Prototype Performance in D0 test stand & fiber intrinsic performance with KEK test beam M.Yoshida (Osaka Univ.) Osaka.

Slides:



Advertisements
Similar presentations
MICE Collaboration MTG IIT – Feb 2002 The Fiber Tracker Option for MICE Spectrometers The D0 Central Fiber Tracker – Experience and Implications for MICE.
Advertisements

SciFi Tracker DAQ M. Yoshida (Osaka Univ.) MICE meeting at LBNL 10.Feb.2005 DAQ system for KEK test beam Hardware Software Processes Architecture SciFi.
Jin Huang Los Alamos National Lab.  Cited from March collaboration Meeting EC group Internal Communication Jin Huang 2 Preshower ID power drop significantly.
Status of MICE Tracker System H. Sakamoto, Osaka University (on behalf of the MICE Collaboration) International Muon Ionization Cooling Experiment (MICE)
KEK Test Beam Phase II Plan Makoto Yoshida (Osaka Univ.) MICE FT Daresbury 2005/8/30.
KEK beam test H. Sakamoto. Purpose To optimize a concentration of the second dopant for scintillating fibers KEK beam test to study light yields for various.
First Results from Tracker 1  Cryostat Commissioning  AFE/VLSB Firmware and Readout  Cosmic Ray Setup  Tracker Readout  Software  Trigger Timing.
1 Scintillating Fibre Cosmic Ray Test Results Malcolm Ellis Imperial College London Monday 29 th March 2004.
Tracker DAQ Makoto Yoshida (Osaka Univ.) MICE Frascati 2005/6/27.
1 Status of Cosmic Analysis Malcolm Ellis Imperial College London Wednesday 10 th March 2004.
Status of the MICE SciFi Simulation Edward McKigney Imperial College London.
1 VLPC system and Cosmic Ray test results M. Ellis Daresbury Tracker Meeting 30 th August 2005.
SciFi Tracker DAQ M. Yoshida (Osaka Univ.) MICE Tracker KEK Mar. 30, 2005.
Prototype Performance in D0 test stand M.Yoshida (Osaka Univ.)
KEK Test Results / Plans Akira SATO Osaka University, Japan.
KEK Analysis Report Makoto Yoshida Osaka Univ. 2006/06/10 MICE CM15.
KEK Beam Test Koji YOSHIMURA KEK MICE Collaboration Meeting Koji YOSHIMURA KEK MICE Collaboration Meeting
1 Online data quality and monitoring M. Ellis Daresbury DAQ Meeting 31 st August 2005.
MICE Video MTG 9/25/2002 MICE Fiber Tracker Design Update Requirements and Proposed Detector Implementations A. Bross Fermilab.
2005/10/22 MICE CM at RAL, Tracker Parallel, Makoto Yoshida 1 KEK test beam - introduction - M. Yoshida MICE CM tracker parallel 2005/10/ /10/22.
Clear Fiber and Wave Guide Fab. Makoto YOSHIDA (Osaka Univ.) July MICE FT
M. Ellis - 11th February 2004 Sci Fi Cosmic Light Yield 2 views 3 views.
1 KEK Beam Test Analysis Hideyuki Sakamoto 15 th MICE Collaboration Meeting 10 st June,2006.
Tracking Detectors Working Group MICE Collaboration Meeting March 30, 2004 A. Bross.
1 G4MICE Analysis of KEK Test Beam Aron Fish Malcolm Ellis CM15 10th June 2006.
1 Status of the MICE SciFi Tracker Malcolm Ellis Imperial College London Tuesday 9 th March 2004.
J. Estrada - Fermilab1 AFEII in the test cryostat at DAB J. Estrada, C. Garcia, B. Hoeneisen, P. Rubinov First VLPC spectrum with the TriP chip Z measurement.
Takashi Matsushita Imperial College T. Matsushita 1 Station5 in UK.
CFT Calibration Calibration Workshop Calibration Requirements Calibration Scheme Online Calibration databases.
Tracker Summary Makoto Yoshida Osaka Univ. MICE Frascati June 28 th, 2005.
MICE Berkeley, Oct 2002 MICE Spectrometer Design Proposed Tracker Implementations A. Bross Fermilab.
1 MICE Tracker Update M. Ellis UKNFIC Meeting 25 th August 2005.
2005/3/271 3HF 蛍光体を添加した Sci-Fi の基礎 開発 阪大理 (A) 青木正治 有本靖 久野良孝 栗山靖敏 佐藤朗 田窪洋介 中丘末広 中原健吾 堀越篤 松島朋宏 吉田誠 高エ研 (B) 五十嵐洋一 横井武一郎 吉村浩司 FNAL (C) Alan Bross Imperial.
Measurement of 'intrinsic' properties of scintillating fibers H. Sakamoto Osaka University, Japan A.Sato M. Yoshida Y. Kuno Osaka Univ. K. Yoshimura KEK.
1 SciFi Results and Comparison Malcolm Ellis, for the MICE Scintillating Fibre Group Abingdon, 31 st October 2003.
1 MICE Tracking Detectors Malcolm Ellis NFMCC Meeting 12 th March 2006.
THE FORWARD PROTON DETECTOR AT DZERO Gilvan Alves Lafex/CBPF 1) MOTIVATION 2) DETECTOR OPTIONS 3) FPD R&D 4) OUTLOOK Lishep 98 Lafex/CBPF Feb 17, 1998.
Future Beam Test Plans of the GLD Calorimeter Aug 学術創成会議 Satoru Uozumi (Shinshu) for the GLD calorimeter group We are planning to have two beam.
Fiber Tracker Update Edward McKigney Imperial College July 3 rd, 2002.
Start Counter Collaboration Meeting September 2004 W. Boeglin FIU.
TOP counter overview and issues K. Inami (Nagoya university) 2008/7/3-4 2 nd open meeting for proto-collaboration - Overview - Design - Performance - Prototype.
Status of cosmic-ray test of the SciFi prototype and SciFi software in G4MICE M. Yoshida (Osaka Univ.)
All DØ Meeting, 12/01/00 Central Fiber Tracker Light Guide Performance Thomas Nunnemann Fermilab 90 days before RunII … (a.k.a. 12/01/00)
1M. Ellis - NFMCC - 31st January 2007 MICE Tracker.
MICE Phase 1 Koji Yoshimura KEK June
KEK beam test in May 2005 Makoto Yoshida Osaka Univ. MICE Frascati June 27 th, 2005.
1M. Ellis - 17th May 2007 SciFi Decoding (Everything you never wanted to know but couldn’t avoid going over and over)  VLSB Data (unpacking to AFE, MCM,
1 KEK test-beam software progress Malcolm Ellis MICE Video Conference 4 th May 2005.
1 A first look at the KEK tracker data with G4MICE Malcolm Ellis 2 nd December 2005.
2005/10/24 MICE CM at RAL, KEK test beam, Makoto Yoshida 1 KEK Beam Test for MICE SciFi Tracker - KEK-PS T585 - M. Yoshida MICE 2005/10/ /10/24.
Tracker Summary Alan Bross MICE CM17 CERN February 25, 2007.
VLPC System Update A.Bross MICE CM Feb 9, Cryo  Production cryostats 1 and 2 ran smoothly at operating temperature  However, Cassette 109 in cryo.
KEK Test Beam Phase I (May 2005) Makoto Yoshida Osaka Univ. MICE-FT Daresbury Aug 30th, 2005.
Database David Forrest. What database? DBMS: PostgreSQL. Run on dedicated Database server at RAL Need to store information on conditions of detector as.
F Don Lincoln, Fermilab f Fermilab/Boeing Test Results for HiSTE-VI Don Lincoln Fermi National Accelerator Laboratory.
Analysis for QA (temporary) Hideyuki Sakamoto 1 st October 2007 MICE Tracker Phone Meeting.
1 Light Yield results from the KEK tracker test using G4MICE M. Ellis Tracker Phone Meeting 25 th January 2006.
T585 analysis status /2/2 HIDEYUKI SAKAMOTO Contents On small light yield problem checked by Aron’s information Tracking status Transverse and Longitudinal.
Summary of final results from MICE note: “ MICE Scintillating Fibre Tracker Prototype - First progress report - ” M.Yoshida (Osaka Univ.) for the SciFi.
T585 analysis status 2005/12/02 HIDEYUKI SAKAMOTO This analysis was done by RUN# (+1.0 GeV/c normal beam run) For the problem of small light yield.
Station Acceptance Test. 22/02/2007 M. Takahashi 2 Lab Layout at IC.
1M. Ellis - MICE Tracker PC - 1st October 2007 Station QA Analysis (G4MICE)  Looking at the same data as Hideyuki, but using G4MICE.  Have not yet had.
A Brand new neutrino detector 「 SciBar 」 (2) Y. Takubo (Osaka) - Readout Electronics - Introduction Readout electronics Cosmic ray trigger modules Conclusion.
Upgrade with Silicon Vertex Tracker Rachid Nouicer Brookhaven National Laboratory (BNL) For the PHENIX Collaboration Stripixel VTX Review October 1, 2008.
20 April 2007MICE Tracker Phone Meeting1 Analysis of cosmic/self-triggerd data of station 5 Hideyuki Sakamoto MICE Tracker Phone Meeting 20 th April 2007.
Future Beam Test Plans of the Calorimeter Group Aug 学術創成会議 Satoru Uozumi (Shinshu) for the GLD calorimeter group We are planning to have two beam.
The Beam Test at Fermilab:
Preparation for Station Acceptance Test
The E835 SCI-FI Detector In Ferrara It has been built a scintillating fibers detector for the tracking system of exp. E835 (Charmonium spectroscopy) a.
R&D of MPPC in kyoto M.taguchi.
Presentation transcript:

Prototype Performance in D0 test stand & fiber intrinsic performance with KEK test beam M.Yoshida (Osaka Univ.) Osaka

Prototype of SciFi tracker Scifi stations Top (station C) X and V view Middle (station B) X,V,W view Bottom (station A) X and W view ~80 cm X view W view V view

Waveguide Connection bundle of 18 clear fibers (4meter long, 1.05mm  ) bundle of 7×18 clear fibers 126 channel / waveguide

DAQ at D0 test stand VLPC VLPC QE~80% for 3HF spectrum AFE (516 channels) AFE (516 channels) 8 MCM (64 channels in each) 8 MCM (64 channels in each) SVX (Sample&Hold / Degitize) SVX (Sample&Hold / Degitize) SASeq (Stand-Alone Sequencer) SASeq (Stand-Alone Sequencer) VB Program on MS- Excell VB Program on MS- Excell 3HF spectrum 500nm 700nm

Setup in D0 test stand at Fermilab Cryostat for VLPC cassette AFE (Analog Front End board) Trigger Scintillator 36cm×36cm×0.5cm(t) waveguide Lead blocks 10cm thick (100MeV for MIP)

Sinple tracking in X view (H. Sakamoto) Hit definition Threshold is set at 0.5 p.e. Tracking 1D tracking in X view Minimize residual Δ A B C X view × × Δ

Light yield as a function of 3HF concentration 3HF concentration in B station X view (B) 5000ppm W view (B) 3500ppm V view (B) 2500ppm ADC spectrum for each view 3HF5000ppm3500ppm2500ppm ADC mean (p.e.)

3D tracking (M. Ellis) hit definition : 2.5 p.e. threshold tracking in 3D Light yield (3HF2500ppm) Typical cosmic-ray event Most probable ~10.5 p.e.

Results of 3D tracking analysis Resolution: 442 ± 4 (stat) ± 27 (syst)  m Resolution: 442 ± 4 (stat) ± 27 (syst)  m Expectation from fibre geometry: 424 – 465  m (single fiber bunch or two fiber bunch) Expectation from fibre geometry: 424 – 465  m (single fiber bunch or two fiber bunch) Most probable light yield: 10.5 – 11 p.e. (3HF2500ppm) Most probable light yield: 10.5 – 11 p.e. (3HF2500ppm) Expectation based on D0 experience ~10 p.e. Expectation based on D0 experience ~10 p.e. Efficiency: (99.7 ± 0.2)% Efficiency: (99.7 ± 0.2)% Poisson expectation for 10 p.e. signal 99.7% Poisson expectation for 10 p.e. signal 99.7% Dead channels 0.2% (two channels) Dead channels 0.2% (two channels) 0.25% assumed in G4MICE simulation based on D0 experience 0.25% assumed in G4MICE simulation based on D0 experience

Purpose of KEK beam test Intrinsic performance of 3HF scintillating fiber was measured with KEK test-beam in Apr.-May, To optimize a concentration of the 1 st and 2 nd dopant in 3HF fibers Kuraray SCSF-3HF ; 0.35mm-phi, multi-clad, s- type Fibers to be tested: pT(1%) + 3HF(5000ppm) pT(2%) + 3HF(5000ppm) pT(1%) + 3HF(3500ppm) pT(1%) + 3HF(2500ppm) pT(1%) + 3HF(4500ppm) pT(1%) + 3HF(7500ppm) pT(1%) + 3HF(10000ppm) pT(2%) + 3HF(10000ppm)

Attaching SciFi with MICE conn. Attached the SciFi and clear fibers with MICE conn. Attached the SciFi and clear fibers with MICE conn. Clear fibers for pmt ’ s gain calibration Clear fibers for pmt ’ s gain calibration Clear fiber (1.05mmΦ) SciFi (0.35mmΦ): 14fibers SciFi Clear fib

Set up (KEK-T553) Beam area : KEK-T1 beam line Dark box

Setup (T553) mirror pmt SciFi SciFi on support structure in the dark room

Light yield with various 3HF concentration % % % % % % % % 1.2GeV/c  1.2GeV/c proton 0.6GeV/c proton (5000ppm with 20% higher PMT gain )

Result Result Double layer && 4m clear fiber 5000ppm-1% 2500ppm-1%  Almost same light yield

Summary Prototype tracker was constructed in Oct., 2003 Prototype tracker was constructed in Oct., stations 3 stations VLPC readout VLPC readout Light yield of the prototype is measured Light yield of the prototype is measured 1D & 3D tracking have been carried out. 1D & 3D tracking have been carried out. Light yield in pT1%+3HF5000ppm is found to be less than pT1%+2500ppm Light yield in pT1%+3HF5000ppm is found to be less than pT1%+2500ppm Beam test was carried out in Apr.-May 2003 Beam test was carried out in Apr.-May 2003 Check intrinsic performance of 3HF fiber Check intrinsic performance of 3HF fiber PTP1%+3HF5000ppm has the best light yield in the data set w/o waveguide. PTP1%+3HF5000ppm has the best light yield in the data set w/o waveguide. 3HF5000ppm was found to have almost same light yield (4-5p.e.) as 3HF2500ppm after transmitting in 4m-long waveguide 3HF5000ppm was found to have almost same light yield (4-5p.e.) as 3HF2500ppm after transmitting in 4m-long waveguide Discrepancy between the prototype and beam-test Discrepancy between the prototype and beam-test We should estimate systematic errors in the beam-test We should estimate systematic errors in the beam-test We will produce an additional station with both 2500ppm and 5000ppm for prototype upgrade. We will produce an additional station with both 2500ppm and 5000ppm for prototype upgrade.