Hiroyasu Tajima Stanford Linear Accelerator Center VERTEX 2005 November 11, 2005 Chuzenji-lake, Japan GLAST Tracker Woodblock print by Hasui Kawase Kegon.

Slides:



Advertisements
Similar presentations
Marco Bregant Vertex05 - Nikko, November 2005 Dipartimento di Fisica Universit à di Trieste & Istituto Nazionale di Fisica Nucleare (INFN) - Trieste ALICE.
Advertisements

GLAST The GLAST Balloon Flight experiment was performed with the collaboration of NASA Goddard Space Flight Center, Stanford Linear Accelerator Center,
Bulk Micromegas Our Micromegas detectors are fabricated using the Bulk technology The fabrication consists in the lamination of a steel woven mesh and.
2005 LAT-COLLABORATION MEETING Gamma-ray Large Area Space Telescope A walk through the LAT Tracker towers alignment Nicola Omodei INFN-Pisa.
The Gamma-ray Large Area Space Telescope: UNDERSTANDING THE MOST POWERFUL ENERGY SOURCES IN THE UNIVERSE The GLAST LAT Silicon Strip Tracker-Converter.
The Gamma-Ray Large Area Space Telescope: UNDERSTANDING THE MOST POWERFUL ENERGY SOURCES IN THE UNIVERSE Anticoincidence Detector for GLAST Alexander Moiseev,
GLAST LAT ProjectDOE/NASA Review of the GLAST/LAT Project, Feb , 2001 R.P. Johnson, UCSC 1 Silicon-Strip Tracker Converter Robert P. Johnson Santa.
GLAST LAT Silicon Tracker Marcus ZieglerAPS April Meeting The GLAST Silicon Tracker Marcus Ziegler Santa Cruz Institute for Particle Physics University.
GLAST LAT ProjectOctober 14, 2002 Tracker, WBS GLAST Large Area Telescope: Tracker Subsystem WBS Engineering Meeting Tracker Engineering-Model.
GLAST LAT ProjectMarch 24, C Tracker Peer Review, WBS GLAST Large Area Telescope: Tracker Subsystem WBS C: On-Orbit Calibration and.
GLAST LAT Project July 19, 2005 E. do Couto e Silva 1/17 Science Verification Analysis and Calibration GLAST Large Area Telescope Eduardo do Couto e Silva.
GLAST LAT Readout Electronics Marcus ZieglerIEEE SCIPP The Silicon Tracker Readout Electronics of the Gamma-ray Large Area Space Telescope Marcus.
GLAST LAT Readout Electronics Marcus ZieglerIEEE SCIPP The Silicon Tracker Readout Electronics of the Gamma-ray Large Area Space Telescope Marcus.
28 June 2002Santa Cruz LC Retreat M. Breidenbach1 SD – Silicon Detector EM Calorimetry.
GLAST LAT Silicon Tracker Marcus ZieglerAPS April Meeting The GLAST Silicon Tracker Marcus Ziegler Santa Cruz Institute for Particle Physics University.
GLAST Large Area Telescope (LAT) Science Instrument Robert P. JohnsonIEEE NSS 2003 N42-11 GLAST Large Area Telescope: Project Overview Robert P. Johnson.
GLAST LAT Silicon Tracker Marcus ZieglerIEEE The Silicon Tracker Readout Electronics of the Gamma-ray Large Area Space Telescope Marcus Ziegler.
27 th May 2004Daniel Bowerman1 Dan Bowerman Imperial College 27 th May 2004 Status of the Calice Electromagnetic Calorimeter.
GLAST LAT Silicon Tracker Marcus ZieglerAPS April Meeting The GLAST Silicon Tracker Marcus Ziegler Santa Cruz Institute for Particle Physics University.
Hiroyasu Tajima Stanford Linear Accelerator Center Nov 3–8, 2002 VERTEX2002, Kailua-Kona, Hawaii Gamma-ray Polarimetry ~ Astrophysics Application ~
Tracker Subsystem1 GLAST LAT Project FM6 PSR, July 21, 2005 GLAST LAT Tracker Tower6 Pre-Ship Review INFN-Pisa.
GLAST LAT ProjectFebruary 10, 2004 R. Johnson Tracker MCM Production Readiness Review 1 GLAST Large Area Telescope: Tracker Subsystem MCM Production Readiness.
GLAST LAT ProjectDOE/NASA Review of the GLAST/LAT Project, Aug. 14, 2001 Robert P. Johnson 1 GLAST Large Area Telescope: Silicon-Strip Tracker/Converter.
GLAST LAT ProjectIntegration and Test CDR Peer Review, March 28, 2003 Document: LAT-PR Section 8 - Page 1 GLAST Large Area Telescope: I & T Peer.
The Gamma-ray Large Area Space Telescope: The GLAST LAT Silicon Strip Tracker-Converter Robert P. Johnson, U.C. Santa Cruz and the Santa Cruz Institute.
Instrument Performance Sensitivity The improved angular resolution, effective area and field of view of the LAT result in greatly improved source sensitivity,
Tom Tom Davinson School of Physics DESPEC DSSD Working Group Status & Open Issues.
Pixel hybrid status & issues Outline Pixel hybrid overview ALICE1 readout chip Readout options at PHENIX Other issues Plans and activities K. Tanida (RIKEN)
Introduction to gamma-ray astronomy GLAST-Large Area Telescope Introduction to GLAST Science New way of studying astrophysics Schedule of GLAST project.
GLAST:Gamma Ray Large Area Telescope
SiW ECAL Technological Prototype Test beam results Thibault Frisson (LAL, Orsay) on behalf of the CALICE collaboration.
Tracker Production Overview Readout Cables UCSC, SLAC (Parlex) SSD Procurement, Testing SLAC,Japan, Italy (HPK) Electronics Fabrication, burn-in, & Test.
The GLAST Large Area Telescope – Design, construction, test and calibration Luca Latronico (INFN-Pisa), Gloria Spandre (INFN-Pisa) on behalf of the GLAST.
GLAST LAT ProjectMarch 24, F Tracker Peer Review, WBS GLAST Large Area Telescope: Tracker Subsystem WBS F: On-Orbit Calibration and.
The AMS Transition Radiation Detector and the Search for Dark Matter Gianpaolo Carosi Lab for Nuclear Science, MIT The AMS Collaboration Lake Louise Winter.
Fine Pixel CCD for ILC Vertex Detector ‘08 7/31 Y. Takubo (Tohoku U.) for ILC-FPCCD vertex group ILC vertex detector Fine Pixel CCD (FPCCD) Test-sample.
Beam Tests of 3D Vertically Interconnected Prototypes Matthew Jones (Purdue University) Grzegorz Deptuch, Scott Holm, Ryan Rivera, Lorenzo Uplegger (FNAL)
SPIE 4784A-35 GLAST LAT Silicon Tracker Robert P. JohnsonSPIE 47 th Annual Meeting1 GLAST Large Area Telescope Silicon-Strip Tracker Robert P. Johnson.
Swadhin Taneja Stony Brook University On behalf of Vertex detector team at PHENIX Collaboration 112/2/2015S. Taneja -- DNP Conference, Santa Fe Nov 1-6.
GLAST Large Area Telescope (LAT) Overview Peter F. Michelson Instrument Principal Investigator Stanford University William E.
LHCf: installation & commissioning Measurement of Photons and Neutral Pions in the Very Forward Region of LHC Oscar Adriani INFN Sezione di Firenze - Dipartimento.
GLAST LAT ProjectMarch 24, B Tracker Peer Review, WBS GLAST Large Area Telescope: Tracker Subsystem WBS B: EM Mini-Tower Robert Johnson.
Valerio Re, Massimo Manghisoni Università di Bergamo and INFN, Pavia, Italy Jim Hoff, Abderrezak Mekkaoui, Raymond Yarema Fermi National Accelerator Laboratory.
Gamma-ray Large Area Space Telescope 15th INTERNATIONAL WORKSHOP ON VERTEX DETECTORS September , 2006 Perugia, Italy GLAST Silicon Tracker beam.
GLAST The GLAST Balloon Flight experiment was performed with the collaboration of NASA Goddard Space Flight Center, Stanford Linear Accelerator Center,
GLAST LAT ProjectMarch 24, C Tracker Peer Review, WBS GLAST Large Area Telescope: Tracker Subsystem WBS C: Electronics Module Testing.
5-9 June 2006Erika Garutti - CALOR CALICE scintillator HCAL commissioning experience and test beam program Erika Garutti On behalf of the CALICE.
D. M. Lee, LANL 1 07/10/07 Forward Vertex Detector Overview Technical Design Overview Design status.
The DAMPE STK G. Ambrosi INFN Perugia. The DAMPE Detector Mass: 1480 Kg Power: 600 W Data: 16 Gbyte/day Liftime: 5 years 2.
GLAST LAT ProjectQuarterly Review, November 12, 2002 LAT-PR GLAST Large Area Telescope: Tracker Subsystem Robert Johnson Santa Cruz Institute for.
The GLAST Background Model J. F. Ormes 1, W. Atwood 2, T. Burnett 3, E. Grove 4, F. Longo 5, J. McEnery 6, T. Mizuno 7 & S. Ritz 6 on behalf of the GLAST.
Pixel Atsushi Taketani RIKEN RIKEN Brookhaven Research Center 1.Overview of Pixel subsystem 2.Test beam 3.Each Components 4.Schedule 5.Summary.
Gamma-ray Large Area Space Telescope Tower 1 TVAC tests Bad ladders issues.
GLAST LAT ProjectMarch 24, A Tracker Peer Review, WBS GLAST Large Area Telescope: Tracker Subsystem WBS A: Parts and Materials Procurement.
Gamma-ray Large Area Space Telescope -France -Germany -Italy -Japan -Sweden -USA Energy Range 10 keV-300 GeV. GLAST : - An imaging gamma-ray telescope.
Upgrade with Silicon Vertex Tracker Rachid Nouicer Brookhaven National Laboratory (BNL) For the PHENIX Collaboration Stripixel VTX Review October 1, 2008.
DAMPE: now in orbit G. Ambrosi – DAMPE coll.. DAMPE: now in orbit G. Ambrosi – DAMPE coll.
FCAL R&D towards a prototype of very compact calorimeter
Mini-Tower test results
Gamma-ray Large Area Space Telescope ACD Final Performance
Comparison of GAMMA-400 and Fermi-LAT telescopes
Silicon Pixel Detector for the PHENIX experiment at the BNL RHIC
GLAST LAT tracker signal simulation and trigger timing study
Gamma-ray Large Area Space Telescope
GLAST Large Area Telescope:
Gamma-ray Large Area Space Telescope
GLAST Large Area Telescope:
Lessons Learned and Earned Value Management System Assessment
GLAST Large Area Telescope:
Mini Tower Preliminary Results
Presentation transcript:

Hiroyasu Tajima Stanford Linear Accelerator Center VERTEX 2005 November 11, 2005 Chuzenji-lake, Japan GLAST Tracker Woodblock print by Hasui Kawase Kegon fall Chuzenji lake

GLAST Tracker, H. Tajima, VERTEX 2005, NOV. 11, 2005 Outline Overview of GLAST Tracker.  Requirements.  Mechanical and electronics design. Production.  Alignment.  Production issues. Performance.  Bad strips, hit efficiencies.  TOT calibrations.  Threshold, trigger dispersions.  Transient noise issues. Current Status and Future Schedule.

GLAST Tracker, H. Tajima, VERTEX 2005, NOV. 11, 2005 GLAST/LAT Collaboration Gamma-ray Large Area Space Telescope Stanford University & Stanford Linear Accelerator Center NASA Goddard Space Flight Center Naval Research Laboratory University of California at Santa Cruz Sonoma State University University of Washington Texas A&M University – Kingsville Ohio State University Commissariat a l’Energie Atomique, Saclay Ecole Polytechnique, College de France, CENBG (Bordeaux) Hiroshima University Institute of Space and Astronautical Science University of Tokyo Instituto Nazionale di Fisica Nucleare Agenzia Spaziale Italiana Instituto di Fisica Cosmica, CNR Royal Institute of Technology, Stockholm Stockholms Universitet

GLAST Tracker, H. Tajima, VERTEX 2005, NOV. 11, 2005 GLAST/LAT Overview Satellite experiment to observe gamma-try from Universe.  Wide energy range: 20 MeV – 300 GeV  Large effective area: > 8000 cm 2 (5xEGRET)  Wide field of view: > 2 sr (4xEGRET) Scientific objectives.  Dark matter. Neutralino annihilation.  Particle acceleration. Cosmic ray origin Pair-conversion telescope.  “Clear” signature.  Background rejection.  e+e+ e–e–

GLAST Tracker, H. Tajima, VERTEX 2005, NOV. 11, 2005 Instrument Configuration Tracker: conversion, tracking.  Angular resolution is dominated by scattering.  Converter thickness optimization. Calorimeter: energy measurement.  8.4 radiation length.  Use shower development to compensate for the leak. Anti-coincidence detector:  Efficiency > 99.97%. Si Tracker 90 m 2, 228 µm pitch ~0.9 million channels CsI Calorimeter 8.4 radiation length Anti-coincidence Detector Segmented scintillator tiles 99.97% efficiency e+e+ e-e- 

GLAST Tracker, H. Tajima, VERTEX 2005, NOV. 11, 2005 Requirements for Tracker Conversion Efficiency > 58%. Aspect (H/W) ratio < 0.45 (for wide field of view). Active area > 19,000 cm 2 (Fraction > 88%). 6-in-a-row tracker trigger.  Efficiency > 90%.  Single layer trigger rate < 50 kHz.  Trigger jitter 0.5 MIP. Threshold dispersion < 10%. Noise data volume: 40 noise hits per event.  Average Noise occupancy < 5x Hit efficiency > 98% Dead time < 10% for 10 kHz. Power consumption < 160 W. Survival temperature range: -15 – 45 °C. Careful for what you wish in NASA project.

GLAST Tracker, H. Tajima, VERTEX 2005, NOV. 11, 2005 Mechanical Design Readout Cable Multi-Chip Electronics Module (MCM) 2 mm gap 19 Carbon-Fiber Tray Panels Titanium Flexure Mounts Carbon-Fiber Sidewalls (Aluminum covered) Silicon Strip Detectors 18 X-Y Pairs of Planes “Thin” Tungsten Foil (3% X 0 ) 12 Locations “Thick” Tungsten Foil (18% X 0 ) 4 Locations No Tungsten Foil 2 Locations 1 X 2 Y 3 X 4 Y 18 Y 17 X 16 Y 0 Y 5 type of trays.

GLAST Tracker, H. Tajima, VERTEX 2005, NOV. 11, 2005 Tray Structure Silicon Strip Detectors Bias Plane Tungsten Foil Multi-Chip Module Top Layer Wire Bonds Multi-Chip Module Bottom Layer Structural tray panel: C-C machined closeout frame Aluminum honeycomb core CFRP face sheets Microbonding

GLAST Tracker, H. Tajima, VERTEX 2005, NOV. 11, 2005 Readout Electronics Architecture GLAST Tracker Readout Controller (GTRC) 9 GTRC per cable. Communication between 24 GTFE and back-end electronics. TOT measurement from layer-OR trigger signal Emphasis on compactness, minimum of wiring, and redundancy: Serial, LVDS readout and control lines on flat flex-circuit cables. Any single component (GTFE, GTRC, cable) can fail without affecting the other.

GLAST Tracker, H. Tajima, VERTEX 2005, NOV. 11, 2005 Tracker Front-end Electronics GTFE (GLAST Tracker Front-end Electronics) ASIC  Preamplifier - shaper - discriminator  One threshold DAC and one calibration DAC per chip.  64 channels per chip, 24 chips per MCM.  Noise: ~1500 e for 4 SSD ladder.  Gain: ~100 mV/fC.  Peaking time: 1.5 µs.  0.1 mW/channel. GTFE GTRC

GLAST Tracker, H. Tajima, VERTEX 2005, NOV. 11, 2005 SSD SSD reference crosses 8.95 cm 8.95 cm x 8.95 cm. 226 µm pitch. 400 µu thick. Manufactured by HPK. 10,368 wafers. 0.5% rejection fraction. 2.5 µm dicing accuracy. INFN/Pisa

GLAST Tracker, H. Tajima, VERTEX 2005, NOV. 11, 2005 Ladder and Tray Assembly Ladder Assembly  Take advantage of excellent dicing accuracy.  Manual alignment.  Precise SSD alignment within ladder.  No CMM required. Tray Assembly  20 µm ladder placement accuracy. INFN/Pisa

GLAST Tracker, H. Tajima, VERTEX 2005, NOV. 11, 2005 Tower Assembly Alignment pin ~1m 8 type of cables due to space constraint Stacking trays Attach cables Side panel

GLAST Tracker, H. Tajima, VERTEX 2005, NOV. 11, 2005 Tray Alignment by Muon Track X4 X3 X2 X1 X0 real position ideal position res =  x +  z · cot(θ) θ horizontal displacement: 157  m vertical displacement: 81  m MC Data after alignment Residual rms = 137  m Residual rms = 124  m Scattering dominant INFN/Pisa

GLAST Tracker, H. Tajima, VERTEX 2005, NOV. 11, 2005 Production Issues Delamination due to thermal-vacuum cycles.  Kapton bias circuit. Extremely difficult to glue tungsten. Polymer coating of tungsten.  Wire-bonding encapsulation. Silicone contamination from pitch-adapter bonding process. - Eliminate use of silicone based tape. SSD movement due to CTE mismatch of tungsten foil. -Eliminate encapsulation for SSD wire-bonding. -Reduce thermal excursion. Pitch-adapter cracking.  Silent modification of Ni plating process. Flex circuit delivery delays.  Incompetent vender. MCM PWB ASIC Pitch-adapter flex bonded over radius Adhesive Kapton Bias Circuit

GLAST Tracker, H. Tajima, VERTEX 2005, NOV. 11, 2005 Flight Module Delivery All flight modules are delivered and integrated.  Flex cable delivery has been bottle neck. ACD is being integrated. Total Monthly

GLAST Tracker, H. Tajima, VERTEX 2005, NOV. 11, 2005 Hot and Dead Strips Hot strip definitions.  Data mask. Mask noisiest strips to satisfy 5x10 -5 average occupancy. 7 masked strips.  Trigger mask. Mask noisiest strips to satisfy 50 kHz layer trigger rate. Dead strips Mean: 0.8 / layer Hot strips Mean: 0.7 / layer 1%

GLAST Tracker, H. Tajima, VERTEX 2005, NOV. 11, 2005 Disconnected Strips.  Broken pitch adapter.  Disconnected wire-bond between MCM and SSD.  Disconnected wire-bond between SSDs. Broken ladder strips Mean: 4.4 / layer Disconnected strips Mean: 3.0 / layer 1%

GLAST Tracker, H. Tajima, VERTEX 2005, NOV. 11, 2005 Hit Efficiencies Specification: hit efficiency > 98%.  99.0% of layers satisfy the specification.  Average efficiency: 99.6%.  2%

GLAST Tracker, H. Tajima, VERTEX 2005, NOV. 11, 2005 TOT/Calibration DAC Calibration TOT gain is calibrated for each channel. Use MIP signals to calibrate “calibration” DAC. With gain correction Without gain correction ~30% rms ~8% rms

GLAST Tracker, H. Tajima, VERTEX 2005, NOV. 11, 2005 Trigger Jitter Trigger jitter important for ACD veto.  Trigger time walk due to input charge is dominant source of trigger jitter.  Specification: Trigger jitter 0.5 MIP.  Proper threshold setting necessary. Specification Trigger timing for 0.5MIP

GLAST Tracker, H. Tajima, VERTEX 2005, NOV. 11, 2005 Threshold Dispersion Trigger threshold.  Threshold at pulse peak.  Dispersion: 5.9%. (within chip: 5.2%, chip-to-chip: 2.7%). Threshold for data capture.  Strip data is captured ~2 µs after trigger request.  Larger dispersion due to variation of fall time.  Dispersion: 12.0%. (within chip: 8.3%, chip-to-chip: 7.0%). ~2 µs

GLAST Tracker, H. Tajima, VERTEX 2005, NOV. 11, 2005 Transient Noise Issue 6 layers out of 612 layers exhibit transient noise.  Infrequent (0/day – a few/hour).  Confined within one ladder.  Noisy ladder different episode to episode.  Many strips are affected at the same.  No apparent dependence on bias voltage or vacuum. No major effect on operation.  Trigger rate, occupancy within specification on ground. Occupancy time profileLayer-OR time profile Strip profile

GLAST Tracker, H. Tajima, VERTEX 2005, NOV. 11, 2005 Current Status and Future Schedule All flight detector modules are delivered.  Tracker meet all specifications. DAQ integration and online software test.  Now – Jan Environmental test at NRL.  Feb – June Beam test at CERN(?)  Spare modules.  Proposal in preparation.  ~ June Space craft integration. Launch from Kennedy SFC.  Sep  Largest Silicon Detector in the Space. Spitzer Telescope Launch on a Delta II Heavy (near Earth)