1 Report on analysis of PoGO Beam Test at Spring-8 Tsunefumi Mizuno July 15, 2003 July 21, 2003 revised.

Slides:



Advertisements
Similar presentations
RHESSI Studies of Solar Flare Hard X-Ray Polarization Mark L. McConnell 1, David M. Smith 2, A. Gordon Emslie 4, Martin Fivian 3, Gordon J. Hurford 3,
Advertisements

Dante Nakazawa with Prof. Juan Collar
PMT Calibration Results and the MC simulation Shigeru Yoshida, Chiba University
E : HRS Cross Section Analyses Vincent Sulkosky Massachusetts Institute of Technology GMp Collaboration Meeting September 24 th, 2012.
IEEE_2007Nov.ppt Tsunefumi Mizuno 1 High Sensitivity Balloon-Borne Hard X-Ray/Soft Gamma-Ray Polarimeter PoGOLite November 2 nd, 2007 IEEE Nuclear Science.
Robert Cooper L. Garrison, L. Rebenitsch, R. Tayloe, R. Thornton.
RHESSI Studies of Solar Flare Hard X-Ray Polarization Mark L. McConnell 1, David M. Smith 2, A. Gordon Emslie 4, Martin Fivian 3, Gordon J. Hurford 3,
1 Veto Wall Test Hyupwoo Lee MINERvA/Jupiter Group Meeting June 20, 2007.
In this event 240 eV electron is passing through the MICE Cerenkov detector.
GAMMA RAY SPECTROSCOPY
Main detector types Multi Pixel Photon Counter (MPPC) and Charge Coupled Devices (CCDs) How does it work? 1. Photon hits a pixel producing electron hole.
PoGOandGlast_ ppt 1 Hard X-ray Polarimeter PoGO and GLAST mission ( 硬 X 線偏光観測 PoGO 計画と GLAST との連携 ) November 25, 2005, GLAST Science Workshop.
Rate and Gain Measurements of the 1-m long GEM detector Aiwu Zhang EIC tracking R&D weekly meeting.
X-ray Polarimetry with gas proportional counters through rise-time K. Hayashida, T. Horikawa, Y. Nakashima, H. Tsunemi (Osaka University, Japan)
DAQ_HowTo_ ppt1 How to use DAQ for Argonne Beam Test Tsunefumi Mizuno November 07, 2003 History.
The Transverse detector is made of an array of 256 scintillating fibers coupled to Avalanche PhotoDiodes (APD). The small size of the fibers (5X5mm) results.
The PEPPo e - & e + polarization measurements E. Fanchini On behalf of the PEPPo collaboration POSIPOL 2012 Zeuthen 4-6 September E. Fanchini -Posipol.
IceTop Tank Calibration Abstract This report outlines the preliminary method developed to calibrate IceTop tanks using through going single muon signals.
Data Acquisition System of the PoGOLite Balloon Experiment Hiromitsu TAKAHASHI (Hiroshima University) M. Matsuoka,
14/02/2007 Paolo Walter Cattaneo 1 1.Trigger analysis 2.Muon rate 3.Q distribution 4.Baseline 5.Pulse shape 6.Z measurement 7.Att measurement OUTLINE.
ArgonneBeamTest_ ppt1 Argonne Beam Test preparation Tsunefumi Mizuno Tuneyoshi Kamae
1 Report on analysis of PoGO Beam Test at Spring-8 Tsunefumi Mizuno July 15, 2003.
ArgonneBeamTest_ ppt1 Argonne Beam Test preparation Tsunefumi Mizuno Tuneyoshi Kamae
1 PoGO spring-8 BeamTest preparation Tsunefumi Mizuno and others June 2, 2003 at teleconference.
5th July 00PSI SEU Studies1 Preliminary PSI SEU Studies Study SEU effects by measuring the BER of the link in  /p beams at PSI. Measure the SEU rate as.
PoGO_G4_ ppt1 Study on Key Properties of PoGO by Geant4 Simulator January 28, 2004 Tsunefumi Mizuno History of changes:
We report the result of a beam test on a prototype of Astronomical hard X-ray/soft gamma-ray Polarimeter, PoGO (Polarized Gamma-ray Observer). PoGO is.
1 Report on analysis of PoGO Beam Test at Spring-8 Tsunefumi Mizuno July 15, 2003 July 21, 2003 revised August 1, 2003 updated.
Hard X-ray Polarimeter for Small Satellite Design, Feasibility Study, and Ground Experiments K. Hayashida (Osaka University), T. Mihara (RIKEN), S. Gunji,
V. Vorobel, SuperNEMO meeting, Aussois Vacuum system upgrade Vacuum probe installed Spectrometer sealed – vacuum improved from 300 Pa to 7 Pa.
Electron Detection for Compton Polarimetry Michael McDonald Outline -Compton Effect -Polarimetry -Detectors -Diamond Results.
M. Dugger, February Triplet polarimeter study Michael Dugger* Arizona State University *Work at ASU is supported by the U.S. National Science Foundation.
BigCal Reconstruction and Elastic Event Selection for GEp-III Andrew Puckett, MIT on behalf of the GEp-III Collaboration.
Neutron detection in LHe ( HMI run 2004) R.Golub, E. Korobkina, J. Zou M. Hayden, G. Archibold J. Boissevain, W.S.Wilburn C. Gould.
Nov Beam Catcher in KOPIO (H. Mikata Kaon mini worksyop1 Beam Catcher in the KOPIO experiment Hideki Morii (Kyoto Univ.) for the KOPIO.
Polarization Characteristic of Multi-layer Mirror for Hard X-ray Observation of Astrophysical Objects T. Mizuno 1, J. Katsuta 2, H. Yoshida 1, H. Takahashi.
May 26-27, 2005Tadashi Nomura (Kyoto U), KRare05 at Frascati, Italy1 Studies on High QE PMT Tadashi Nomura (Kyoto U.) Contents –Motivation –Performance.
30/8/05Lisa Fogarty Testing Detector Arrangements For 22 Na(p,γ) Experiment.
00 Cooler CSB Direct or Extra Photons in d+d  0 Andrew Bacher for the CSB Cooler Collaboration ECT Trento, June 2005.
Progress report of the GLAST ACD Beam Test at CERN (Backsplash study) simulation and analysis Tsunefumi Mizuno, Hirofumi Mizushima (Hiroshima Univ.) and.
1. 2 Contents The “Tsubame” Project Description of Hard X-ray Polarimeter (HXCP) Results of X-ray Beam Test Summary.
1 Study of scintillator/PMT properties for PoGO experiment August 25, PoGO Teleconference Tsunefumi Mizuno BGO Transmission.
RF background, update on analysis Rikard Sandström, Geneva University MICE Analysis phone conference, October 30, 2007.
PoGO_collimator_ ppt1 Study of PoGO background dependence on the collimator material/slow scintillator threshold April 21, 2004 Tsunefumi Mizuno.
Results From the Radphi LGD Dan Krop 12/11/03. The Radphi Experiment Radphi Experiment Took Data in Jlab Hall B From May to July Hours Of Beam.
PoGO_G4_ ppt1 Study of optimized fast scintillator length for the astronomical hard X- ray/soft gamma-ray polarimeter PoGO November 1, 2004 Tsunefumi.
Development of a pad interpolation algorithm using charge-sharing.
PoGO_G4_ ppt1 Study of BGO/Collimator Optimization for PoGO August 8th, 2005 Tsunefumi Mizuno, Hiroshima University/SLAC
PoGOLiteMC_ ppt 1 Updated MC Study of PoGOLite Trigger Rate/BG January 30, 2007 Tsunefumi Mizuno (Hiroshima Univ.)
ArgonneResult_ ppt1 Comparison of data and simulation of Argonne Beam Test July 10, 2004 Tsunefumi Mizuno
CdTe prototype detector testing Anja Schubert The University of Melbourne 9 May 2011 Updates.
ArgonneResult_ ppt1 Results of PoGO Argonne Beam Test PoGO Collaboration meeting at SLAC, February 7, 2004 Tsunefumi Mizuno
O Tsunefumi Mizuno, Tuneyoshi Kamae, Jonny Ng, Hiroyasu Tajima (SLAC), John W. Mitchell, Robert Streitmatter (NASA GSFC), Richard C. Fernholz, Edward Groth.
Analysis of    production ► Data taking ► Reaction identification ► Results for double polarization observable F ► Summary Based on data taken in the.
1 Methods of PSD energy calibration. 2 Dependence of energy resolution on many factors Constant term is essential only for energy measurement of single.
1 PMT Univ. of Tokyo Yasuko HISAMATSU ICEPP, The University of Tokyo MEG VRVS meeting Jan. 20th, 2004.
Geometry of the ACD Beam Test at CERN (2002) Tsunefumi Mizuno Overview of the Setup: p.2 ACD tile configuration: pp.3-4 Sn Calorimeter:
ICARUS T600: low energy electrons
The PSD at Pb-Pb run PSD drawbacks at Ar beam
The Lund R3B prototype: In-beam proton tests and simulations
Upgrade of the scintillator testing station in Prague
June 1, 2004 Tsunefumi Mizuno Expected Modulation Factor of PoGO calculated with Geant4 Simulator with PoGO-fix June 1, 2004 Tsunefumi.
Natural CMO+HPGe experiment
BNL electronics: first tests
Very preliminary study of the random background for the BiPo detector (PhoSwich configuration) Work done by Jonathan Ferracci.
Timing Counter Sept CSN I, Assisi 2004 Giorgio Cecchet.
Sergey Abrahamyan Yerevan Physics Institute APEX collaboration
Tadashi Nomura (Kyoto U), KRare05 at Frascati, Italy
HyCal Energy Calibration using dedicated Compton runs
Beam Halo Considerations for Back Angle Running
Presentation transcript:

1 Report on analysis of PoGO Beam Test at Spring-8 Tsunefumi Mizuno July 15, 2003 July 21, 2003 revised

2 Detector/Beam configuration (1) Beam goes from +x to –x Polarization vector of incident beam: along x-axis Beam size (for detector): a circle of 2.68cm diameter Expected beam energy (for detector):83.6 keV (incident beam of 100keV is scattered at 90 degree; this direction picks up the minor component of incident beam whose polarization vector is along z-axis) Expected polarization vector (for detector): along z-axis We decreased the beam rate by a factor of ~100 (from ~10^13Hz down to ~10^11Hz) to prevent pile-up (<=5kHz at the center scintillator). We used an Al block instead of a foil to get an appropriate S/N ratio. Typical trigger rate was ~160Hz and that of background was ~80Hz (Pb block was put in front of the collimator hole). Beam(100keV) polarization vector Collimator (Pb with smaller hole) Collimator (Pb with bigger hole) x y Scatterer (Al block) (Pb sheet)

3 Detector/Beam configuration (2) y z Id: Expected polarization vector 26.8mm 49mm hexagonal scintillators 20cm long Beam direction Beam goes from +x to –x Beam size: a circle of 2.68cm diameter Expected polarization vector: along z-axis Expected beam energy:83.6 keV (incident beam of 100keV is scattered at 90 degree) Right figure corresponds to the rotation angle of 0 degree. We rotated the detector. rotation angle

4 Run summary Data are stored in calibration with 241Am for PMT1 (before beam test): run16_p.txt. Shaper gains (for all PMTs) were adjusted to give ~3V for 60keV. 0 degree run/bg: run17_p.txt and run18_p.txt 30 degree run/bg: run19_p.txt and run20_p.txt 15 degree run/bg: run21_p.txt and run22_p.txt 180 degree run/bg: run23_p.txt and run24_p.txt bg without beam: run25_p.txt calibration with 241Am (after beam test): run26_p.txt Data files with _p are peak data and without are waveform data (binary).

5 Calibration run (1) PMT/scint 1 PMT/scint 2 PMT/scint 3 PMT/scint 4 A gain of PMT1 might be shifted during the test. (from ~3V to ~2.7V)

6 Calibration run (2) PMT/scint 5 PMT/scint 6 PMT/scint 7 PMT/scint 4 PMT/scintillator of #4 is taken by ch4(upper card) and ch8(lower card) and gives consistent spectra -> DAQ itself works well.

7 Energy spectrum of each scint. 0 degree 180 degree Event selection: 2 scintillators are with hit (detection threshold is set at 3keV) Total deposit energy above 45 keV is selected. Energy scale of ch1 might have been shifted during the test and not appropriate for 0 degree run (see page 5). For other PMT/scintillators, no significant difference (modulation) is observed. ch1 ch2 ch3 ch1 ch2 ch3 ch5 ch6 ch7 ch5 ch6 ch7

8 Total energy deposition Event selection:2 scintillators are with hit (detection threshold is set at 3keV) Beam energy was expected to be 83.6 keV (100keV is scattered at 90 degree), but is ~70 keV. -> main component is double scattered photons? might be unpolarized? run17: 0 degreerun23: 180 degree

9 Summary Gain of PMT/scint. #1 seemed to have changed during the test; We have adjusted shaper gain so that 60keV peak comes to 3V, but it was 2.7V in the calibration run (run26). For other PMT/scintillators, no significant difference (modulation) is observed in spectra. This might be due to that beam (after 90degree scattering) was not what we expected. Mean energy(70keV) is lower than calculation (100keV->83.6keV). ->Double scattered beam is the main component? unpolarized?