gamma ray lines is complicated by the presence of Compton
CCD OPERATION. The BBD was an analog delay line, made up of capacitors such that an analog signal was moving along one step at each clock cycle.
CCDS Lesson 4 CCD OPERATION The predecessor of the CCD was a device called the BUCKET BRIGADE DEVICE developed at the Phillips Research Labs The BBD was an analog delay line, made up of capacitors such
Application of EUDET telescope for neutron source calibration at Cadarache (Provence, Fr)
EUDET-JRA1 Meeting, DESY, January 2008 Wojciech.Dulinski@ires.in2p3.fr Application of EUDET telescope for neutron source calibration at Cadarache (Provence, Fr) Wojciech Dulinski on behalf of IPHC Outline
Development of a 3D-Imaging Calorimeter in LaBr 3 for Gamma-Ray Space Astronomy
Development of a 3D-Imaging Calorimeter in LaBr 3 for Gamma-Ray Space Astronomy Aleksandar GOSTOJIĆ CSNSM, Orsay, France 7 th New Developmeants In Photodetection, Tours, France, 2014 Introduction: Gamma-ray
Semiconductor X-Ray Detectors. Tobias Eggert Ketek GmbH
Semiconductor X-Ray Detectors Tobias Eggert Ketek GmbH Semiconductor X-Ray Detectors Part A Principles of Semiconductor Detectors 1. Basic Principles 2. Typical Applications 3. Planar Technology 4. Read-out
GAMMA RAY SPECTROSCOPY
GAMMA RAY SPECTROSCOPY Gamma Ray Spectroscopy 1 In this experiment you will use a sodium iodide (NaI) detector along with a multichannel analyzer (MCA) to measure gamma ray energies from energy level transitions
Development of Next Generation Compton Gamma-ray Telescope Hiroyasu Tajima Stanford Linear Accelerator Center
Development of Next Generation Compton Gamma-ray Telescope Hiroyasu Tajima Stanford Linear Accelerator Center May 3, 2004 UC Santa Cruz Collaboration H. Tajima, T. Kamae, G. Madejski, E. do Couto e Silva
Internal conversion electrons and SN light curves
Internal conversion electrons and SN light curves International School of Nuclear Physics 32nd Course: Particle and Nuclear Astrophysics September 23, 2010, Erice Ivo Rolf Seitenzahl DFG Emmy Noether Research
Characterizing New Multi-Channel Peak Sensing ADC-Mesytec MADC-32
Armenian Journal of Physics, 2016, vol. 9, issue 1, pp. 29-33 Characterizing New Multi-Channel Peak Sensing ADC-Mesytec MADC-32 A. Gyurjinyan 1,2, R. Avetisyan 1,2 1 Experimental Physics Division, Yerevan
Measurement of material uniformity using 3-D position sensitive CdZnTe gamma-ray spectrometers
Nuclear Instruments and Methods in Physics Research A 441 (2000) 459}467 Measurement of material uniformity using 3-D position sensitive CdZnTe gamma-ray spectrometers Z. He *, W.Li, G.F. Knoll, D.K. Wehe,
Radiation Detection for the Beta- Delayed Alpha and Gamma Decay of 20 Na. Ellen Simmons
Radiation Detection for the Beta- Delayed Alpha and Gamma Decay of 20 Na Ellen Simmons 1 Contents Introduction Review of the Types of Radiation Charged Particle Radiation Detection Review of Semiconductor
Laura Barragán. Universidad Complutense de Madrid
. Universidad Complutense de Madrid Tutors: Erik Kuulkers & Peter Kretschmar INTEGRAL: International Gamma-Ray Astrophysics Laboratory The payload The mission The project IBIS (Imager on-board the Integral
arxiv:nucl-ex/ v2 21 Jul 2005
Gamma-spectrometric uranium age-dating using intrinsic efficiency calibration arxiv:nucl-ex/0506029v2 21 Jul 2005 Cong Tam Nguyen and József Zsigrai Institute of Isotopes of the Hungarian Academy of Sciences
Digital simulation of neutron and gamma measurement devices
3Security of radioactive materials and transport 3 2 Digital simulation of neutron and gamma measurement devices A.-L. WEBER (IRSN) 1 - Maximum activity that a radioactive element can present without being
CZT Gamma Spectrometry Applied to the In-situ Characterisation of Radioactive Contaminations
CZT Gamma Spectrometry Applied to the In-situ Characterisation of Radioactive Contaminations Alain Rocher (EDF/DPN; e-mail : alain.rocher@edf.fr) Leon Piotrowski (EDF/R&D; e-mail : leon.piotrowski@edf.fr)
Efficiency and Attenuation in CdTe Detectors
Efficiency and Attenuation in CdTe Detectors Amptek Inc. Bob Redus, May 5, 00 Amptek s XR-00T-CdTe is a high performance x-ray and gamma ray detector system. Like Amptek s other XR00 products, a detector
arxiv:astro-ph/ v1 26 Sep 2003
Applications of Gas Imaging Micro-Well Detectors to an Advanced Compton Telescope arxiv:astro-ph/0309731v1 26 Sep 2003 P. F. Bloser a,, S. D. Hunter a, J. M. Ryan b, M. L. McConnell b, R. S. Miller b,,
ASTRO-H ASTRO-H and future missions in JAXA program. Tadayuki Takahashi PI/Project Manager on behalf of the ASTRO-H team
ASTRO-H ASTRO-H and future missions in JAXA program Tadayuki Takahashi PI/Project Manager on behalf of the ASTRO-H team 1 Status The ASTRO-H Project is in Phase B, since 2008 Oct. (JAXA) 2009/Jan-Feb :
Interaction of particles with matter - 2. Silvia Masciocchi, GSI and University of Heidelberg SS2017, Heidelberg May 3, 2017
Interaction of particles with matter - 2 Silvia Masciocchi, GSI and University of Heidelberg SS2017, Heidelberg May 3, 2017 Energy loss by ionization (by heavy particles) Interaction of electrons with
Detector R&D at KIPAC
Detector R&D at KIPAC Hiro Tajima Kavli Institute for Particle Astrophysics and Cosmology 1 Detector R&D Overview Si detector ASIC Integration GLAST GeV Gamma-ray Observatory ASIC DAQ Next generation X-ray
A Study On Radioactive Source Imaging By Using A Pixelated CdTe Radiation Detector
ISSN: 1791-4469 Copyright 2012 Hellenic Naval Academy A Study On Radioactive Source Imaging By Using A Pixelated CdTe Radiation Detector K. Zachariadou a,c, K. Karafasoulis b,c, S. Seferlis c, I. Papadakis
Emission Model And GRB Simulations
Emission Model And GRB Simulations Nicola Omodei (University of Siena, INFN Pisa) 1 ISSS-L Aquila 2001 N. Omodei Spectral Properties? Data collected Range (γ) 10 KeV 10 GeV In the BATSE energy range: (25
NGN PhD Studentship Proposal
NGN PhD Studentship Proposal Note that proposals will be assessed against both the quality of the scientific content and of the proposed training experience. Proposed supervisors (lead first) Dr Laura
High Yield Structured X-ray Photo-Cathode Development and Fabrication
High Yield Structured X-ray Photo-Cathode Development and Fabrication K. Opachich 1, P. Ross 1, J. Koch 1, A. MacPhee 2, O. Landen 2, D. Bradley 2, P. Bell 2, S. Nagel 2, T. Hilsabeck 4, N. Chen 5, S.
The MEGA Advanced Compton Telescope Project
The MEGA Advanced Compton Telescope Project P. F. Bloser a, R. Andritschke a, G. Kanbach a, V. Schönfelder a, F. Schopper a, A. Zoglauer a, for the MEGA Collaboration a,b arxiv:astro-ph/0110129v1 5 Oct
A very wide field focusing telescope for Synoptic studies in the soft X-ray band
A very wide field focusing telescope for Synoptic studies in the soft X-ray band Paul Gorenstein Harvard-Smithsonian Center for Astrophysics Cambridge, MA 02138 Synoptic Telescopes, (Broad Coverage of
Radioactivity. Lecture 6 Detectors and Instrumentation
Radioactivity Lecture 6 Detectors and Instrumentation The human organs Neither humans nor animals have an organ for detecting radiation from radioactive decay! We can not hear it, smell it, feel it or
AGATA preamplifier performance on large signals from a 241 Am+Be source. F. Zocca, A. Pullia, D. Bazzacco, G. Pascovici
AGATA preamplifier performance on large signals from a 241 Am+Be source F. Zocca, A. Pullia, D. Bazzacco, G. Pascovici AGATA Week - LNL (PD), Italy, 12-15 November 2007 Outline Recalls : Fast reset device
The ASIM experiment on the ISS. Torsten Neubert and the ASIM Team
The ASIM experiment on the ISS Torsten Neubert and the ASIM Team Content The Science The ASIM Payload The Science Instruments Status and Consortium 2 DTU Space, Technical University of Denmark The occurrence
A CdTe detector with a Gd converter for thermal neutron detection
A CdTe detector with a Gd converter for thermal neutron detection Aki Miyake, Takahiro Nishika, Shailendra Singh, Hisashi Morii, Hidenori Minura, Toru Aoki. Nuclear Instruments and Methods in Physics Research
Pulse Height Analysis System (PHA) designed for W7-X Presented by Monika KUBKOWSKA
Pulse Height Analysis System (PHA) designed for W7-X Presented by Monika KUBKOWSKA This scientific work has been partly supported by Polish Ministry of Science and Higher Education within the framework
Detectors for 20 kev 10 MeV
Gamma-Ray Bursts Detectors for 20 kev to 10 MeV Discovery The early years BATSE Fast versus slow bursts Uniformity and log N log S relation BeppoSAX and discovery of afterglows Redshift measurements Connection
Characterization of low energy ionization signals from Compton scattering in a CCD Dark Matter detector
Characterization of low energy ionization signals from Compton scattering in a CCD Dark Matter detector Karthik Ramanathan University of Chicago arxiv:1706.06053 (Accepted PRD) TeVPA 2017/08/07 1 Motivation
Development of a Dedicated Hard X-Ray Polarimeter Mark L. McConnell, James R. Ledoux, John R. Macri, and James M. Ryan
Development of a Dedicated Hard X-Ray Polarimeter Mark L. McConnell, James R. Ledoux, John R. Macri, and James M. Ryan Space Science Center University of New Hampshire Durham, NH AAS-HEAD Mt. Tremblant,
Digital Gamma-ray Spectroscopy & Imaging with Semiconductor detectors Frontiers of gamma-ray spectroscopy
Digital Gamma-ray Spectroscopy & Imaging with Semiconductor detectors Frontiers of gamma-ray spectroscopy AGATA GRETA Dr Andy Boston ajboston@liv.ac.uk And its applications The AGATA Concept Without Compton
Studying microquasars with X-ray polarimetry
Studying microquasars with X-ray polarimetry extp Andrea Marinucci IXPE Congresso Nazionale Oggetti Compatti X Padova 14 September 2017 Outline - Introduction - Polarimetry and microquasars: Coronal geometry
GRB Polarimetry with POLAR. Merlin Kole
GRB Polarimetry with POLAR Merlin Kole Alsatian X-ray Workshop, November 13th, 2017 POLAR on the TG-2 2011: TG-1 Space Lab launched TG-2 Chinese Space Lab launched in September 2016 POLAR launched with
Motivation Electron-Tracking Compton Telescope 1 st Flight of SMILE Preparation for next step summary
A. Takada (ISAS/JAXA), T. Tanimori, H. Kubo, K. Miuchi, S. Kabuki, Y. Kishimoto, J. Parker, H. Nishimura, K. Hattori, K. Ueno, S. Kurosawa, S. Iwaki, C. Ida, M. Takahashi, T. Sawano, K. Taniue, K. Nakamura,
Development of a modular CdTe detector plane for gamma-ray burst detection below 100 kev
Development of a modular CdTe detector plane for gamma-ray burst detection below 100 kev M. Ehanno a, C. Amoros a, D. Barret a, K. Lacombe a, R. Pons a, G. Rouaix a, O. Gevin b, O. Limousin b, F. Lugiez
The CSPD-1 y-ray Vision System
1554 IEEE TRANSACTIONS ON NUCLEAR SCIENCE, VOL. 43, NO. 3, JUNE 1996 The CSPD-1 y-ray Vision System Z. He, J. Obermarkf, J. Du, D.K. Wehe, S.W. Leet, G.F. Knoll Nuclear Engineering Department, +Electrical
Energy resolution and absolute detection efficiency for LSO crystals: a comparison between Monte Carlo simulation and experimental data
Energy resolution and absolute detection efficiency for LSO crystals: a comparison between Monte Carlo simulation and experimental data Harold Rothfuss a,b, Larry Byars c, Michael E. Casey a, Maurizio
Particle nature of light & Quantization
Particle nature of light & Quantization A quantity is quantized if its possible values are limited to a discrete set. An example from classical physics is the allowed frequencies of standing waves on a
Recent Advances on CdTe/CdZnTe detectors
Recent Advances on CdTe/CdZnTe detectors For High Energy PHOTON Tad Takahashi Institute of Space and Astronautical Science (ISAS) Japan Aerospace exploration Agency (JAXA) and Univ. of Tokyo Acknowledgement
Detectors for High Resolution Gamma-ray Imaging Based on a Single CsI(Tl) Scintillator Coupled to an Array of Silicon Drift Detectors
1 Detectors for High Resolution Gamma-ray Imaging Based on a Single CsI(Tl) Scintillator Coupled to an Array of Silicon Drift Detectors C. Fiorini, A. Longoni, F. Perotti, C. Labanti, E. Rossi, P. Lechner,
Astrophysics with GLAST: dark matter, black holes and other astronomical exotica
Astrophysics with GLAST: dark matter, black holes and other astronomical exotica Greg Madejski Stanford Linear Accelerator Center and Kavli Institute for Particle Astrophysics and Cosmology (KIPAC) Outline:
estec NIRSpec Technical Note NTN Spectral intensity of the MSA glow sources Abstract:
NIRSpec Technical Note NTN-2013-014 Authors: P. Ferruit & G. Giardino Date of Issue: 29.11.2013 Version: 1 estec European Space Research and Technology Centre Keplerlaan 1 2201 AZ Noordwijk The Netherlands
Sample Spectroscopy System Hardware
Semiconductor Detectors vs. Scintillator+PMT Detectors Semiconductors are emerging technology - Scint.PMT systems relatively unchanged in 50 years. NaI(Tl) excellent for single-photon, new scintillation
Drift plane. substrate (20ÉIm polyimide) 200ÉIm. Back strip (180ÉIm width) Base (Ceramic) Anode strip (10ÉIm width) Cathode strip (100ÉIm width)
Proceedings of the Second International Workshop on EGS, 8.-1. August, Tsukuba, Japan KEK Proceedings -, pp.11-17 Development of Gamma-Ray Direction Detector Based on MSGC T. Nagayoshi 1, H. Kubo 1, A.
Mass Determination of Rn and Hg isotopes using MASHA
Mass Determination of Rn and Hg isotopes using MASHA Alfred M. Sehone Lumkile Msebi Oleg Lishyk Stanislav Stanishevski Yuliya Brechko Supervisor Krupa Lubosh Flerov Laboratory of Nuclear reactions, JINR,
Student Projects for
MINERALS RESOURCES Student Projects for 2016-17 The CSIRO On-line Analysis (OLA) Group offers opportunities for students to undertake applied physics research projects at our Lucas Heights laboratories.
DOUBLE BETA DECAY OF 106 Cd - EXPERIMENT TGV (Telescope Germanium Vertical) EXPERIMENT SPT (Silicon Pixel Telescope)
DOUBLE BETA DECAY OF 106 Cd - EXPERIMENT TGV (Telescope Germanium Vertical) EXPERIMENT SPT (Silicon Pixel Telescope) I. Štekl (IEAP CTU in Prague) on behalf of TGV collaboration CSNSM Orsay, France CU
Peter Fischer, ziti, Universität Heidelberg. Silicon Detectors & Readout Electronics
Silicon Detectors and Readout Electronics Peter Fischer, ziti, Universität Heidelberg 1 Content of the Lecture (sorted by subject) Introduction: Applications of silicon detectors Requirements, measured
Detection of X-Rays. Solid state detectors Proportional counters Microcalorimeters Detector characteristics
Detection of X-Rays Solid state detectors Proportional counters Microcalorimeters Detector characteristics Solid State X-ray Detectors X-ray interacts in material to produce photoelectrons which are collected
Final report on DOE project number DE-FG07-99ID High Pressure Xenon Gamma-Ray Spectrometers for Field Use
Final report on DOE project number DE-FG07-99ID13772 High Pressure Xenon Gamma-Ray Spectrometers for Field Use Principle Investigator: Glenn K. Knoll Co-investigator: David K. Wehe, Zhong He, University
Intrinsic beam emittance of laser-accelerated electrons measured by x-ray spectroscopic imaging
Intrinsic beam emittance of laser-accelerated electrons measured by x-ray spectroscopic imaging G. Golovin 1, S. Banerjee 1, C. Liu 1, S. Chen 1, J. Zhang 1, B. Zhao 1, P. Zhang 1, M. Veale 2, M. Wilson
Stand-off Nuclear Radiation Detection
Stand-off Nuclear Radiation Detection Peter E. Vanier Detector Development and Testing Div. Nonproliferation and National Security Dept. Brookhaven National Laboratory Brookhaven Science Associates U.S.