Precise Low-Energy Electron Tracking Using a Gaseous Time Projection Chamber for the Balloon-Borne Gamma Ray Compton Telescope

Similar documents
1. Motivation & Detector concept 2. Performance 3. Confirmation experiments 4. Summary

1. Motivation & Detector concept 2. Performance 3. Applications 4. Summary

1. MeV gamma ray Imaging & ETCC 2. Results of SMILE-I 3. Preparations of SMILE-II

Motivation Electron-Tracking Compton Telescope 1 st Flight of SMILE Preparation for next step summary

1. Motivation & Detector concept 2. Performance 3. Confirmation experiments 4. Summary

Experiment of the 30 cm-cube ETCC under the Intense Radiations with Proton Beam

Motivation Electron-Tracking Compton Telescope 1 st Flight of SMILE Preparation for next step summary

Balloon-borne experiment for observation of sub-mev/mev gamma-rays from Crab Nebula using an Electron Tracking Compton Camera

Observation of Gamma-Rays from Relativistic Electron Precipitation with Balloon Experiment around the Polar regions

A. Takada (Kyoto Univ.)

arxiv: v1 [physics.ins-det] 6 Aug 2015

Development of a new MeV gamma-ray camera

The simulation of the Electron Tracking Compton Camera with a gaseous time projection chamber and a scintillator

PoS(ICRC2015)1019. Balloon-Borne Experiment for Deep Sky Survey of MeV Gamma Rays using an Electron-Tracking Compton Camera

1. MeV gamma ray Imaging & ETCC 2. Results of SMILE-I 3. Preparations of SMILE-II. A. Takada (Kyoto Univ.)

TitleDevelopment of an MeV gamma-ray ima. works must be obtained from the IEE

Micro Pixel Chamber Operation with Gas Electron Multiplier

Joe Parker for the Cosmic Ray γ Group Kyoto University

NEWAGE. Kentaro Miuchi (Kyoto University) (New generation WIMP search with an advanced gaseous tracker experiment)

A NEW GENERATION OF GAMMA-RAY TELESCOPE

Imaging detection for GRBs & SNe with high sensitivity and good polarimetry by Electron Tracking Compton camera

Direction-Sensitive Dark Matter Search --NEWAGE--

Performance of the Gamma-ray Imaging Detector with Micro-TPC

Title Rays based on Geometrical Optics

Study of the HARPO TPC for a high angular resolution g-ray polarimeter in the MeV-GeV energy range. David Attié (CEA/Irfu)

Establishment of Imaging Spectroscopy of Nuclear Gamma-Rays based on Geometrical Optics

A novel design of the MeV gamma-ray imaging detector with Micro-TPC

Direction-Sensitive Dark Matter Search --NEWAGE--

Xenon Compton Telescopes at Columbia: the post LXeGRIT phase. E.Aprile. Columbia University

Liquid Argon TPC for Next Generation of MeV Gamma-ray Satellite

Non-thermal emission from pulsars experimental status and prospects

The Path From COSI to COSI-X

The Compton Spectrometer and Imager A balloon- borne gamma- ray spectrometer, polarimeter, and imager

Development of a 3D-Imaging Calorimeter in LaBr 3 for Gamma-Ray Space Astronomy

Extreme high-energy variability of Markarian 421

Development of Next Generation Compton Gamma-ray Telescope Hiroyasu Tajima Stanford Linear Accelerator Center

TPC-like analysis for thermal neutron detection using a GEMdetector

Detector R&D in KAPAC

Semi conductor detectors for soft gamma-ray astrophysics

Soft Gamma-ray Detector (SGD) for the NeXT mission and beyond Astro-E2 Tadayuki Takahashi

Development of High-Z Semiconductor Detectors and Their Applications to X-ray/gamma-ray Astronomy

E. Caroli(1), R. M. Curado da Silva(2), J.B. Stephen(1), F. Frontera(1,3), A. Pisa (3), S. Del Sordo (4)

Prompt gamma measurements for the verification of dose deposition in proton therapy. Contents. Two Proton Beam Facilities for Therapy and Research

Makoto; Tanimori, Toru. Creative Commons license, users wil

Detector R&D at KIPAC

arxiv:astro-ph/ v1 26 Sep 2003

Drift plane. substrate (20ÉIm polyimide) 200ÉIm. Back strip (180ÉIm width) Base (Ceramic) Anode strip (10ÉIm width) Cathode strip (100ÉIm width)

Dark Matter Particle Explorer: The First Chinese Cosmic Ray and Hard γ-ray Detector in Space

Expected detection rate of gravitational wave estimated by Short Gamma-Ray Bursts

The Large Area Telescope on-board of the Fermi Gamma-Ray Space Telescope Mission

Gamma-ray Astrophysics

Background and Sensitivity Simulation of a Space Based Germanium Compton Telescope

Preliminary results from gamma-ray observations with the CALorimeteric Electron Telescope (CALET)

Development of a Hard X-Ray Polarimeter for Solar Flares and Gamma-Ray Bursts

Detector R&D at KIPAC. Hiro Tajima Kavli InStitute of Particle Astrophysics and Cosmology

X-ray polarimetry and new prospects in high-energy astrophysics

Results of a Si/CdTe Compton Telescope

Astrophysics with GLAST: dark matter, black holes and other astronomical exotica

Improvement of Spatial Resolution by Selfconsistent Full Muon Track Reconstruction in Gaseous Detectors

THE AMS RICH COUNTER

VERITAS Observations of Starburst Galaxies. The Discovery of VHE Gamma Rays from a Starburst Galaxy

The Extreme Universe Rene A. Ong Univ. of Michigan Colloquium University of California, Los Angeles 23 March 2005

AGIS (Advanced Gamma-ray Imaging System)

GLAST Large Area Telescope:

Observation of Crab Nebula by Nuclear Compton Telescope (NCT)

Gamma-Ray Polarimetry in the Pair Production Regime

The Silicon-Tungsten Tracker of the DAMPE Mission

Special Topics in Nuclear and Particle Physics

Status of the MAGIC telescopes

THE Compton camera is the most promising approach

HARPO: Measurement of polarised gamma rays (1.7 to 72MeV) with the HARPO TPC

The MEGA Advanced Compton Telescope Project

Gamma-Ray Astronomy. Astro 129: Chapter 1a

The Fermi Gamma-ray Space Telescope

for the HARPO Collaboration: *

Particle Energy Loss in Matter

GRAINE project: Cosmic Gamma-ray Observation by Balloon-Borne Telescope with Nuclear Emulsion

Accretion Disks. 1. Accretion Efficiency. 2. Eddington Luminosity. 3. Bondi-Hoyle Accretion. 4. Temperature profile and spectrum of accretion disk

arxiv:astro-ph/ v2 4 Dec 2002

Recent Observations of Supernova Remnants

detector development Matthias Beilicke X ray Science Analysis Group meeting (12 April 2013, Monterey, CA) Collaborators: GSFC, BNL

Experimental Particle

Neutron Structure Functions and a Radial Time Projection Chamber

Particle Energy Loss in Matter

Dr. John Kelley Radboud Universiteit, Nijmegen

Development of semiconductor imaging detectors for a Si/CdTe Compton camera

Radiation Issues in GLAST Si

Search for high energy neutrino astrophysical sources with the ANTARES Cherenkov telescope

arxiv: v1 [astro-ph.im] 6 Dec 2010

MAX, a Laue Diffraction Lens for nuclear astrophysics

Developing a test procedure for neutron detection/non detection using a Small TPC Prototype

Detectors for astroparticle physics

The LHAASO-KM2A detector array and physical expectations. Reporter:Sha Wu Mentor: Huihai He and Songzhan Chen

Detectors in Nuclear and High Energy Physics. RHIG summer student meeting June 2014

GLAST and beyond GLAST: TeV Astrophysics

The MEGA Project. Key words: gamma-ray astronomy, medium energies, MEGA PACS: K

Gamma-ray observations of millisecond pulsars with the Fermi LAT. Lucas Guillemot, MPIfR Bonn. NS2012 in Bonn 27/02/12.

ATLAS New Small Wheel Phase I Upgrade: Detector and Electronics Performance Analysis

Micromegas detectors & the Great Pyramid. S. Procureur

arxiv: v1 [physics.ins-det] 1 Nov 2011

Transcription:

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. Mizumura, D. Tomono, T. Sawano, K. Nakamura, Y. Matsuoka, S. Komura, Y. Sato, S. Nakamura, K. Miuchi, S. Kabuki, Y. Kishimoto, S. Kurosawa, S. Iwaki, M. Tanaka, M. Ikeno, T. Uchida Contents i. MeV gamma ray astronomy ii. Electron Tracking Compton Camera and SMILE-II iii. New DAQ system for SMILE-II ETCC iv. Performances of SMILE-II flight model ETCC 2013 IEEE Nuclear Science Symposium, October 29, 2013 @ COEX, Seoul, Korea, N10-2

Motivation (sub-mev/mev gamma-ray astronomy) Nucleosynthesis SNR : Radio-isotopes Galactic plane : 26 Al 60 Fe Annihilation Acceleration GRB, Jet (AGN) : Synchrotron + Inverse Compton Strong Gravitational Potential Black Hole : accretion disk, π 0 Etc. Gamma-ray Pulsar, solar flare Bad Sensitivity Good erg / (cm 2 sec) Astro-H Sensitivity Fermi EGRET Obs. Time : 10 6 sec Air Cherenkov The observation of continuum component is important. Where are MeV gamma-ray objects? There are many background events which obstruct the observations. Requirements for the next-generation detectors are Wide-band detection Large Field of View Background rejection

Electron Tracking Compton Camera (ETCC) for SMILE μ-tpc GSO ASIC FPGA 1 m GSO Schematic of ETCC (left) and photograph of flight model ETCC for SMILE-II experiment (right) SMILE experiment μ T P C G S O SMILE-I (2006) SMILE-II Size (10 10 15)cm 3 (30 30 30)cm 3 Readout Number Readout Pitch pixel number 256 strips /10 cm 384 strips /30 cm 400 μm 800 μm 2112 pixels 6912 pixels

370 mm 22 cm (10 10 15)cm 3 μ -TPC &GSO μ-tpc readout for SMILE-I and SMILE-II SMILE-I ETCC (30cm) 3 μ -TPC SMILE-II ETCC 11.8 cm GSO readout circuit ASD(256ch/10cm) 4.5 kg 560 mm GSO & GSO readout circuit 1 m 1 m SMILE-I FM ETCC encoder(1 board/1etcc) 7.8 kg SMILE-II FM ETCC new readout board (128 strips/10 cm) conventional readout circuit... massive takes up a lot of space high electric power consumption ASIC chip transistor type strip number per 1 ASIC chip ASD system (for SMILE-I) bipolar transistor 4 16 new readout board (for SMILE-II) CMOS transistor ->developed new readout circuit power consumption 0.24 W/strip 0.17W/strip

1 10 100 1000 Cathode 100MHz clock(0-1023) Anode Example TPC data of SMILE-II ETCC with new readout board TPC hit data TPC FADC data muon track electron track TPC 3D reconstructed track (SMILE-II ETCC) muon track electron track strip number(0-383) SMILE-I 10cm ETCC SMILE-II 10cm ETCC Number of hit pixel strips SMILE-II 30cm ETCC 0 100 200 300 TPC 3D reconstructed hit data (SMILE-I ETCC) Changed saving method of TPC hit data particle tracks are clearer than ever We can detect recoil electrons perfectly

Example data of SMILE-II ETCC with new DAQ system 137 Cs(0.85MBq) zenith = 0 z = 2055 mm 137 Cs source ETCC reconstructed incidentγ φgeo φkin Incidentγ (to source) Scatter Point PC for command sending Track range Absorption Point We can reconstruct the incident gamma rays by using the scattering point, direction and gamma ray energy, recoil direction and electron energy event by event.

point sources Performances of SMILE-II FM ETCC measurement 10 simulation present value Since we can detect almost all scattered electrons, the measured efficiency is similar to the simulated one. incident γ scattered γ recoil electron ARM : accuracy of the scattering angle SPD : accuracy of the scattering plane effective area 10cm 2 -> reach the efficiency of COMPTEL Legacy and Advanced Compton Imaging ARM 5.3º (FWHM) @662keV SPD 93º (FWHM) @662keV

1088mm In the environment of high background, SMILE-II ETCC system operates correctly and shows powerful imaging ability. Further analysis of the data will be done. Measurement in the environment of high background level (@RCNP Osaka Univ.) Date 2013/10/17 trigger rate : 16.2 khz data saving event rate : 394 Hz Dead Time : 59.6% 137 Cs: 0.84 MBq MIP neutron & proton event Compton e- no cut TPC volume cut volume cut + de/dx cut target (water) lead proton beam 137 Cs source Track range vs energy(de/dx) ETCC target source (-125,167) Energy Spectra after energy cut around 662 kev 30cm ETCC proton beam

Conclusion We have been developing the flight model (30 cm) 3 ETCC for SMILE-II experiment. Since we changed the algorithm for taking track hit data of μ-tpc, hit number per event is increased, and almost all recoil electron can be taken. From the result of the simulation, we can achieve the efficiency 10 times higher than the present one by changing the gas species and pressure of the TPC. For SMILE-II ETCC, we confirmed the detector operates correctly in the high background rate.

Fin My colleagues S. Komura, NPO2-122, Performance Improvement of an Electron- Tracking Compton Camera by a New Track Reconstruction S. Sonoda, M12-10, The Performance Evaluation of the Electron Tracking Compton Camera D. Tomono, N28-2, First Application to Environmental Gamma-Ray Imaging with an Electron Tracking Compton Camera