detector development Matthias Beilicke X ray Science Analysis Group meeting (12 April 2013, Monterey, CA) Collaborators: GSFC, BNL
|
|
|
- Benjamin Richard
- 5 years ago
- Views:
Transcription
1 X-ray X-ray detector detector development development at at Washington Washington University University in in St.Louis St.Louis Matthias Beilicke Washington University in St.Louis, Physics Department & McDonnell Center for the Space Sciences Collaborators: GSFC, BNL X ray Science Analysis Group meeting (12 April 2013, Monterey, CA)
2 X-ray (semiconductor) detectors: Overview Cadmium Zinc Telluride (CZT): X ray mirror technology: Major improvements in fabrication/cost/accuracy Zhang, et al.,proc. of SPIE 8147 (2011) 81470K 7 Focusing (compared to coded mask): larger effective area, better imaging, higher S/N X-ray mirror image: Chandra/NASA Medical & homeland security Astrophysics (Swift: 32,768, INTEGRAL: 16,384) + present and future missions Burrows et al., Mem.S.A.It., 75, 1 Application of CZT: Coded mask Z ~50, = 5.78 g/cm3, X ray photons: photo effect & Compton scattering Operation at room temperature (band gap: ~1.6eV) Limits in energy resolution: charge fraction => phonons Alternatives: Measure T of absorber
3 CZT on board the NuSTAR satellite NuSTAR mission (SMEX): Harrison et al., arxiv (2013) Kitaguchi et al., SPIE, 8145, (2011) Wolter X ray mirror (large effective area) launched in 2012 Focal plane instrument: 2x2x0.2 cm3 CZT detectors (32x32 pixels, 605 m pitch) Energy resolution: 0.5keV@14keV, 0.9keV@122keV Readout: Caltech NuCIT ASIC (0.4keV readout noise) e /h readout > determine depth of interaction X-ray mirror Harrison et al., arxiv (2013)
4 Coded mask and 3D imaging applications ProtoEXIST flight: 3D position sensitive detectors: Hong et al., NIMA, 654, 361 (2011) Coded mask instrument (balloon) Z.He, et al, IEEE, 54, 843 (20107) expertise in thick CZT detectors/readout 3D position sensitive: depth of interaction (<1% energy 662keV) High energy Compton imaging Instrument: 8x8 detectors (64 pixels each, p=2.5mm) RadNET ASIC (power: ~150 W/pixel) X-ray mirror
5 CZT X-ray detectors: fabrication & Washington Univ. Clean room (class-100): Photo lithography masks & E beam evaporation Readout electronics: BNL & Washington University Detector characterization: Energy resolution & threshold, effect of steering grid Comparison to simulations (charge sharing/transport) - Energy resolution: 662keV - threshold: down to ~15 kev
6 Variable size pixels (2mm detector) 122 kev Rapid prototyping: 40 kev (1) quick configuration scan on one detector (2) reduces uncertainties of re fabrication Findings: Big pixels: better energy resolution & rate Steering grid improves energy resolution Steering grid improves rates (esp. HE) steering grid No steering grid
7 Variable pitch pixels (5 mm detector) N=2 N=1 Increasing StGrid voltage N=2 rate resolution N=2
8 Small (sub-mm) pixels Fabricate/test: pixel pitches 350, 600, & 700 um Direct bonding to ASIC broad Collaboration with L.J. Meng (UIUC): AJAT ASIC readout Collaboration with G. Jernigan (Berkeley) & Black Forest: testing 600 um pixel detectors Readout board for 2048-channel AJAT ASIC.
9 Future goal: 150 um pixel detectors Zhang, et al.,proc. of SPIE 8147 (2011) 81470K-7 Motivation: - New X-ray mirrors: improved point spread function Project goals: - Detectors with 150 um pixel pitch (5-10 arc sec) - Low energy threshold (<5keV) - Optimized readout electronics: BNL Astrophysical applications: blue shifted red shifted - Black hole vicinity (Fe K band absorption lines) - Supernova remnants: element emission (C to Ni), relative line power: mechanisms of explosion - Velocity distribution of rotating gas Tycho SNR: iron K-shell emission See also differential deposition: Weisskopf et al.
10 2-D ASIC Development for Li & DeGeronimo Hi-Resolution X-ray Imager at BNL Si sensors (16 by 16 arrays) Bump-bonding Si detector to small-pixel ASIC Preliminary ASIC layout overlapping the silicon sensor: 16 by 16 array, 250-µm pitch, 0.6mW/pixel, ENC<10 electrons 6.5 mm mm5. 5 2/3-stage pre-amp 3rd-order DFF shaper bump pad baseline holder discriminator & peak detector
11 X-ray polarization: motivation & status X-ray astronomy: - Spectral/morphology studies well established (non-thermal astrophysical sources) - Spectro-polarimetric observations: access fraction & angle of polarization Processes resulting in polarized radiation: Synchrotron radiation (linear, ^ to B), curvature radiation (circular), Thomson scattering (perpendicular to scattering plane) X-ray polarimetry: Mission Status - OSO-8: Crab: 2.6/5.2 kev polarization (20%, 30o relative to jet) [ApJ, 220, L117, 1978] - INTEGRAL: Crab polarization (0.1-1MeV): ~46% [Science, 321, 1183, 2008] Astrophysics (extract): - Accreting black holes (BHs): testing accretion disk & BH mass/spin - Pulsars/PWN: constrain magnetic field & particle populations - Active galactic nuclei: testing magnetic jet structure X-ray polarimetry: Possible/future missions: - Gravity and Extreme Magnetism SMEX (GEMS): 2-10 kev (100 x OSO-8) [Swank] - Astro-H: E>10 kev, Compton Polarimetry (systematics) [SPIE, 7732, 34, 2010]
12 X-Calibur design (PI: H.Krawczynski) measure polarization of 20-80keV X-rays 1: Compton scattering in low-z scintillator: more likely to E field vector of photon EJ-200, ~1g/cm3, read by Hamamatsu R7600U PMT 2: photo-absorption in high-z CZT 8x8 pixels each, read by BNL ASIC (DeGeronimo & Wulf) 3: signature in azimuthal scattering distribution CZT CZT HV readout Rotation: reduce systematics
13 X-Calibur: Polarized CHESS Cornell high-energy synchrotron sources (CHESS) 4 Azimuth scatter distribution 3 Compton spectrum CZT detectors Pola rize d 2 scintillator X-ra y bea m 1 CHESS beam
14 X-Calibur: Polarized CHESS Cornell high-energy synchrotron sources (CHESS) 4 Azimuth scatter distribution 3 Compton spectrum CZT detectors Pola rize d 2 scintillator X-ra y Agreement with expectations bea m 1 CHESS beam
15 X-Calibur flight: InFOCuS X-ray telescope 8m focal length, 1.4t, grazing incidence Wolter X-ray mirror X-Calibur/InFOCuS: 1: High detection efficiency (80%) 2: low background (low volume) 3: control/reduction of systematics Flight: 2013 (1day, New Mexico) Crab, Her X-1, Cyg X-1, GRS 1915, Mrk 421, EXO 0331 Rotation: Reduction of systematic effects X-Calibur InFOCuS (NASA, GSFC)
16 Summary & Conclusion Cadmium-Zinc-Telluride: Crab Material of choice for hard X ray detectors Future CZT detector/asic development: Smaller pixels (~200 um pitch) Low threshold (<5 kev) ASIC Hard X-ray polarimeter X-Calibur: Detector fully assembled, calibrated & tested at CHESS 2013-day X-Calibur/InFOCuS balloon flight (Crab, Her X-1, Cyg X-1, GRS 1915, EXO 0331, Mrk 421) Applied for long duration flight (goal: 2keV threshold) Acknowledgements: NASA grants: NNX10AJ56G & NNX12AD51G, discretionary funding from the McDonnell Center for the Space Sciences. CHESS: This work is based upon research conducted at the Cornell High Energy Synchrotron Source (CHESS) which is supported by the National Science Foundation and the National Institutes of Health/National Institute of General Medical Sciences under NSF award DMR X-Calibur
Non-thermal emission from pulsars experimental status and prospects
Non-thermal emission from pulsars experimental status and prospects # γ!"# $%&'() TeV γ-ray astrophysics with VERITAS ( $γ" *$%&'() The charged cosmic radiation - how it all began... Discovery: Victor
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
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
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 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
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
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
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
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,
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, H. Nishimura, K. Hattori, K. Ueno, S. Kurosawa, C. Ida, S. Iwaki, M. Takahashi (Kyoto Univ.) Motivation Electron-Tracking Compton Telescope
High Energy Polarimetry Missons in Japan; PoGOLite, SPHiNX, PolariS
High Energy Polarimetry Missons in Japan; PoGOLite, SPHiNX, PolariS Hiromitsu Takahashi (Hiroshima University) hirotaka@hep01.hepl.hiroshima-u.ac.jp PoGOLite balloon 10m (2013~) SPHiNX satellite 0.5m (Plan:
PoGOLite, PoGO+, SPHiNX High-Energy Polarimetry Missions between Japan and Sweden
PoGOLite, PoGO+, SPHiNX High-Energy Polarimetry Missions between Japan and Sweden Hiromitsu Takahashi (Hiroshima University) hirotaka@astro.hiroshima-u.ac.jp PoGOLite balloon 10m (2013) PoGO+ balloon 10m
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,
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,
Polarimeter for Small Satellite Design, Feasibility Study, and Ground Experiments + Balloon Experiment
Hard X-ray X Polarimeter for Small Satellite Design, Feasibility Study, and Ground Experiments + Balloon Experiment K. Hayashida (Osaka University), T. Mihara (RIKEN), S. Gunji,, F. Tokanai(Yamagata University)
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
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,
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 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
Xenon Compton Telescopes at Columbia: the post LXeGRIT phase. E.Aprile. Columbia University
Xenon Compton Telescopes at Columbia: the post LXeGRIT phase E.Aprile Columbia University Seeon 2003 Sensitivity Goals for An Advanced Compton Telescope ~10-7 ph cm -2 s -1 ( 3σ) for narrow lines and ~
X- ray Polarimetry Satellite GEMS and beyond
ithes Mini-workshop on "Strong-Field Physics X- ray Polarimetry Satellite GEMS and beyond RIKEN Nishina Center Toru Tamagawa Strong- field Physics(May. 29, 2014) 2 Introduc8on X-ray polarimetry is the
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,
Space Application of Geant4 for the Japanese X-ray X Gamma-ray Mission
Space Application of Geant4 for the Japanese X-ray X and Gamma-ray Mission Yukikatsu Terada (RIKEN, Japan), Shin Watanabe, Masanobu Ozaki, Tadayuki Takahashi (ISAS/JAXA), and Motohide Kokubun (Univ. of
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
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
Study of the HARPO TPC for a high angular resolution g-ray polarimeter in the MeV-GeV energy range. David Attié (CEA/Irfu)
Study of the HARPO TPC for a high angular resolution g-ray polarimeter in the MeV-GeV energy range David Attié (CEA/Irfu) Outline Motivation of an MeV-GeV polarimeter Scientific case and expected performance
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.
Optimization of the Design of the Hard X-ray Polarimeter X-Calibur
Optimization of the Design of the Hard X-ray Polarimeter X-Calibur Qingzhen Guo 1, 2*, Matthias Beilicke 1, Alfred Garson 1, Fabian Kislat 1, David Fleming 3, Henric Krawczynski 1 1 Washington University
Special Topics in Nuclear and Particle Physics
Special Topics in Nuclear and Particle Physics Astroparticle Physics Lecture 5 Gamma Rays & x-rays Sept. 22, 2015 Sun Kee Kim Seoul National University Gamma ray astronomy gamma ray synchrotron radition
Marshall Space Flight Center XPE
XPE P.I. Martin Weisskopf / MSFC Co.Is. NASA/MSFC Penn State University University of Costa Rica Collaborators SAO Columbia University Stanford University Max Planck Institute University College London
Detector and Telescope Development for ProtoEXIST and Fine Beam Measurements of Spectral Response of CZT Detectors
Detector and Telescope Development for ProtoEXIST and Fine Beam Measurements of Spectral Response of CZT Detectors J. Hong a*, A. Copete a, J. E. Grindlay a, S. V. Vadawale a, W. W. Craig b, F. Harrison
Imaging Hard X-Ray Compton Polarimeter SOI Sensor Prototype Specification
Imaging Hard X-Ray Compton Polarimeter SOI Sensor Prototype Specification Hiro Tajima 1 and Gary S. Varner 2 1 Contact: htajima@slac.stanford.edu Stanford Linear Accelerator Center Stanford University,
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.
Astrosat First Light: CZT Imager Looks at Crab
Astrosat First Light: CZT Imager Looks at Crab Astrosat - fondly named 'India's own space observatory' was put into orbit on September 28, 2015. Then began the process of putting each of the payloads into
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
Balloon-Borne Gamma-Ray Polarimeter (PoGO) to study Black Holes, Pulsars, and AGN. Jets: Design and Calibration. Zachary Apte
SLAC-TN-05-058 Balloon-Borne Gamma-Ray Polarimeter (PoGO) to study Black Holes, Pulsars, and AGN Jets: Design and Calibration Zachary Apte Office of Science, SULI Program Hampshire College Stanford Linear
A. Takada (Kyoto Univ.)
A. Takada (Kyoto Univ.) Nucleosynthesis SNR : Radio-isotopes Galactic plane : 26 Al Annihilation Particle acceleration Jet (AGN) : Synchrotron + Inverse Compton Strong gravitational potential Black hole
Observation of Crab Nebula by Nuclear Compton Telescope (NCT)
Observation of Crab Nebula by Nuclear Compton Telescope (NCT) 32 nd ICRC, Aug.15, 2011 at Beijing, China Ming-Huey A. Huang for NCT Collaboration National United University & LeCosPA, NTU NCT Collaboration:
Studying microquasars with X-ray polarimetry. Giorgio Matt (Università Roma Tre, Italy)
Studying microquasars with X-ray polarimetry Giorgio Matt (Università Roma Tre, Italy) Accreting black hole systems Fender &Belloni 12 Done et al. 07 Accreting black hole systems The role of the jet The
Future prospects for solar flare (but not only) X-ray polarimetric missions
Future prospects for solar flare (but not only) X-ray polarimetric missions Sergio Fabiani INFN Trieste On the behalf of the High Energy Astrophysics and Related Technology Group at the INAF IAPS (Rome)
Multilayer coating facility for the HEFT hard X-ray telescope
Multilayer coating facility for the HEFT hard X-ray telescope Carsten P. Jensen a, Finn E. Christensen a, Hubert Chen b, Erik B. W.Smitt a, Eric Ziegler c a Danish Space Research Institute (Denmark); b
1. Motivation & Detector concept 2. Performance 3. Confirmation experiments 4. Summary
A. Takada, T. Tanimori, H. Kubo, J. D. Parker, T. Mizumoto, Y. Mizumura, T. Sawano, K. Nakamura, Y. Matsuoka, S. Komura, S. Nakamura, T. Kishimoto, M. Oda, T. Takemura, S. Miyamoto, K. Miuchi, S. Kurosawa
PROJECT STATUS AND PERSPECTIVES
COBRA CdZnTe 0-NEUTRINO BETA-BETA RESEARCH APPARATUS PROJECT STATUS AND PERSPECTIVES DATE JULY 28, 2011 BY JERRAD MARTIN Agenda Introduction to COBRA Past Results Status of Current R&D PROJECT STATUS AND
Status and Future Prospects for Υ-Ray Polarimetry
Status and Future Prospects for Υ-Ray Polarimetry Mark McConnell Space Science Center University of New Hampshire Durham, NH X-Ray Polarimetry Workshop SLAC / Stanford 9-11 February 2004 Overview Recent
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
Cosmic Rays and the need for heavy payloads
Cosmic Rays and the need for heavy payloads T. Gregory Guzik Department of Physics and Astronomy Louisiana State University Baton Rouge, LA LSU 04/19/07 LCANS 2007 - April 27, 2007 1 Ballooning leads the
X-Ray Polarimetry. From the early days to an outlook for the future. Martin C. Weisskopf (NASA/MSFC)
X-Ray Polarimetry From the early days to an outlook for the future Martin C. Weisskopf (NASA/MSFC) Monday August 25, 2014 Outline A look to the past & tribute to Bob Novick The present --- electron tracking
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
Precise Low-Energy Electron Tracking Using a Gaseous Time Projection Chamber for the Balloon-Borne Gamma Ray Compton Telescope
Precise Low-Energy Electron Tracking Using a Gaseous Time Projection Chamber for the Balloon-Borne Gamma Ray Compton Telescope T. Mizumoto, T. Tanimori, H. Kubo, A. Takada, J. D. Parker, S. Sonoda, Y.
Chapter 0 Introduction X-RAY BINARIES
X-RAY BINARIES 1 Structure of this course 0. Introduction 1. Compact stars: formation and observational appearance. Mass transfer in binaries 3. Observational properties of XRBs 4. Formation and evolution
Observation of Gamma-Rays from Relativistic Electron Precipitation with Balloon Experiment around the Polar regions
Observation of Gamma-Rays from Relativistic Electron Precipitation with Balloon Experiment around the Polar regions Yoshitaka Mizumura (Kyoto Univ.) T. Tanimori, H. Kubo, A. Takada, J. D. Parker, T. Mizumoto,
SLS Symposium on X-Ray Instrumentation
SLS Symposium on X-Ray Instrumentation Tuesday, December 7, 2010 10:00 to 12:15, WBGB/019 10:00 The optics layout of the PEARL beamline P. Oberta, U. Flechsig and M. Muntwiler 10:30 Instrumentation for
MoBiKID Kinetic Inductance Detectors for up-coming B-mode satellite experiments
MoBiKID Kinetic Inductance Detectors for up-coming B-mode satellite experiments TIPP 17 - BEIJING INFN, Sezione di Roma Dawn of the universe: where are we? Looking into the CMB for a proof of the Inflation...
1 Gamma-Ray Burst Polarimeter GAP aboard
1 Gamma-Ray Burst Polarimeter GAP aboard the Solar Powered Sail Mission Daisuke Yonetoku, Toshio Murakami, Hirofumi Fujimoto, Tomonori Sakashita (Kanazawa University) Shuichi Gunji, Noriyuki Toukairin
NuSTAR s Extreme Universe. Prof. Lynn Cominsky NASA Education and Public Outreach Sonoma State University
NuSTAR s Extreme Universe Prof. Lynn Cominsky NASA Education and Public Outreach Sonoma State University The NASA Education and Public Outreach Program at SSU We are a group of scientists and educators
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
CRaTER Pre-Ship Review (PSR) Instrument Calibration Science Requirements Compliance
CRaTER Pre-Ship Review (PSR) Instrument Calibration Science Requirements Compliance Justin C Kasper Smithsonian Astrophysical Observatory January 3, 2008 Outline Calibration Relate the ADU of the Pulse
The Silicon-Tungsten Tracker of the DAMPE Mission
The Silicon-Tungsten Tracker of the DAMPE Mission Philipp Azzarello, DPNC, University of Geneva for the DAMPE-STK collaboration 10th International Hiroshima Symposium on the Development and Application
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
Tests of the BURLE 64-anode MCP PMT as the detector of Cherenkov photons
Tests of the BURLE 64-anode MCP PMT as the detector of Cherenkov photons Peter Križan University of Ljubljana and J. Stefan Institute Contents Motivation and requirements BURLE MCP-PMT Beam test results
Large-Area Balloon-Borne Polarized Gamma Ray Observer (PoGO)
Large-Area Balloon-Borne Polarized Gamma Ray Observer (PoGO) Tune Kamae and John Mitchell for the PoGO collaboration (SLAC-Goddard-Princeton-Japan-Sweden-France) 1. Introduction 2. Compton Scattering 3.
First Results of POLAR: A dedicated Gamma-Ray Burst Polarimeter
First Results of POLAR: A dedicated Gamma-Ray Burst Polarimeter DPNC, University of Geneva E-mail: merlin.kole@unige.ch This year marks the 50th anniversary of the first detection of a Gamma-Ray Burst.
Spotting the misaligned outflows in NGC 1068 using X ray polarimetry
Spotting the misaligned outflows in NGC 1068 using X ray polarimetry René W. Goosmann Observatoire astronomique de Strasbourg, France in collaboration with Giorgio Matt, Frédéric Marin, and Martin Gaskell
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
1. MeV gamma ray Imaging & ETCC 2. Results of SMILE-I 3. Preparations of SMILE-II
A. Takada, T. Tanimori, H. Kubo, K. Miuchi, S. Kabuki, J. D. Parker, Y. Kishimoto, T. Mizumoto, K. Ueno, S. Kurosawa, S. Iwaki, T. Sawano, K. Taniue, K. Nakamura, N. Higashi, Y. Matsuoka, S. Komura, Y.
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
Presentation by Indian Delegation. to 49 th STSC UNCOPUOS. February 2012 Vienna
Presentation by Indian Delegation to 49 th STSC UNCOPUOS February 2012 Vienna ASTROSAT Astrosat is India s first dedicated multiwavelength astronomy satellite with a capability to observe target sources
VERITAS Design. Vladimir Vassiliev Whipple Observatory Harvard-Smithsonian CfA
VERITAS Design Vladimir Vassiliev Whipple Observatory Harvard-Smithsonian CfA VERITAS design goals VERITAS is a ground-based observatory for gamma-ray astronomy VERITAS design is derived from scientific
for the HARPO Collaboration: *
Polarimetry and high-angular-resolution gamma-ray observations in the MeV regime using a novel detector concept for the HARPO Collaboration: * * Author list from recent publication: https://arxiv.org/abs/1706.06483
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
CASTER A Scintillator-Based Black Hole Finder Probe
CASTER A Scintillator-Based Black Hole Finder Probe Mark McConnell University of New Hamsphire The CASTER Cast Mark McConnell, Jim Ryan, John Macri University of New Hampshire Mike Cherry, T. Greg Guzik,
Large-Area Balloon-Borne Polarized Gamma Ray Observer (PoGO)
Large-Area Balloon-Borne Polarized Gamma Ray Observer (PoGO) DOE Review (June 3, 2004) Tune Kamae for the PoGO collaboration (SLAC-Goddard-Princeton-Japan-Sweden-France) 1. Introduction 2. of PoGO 3. Beam
Suzaku-WAM soft gamma-ray all-sky monitor by the earth occultation technique
Suzaku-WAM soft gamma-ray all-sky monitor by the earth occultation technique C.Kira 1,Y.Fukazawa 1,T.Asano 1, T.Takahashi 1,T.Uehara 1, Y.Hanabata 1, H.Takahashi 1, K.Yamaoka 2,M.Tashiro 3,Y.Terada 3,
Cadmium Zinc Telluride (CZT) Detectors
Cadmium Zinc Telluride (CZT) Detectors Lee Sobotka (Presenter: Walter Reviol) Oak Ridge, March 2003 WHY: Small portable/mateable device primarily for fast-beam spectrosc. CZT 1) Effective Z ~ 50 PE(dominates
PAMELA: a Satellite Experiment for Antiparticles Measurement in Cosmic Rays
PAMELA: a Satellite Experiment for Antiparticles Measurement in Cosmic Rays PAMELA scientific objectives Detector s overview Subsystems description PAMELA status Massimo Bongi Universita degli Studi di
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
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.
Cosmic Rays at 120,000 feet above Antarctica The Advanced Thin Ionization Calorimeter (ATIC) Experiment
Cosmic Rays at 120,000 feet above Antarctica The Advanced Thin Ionization Calorimeter (ATIC) Experiment ATIC is a ~4,000 pound experiment, carried to the near-space environment (~23 miles) by a large volume
1. Motivation & Detector concept 2. Performance 3. Confirmation experiments 4. Summary
A. Takada, T. Tanimori, H. Kubo, J. D. Parker, T. Mizumoto, Y. Mizumura, T. Sawano, K. Nakamura, Y. Matsuoka, S. Komura, S. Nakamura, M.Oda, K. Miuchi, S. Kurosawa 1. Motivation & Detector concept 2. Performance
GLAST and beyond GLAST: TeV Astrophysics
GLAST and beyond GLAST: TeV Astrophysics Outline: Greg Madejski Assistant Director for Scientific Programs, SLAC / Kavli Institute for Astrophysics and Cosmology Recent excitement of GLAST and plans for
arxiv:astro-ph/ v1 18 Dec 2002
The InFOCµS Hard X-ray Telescope: Pixellated CZT Detector/Shield Performance and Flight Results arxiv:astro-ph/0212428v1 18 Dec 2002 Wayne H. Baumgartner a,b, J. Tueller a, H. Krimm a, S. Barthelmy a,
The path towards measuring Cosmic Ray Air Showers from Space
The path towards measuring Cosmic Ray Air Showers from Space Francesca Bisconti KSETA Workshop 2017 13-15 February 2017 - Durbach KIT The Research University in the Helmholtz Association www.kit.edu Outline
Monte-Carlo simulations of the expected imaging performance of the EXIST high-energy telescope
Monte-Carlo simulations of the expected imaging performance of the EXIST high-energy telescope S. V. Vadawale *a, J. Hong a and J. E. Grindlay a and G. Skinner b a Harvard-Smithsonian Center for Astrophysics,
Recent and Future Observations in the X-ray and Gamma-ray Bands: Chandra, Suzaku, GLAST, and NuSTAR
SLAC-PUB-11572 November 2005 Recent and Future Observations in the X-ray and Gamma-ray Bands: Chandra, Suzaku, GLAST, and NuSTAR Greg Madejski Stanford Linear Accelerator Center and KIPAC, Stanford CA
Effect of the time characteristics of the Compton camera on its performance
Effect of the time characteristics of the Compton camera on its performance Chibueze Zimuzo Uche Howell Round Michael Cree School of Engineering University of Waikato Introduction Anger camera Compton
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,,
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
The Fermi Gamma-ray Space Telescope
Abstract The Fermi Gamma-ray Space Telescope Tova Yoast-Hull May 2011 The primary instrument on the Fermi Gamma-ray Space Telescope is the Large Area Telescope (LAT) which detects gamma-rays in the energy
The Large Area Telescope on-board of the Fermi Gamma-Ray Space Telescope Mission
The Large Area Telescope on-board of the Fermi Gamma-Ray Space Telescope Mission 1 Outline Mainly from 2009 ApJ 697 1071 The Pair Conversion Telescope The Large Area Telescope Charged Background and Events
X-ray Polarimetry with gas proportional counters through rise-time
X-ray Polarimetry with gas proportional counters through rise-time K. Hayashida, T. Horikawa, Y. Nakashima, H. Tsunemi (Osaka University, Japan) Acknowledge to Y. Namito (KEK, Japan) N.Tokanai (Yamagata
Future Gamma-Ray Observations of Pulsars and their Environments
Future Gamma-Ray Observations of Pulsars and their Environments David J. Thompson NASA Goddard Space Flight Center GLAST Large Area Telescope Collaboration djt@egret.gsfc.nasa.gov D. Thompson 363 rd Heraeus
Small Satellite Platform Imaging X-Ray Polarimetry Explorer (IXPE) Mission Concept and Implementation
Small Satellite Platform Imaging X-Ray Polarimetry Explorer (IXPE) Mission Concept and Implementation 31 st Annual AIAA/USU Conference on Small Satellites Utah State University, Logan, UT, USA August 6-10,
THE AMS RICH COUNTER
THE AMS RICH COUNTER G. BOUDOUL ISN Grenoble ISN-GRENOBLE 1 The AMS RICH collaboration: Bologna, Grenoble, Lisbon, Madrid, Maryland, Mexico 2 The AMS collaboration UNAM S.C.C. TING (MIT), PI 3 AMS Scientific
CRaTER Pre-Environmental Review (I-PER) Science Requirements Update
CRaTER Pre-Environmental Review (I-PER) Science Requirements Update Justin C Kasper Smithsonian Astrophysical Observatory September 10-11, 2007 Outline Instrument Overview Verification Methods Science
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
Calibration of photo sensors for the space-based cosmic ray telescope JEM-EUSO
Calibration of photo sensors for the space-based cosmic ray telescope JEM-EUSO Michael Karus for the JEM-EUSO Collaboration Carpathian Summer School of Physics 2014 Sinaia Romania July 2014 Michael Karus
Gamma-ray Astrophysics
Gamma-ray Astrophysics AGN Pulsar SNR GRB Radio Galaxy The very high energy -ray sky NEPPSR 25 Aug. 2004 Many thanks to Rene Ong at UCLA Guy Blaylock U. of Massachusetts Why gamma rays? Extragalactic Background
Discovery of TeV Gamma-ray Emission Towards Supernova Remnant SNR G Last Updated Tuesday, 30 July :01
Background-subtracted gamma-ray count map of SNR G78.2+2.1 showing the VERITAS detection (VER2019+407). For details, see Figure 1 below. Reference: E. Aliu et al. (The VERITAS Collaboration), Astrophysical
Hard X-ray Polarimeter for Small Satellite: Design, Feasibility Study, and Ground Experiments
Hard X-ray Polarimeter for Small Satellite: Design, Feasibility Study, and Ground Experiments Kiyoshi Hayashida a*, Tatehiro Mihara b, Syuichi Gunji c and Fuyuki Tokanai c a Osaka University, 1-1 Machikaneyama-cho,
The high resolution X-ray imaging detector planes for the MIRAX mission
Journal of Instrumentation OPEN ACCESS The high resolution X-ray imaging detector planes for the MIRAX mission To cite this article: B H G Rodrigues et al View the article online for updates and enhancements.