Prototype Performance in D0 test stand M.Yoshida (Osaka Univ.)

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.

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.

MICE-SciFi team, 14 October 2003 SciFi: progress report Progress: All stations shipped to FNAL … … assembly in progress Measurements: Effect of radiated.

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.

KEK Analysis Report Makoto Yoshida Osaka Univ. 2006/06/10 MICE CM15.

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.

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

Tracking Detectors Working Group MICE Collaboration Meeting March 30, 2004 A. Bross.

DAQ for KEK beam test M.Yoshida (Osaka Univ.). Components VLPC readout –Stand Alone Sequencer (SASeq) Slow < 100Hz –Buffering VLPC data with VME interface.

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.

Tracker QA P. Kyberd, M. Takahashi 1 Quality Assurance for SciFi Tracker (Brunel, FNAL, IC, Osaka) A status report: A procedure for ensuring the quality.

Status of the preparation for KEK test beam M. Yoshida (Osaka Univ.) MICE VC 2005/9/14.

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.

MICE Tracker Readout Increased Data Readout Rate VLSB Development 16 AFE II t boards 8 Visible Light Photon Counter (VLPC) cassettes 4 cryostats.

Tracker Summary Makoto Yoshida Osaka Univ. MICE Frascati June 28 th, 2005.

1. 2 Outline Contract Status  Q.A. plan  construction plan Preparations for construction  populating the construction space Microscope electronics.

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.

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.

Fiber Tracker Update Edward McKigney Imperial College July 3 rd, 2002.

1 MICE Tracker Readout Update, Preparation for Cosmic Ray Tests Cosmic Ray Tests at RAL AFE-IIt Firmware Development VLSB Firmware Development Summary.

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

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.

All Experimenters MeetingDmitri Denisov Week of July 7 to July 15 Summary  Delivered luminosity and operating efficiency u Delivered: 1.4pb -1 u Recorded:

1Malcolm Ellis - Tracker Meeting - 28th November 2006 Electronics - Station Acceptance  Hardware: u 1 MICE cryostat with 1 VLPC cassette. u VME crate,

D0 PMG 6/15/00 PMG Agenda June 15, 2000  Overview (Tuts) u Detector status u Reportable milestones u Financial status u Summary  Response to DOE review.

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.

WBS 1.2.8: AFE II Status and Plans Alan Bross for the DZero Central Fiber Tracker Group DZero Run IIb Detector Upgrade Director’s Review July 15, 2004.

1 MICE Tracker Readout Update Introduction/Overview TriP-t hardware tests AFE IIt firmware development VLSB firmware development Hardware progress Summary.

Analysis for QA (temporary) Hideyuki Sakamoto 1 st October 2007 MICE Tracker Phone Meeting.

D0 PMG February 15, 2001 PMG Agenda February 15, 2001  Overview (Weerts) u Detector status u Reportable milestones u Summary  Operations Organization.

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.

CLAS12 Pre-shower H. Voskanyan (YerPhI)  R&D: Test measurements  Prototype CLAS Collaboration, CLAS12 TWG Meeting February 28, 2007, JLAB.

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.

Tracker Summary M. Yoshida (Osaka Univ.) MICE 2005.Feb.12 th.

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.

G.Barber: Summary of Mice Fibre Tracker Meeting FermiLab 8-12 March Developments during Tracker workshop Contents:- Revised Fibre Pitch Fibre Optic.

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.

Shashlyk DAQ and FEE Status and Plans Pavel Semenov IHEP, Protvino on behalf of the IHEP PANDA group PANDA DAQ and FEE Workshop, Rauischholzhausen Castle.

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.

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.

Presentation transcript:

Prototype Performance in D0 test stand M.Yoshida (Osaka Univ.)

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)

1D tracking (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 p.e

3D tracking (M. Ellis)

3D tracking PTP Mean 13.5p.e. PTP Mean 16.3p.e. Shape is reasonable?  Careful study with MC is needed. (We have more data, should update the figures)

Summary Prototype tracker has been constructed Prototype tracker has been constructed 3 stations 3 stations VLPC readout VLPC readout Light yield is measured Light yield 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 Inconsistent result with test-beam data. Inconsistent result with test-beam data. We will produce another station (made of 2500ppm and 5000ppm) to be added to the prototype, and will test it at KEK-PS in Apr We will produce another station (made of 2500ppm and 5000ppm) to be added to the prototype, and will test it at KEK-PS in Apr