SPIE 4784A-35 GLAST LAT Silicon Tracker Robert P. JohnsonSPIE 47 th Annual Meeting1 GLAST Large Area Telescope Silicon-Strip Tracker Robert P. Johnson.

Slides:



Advertisements
Similar presentations
Advanced Implantation Detector Array (AIDA): Update & Issues presented by Tom Davinson on behalf of the DESPEC-DSSD/AIDA collaboration Tom Davinson School.
Advertisements

GLAST The GLAST Balloon Flight experiment was performed with the collaboration of NASA Goddard Space Flight Center, Stanford Linear Accelerator Center,
Detection of Gamma-Rays and Energetic Particles
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 ProjectMarch 24, A Tracker Peer Review, WBS GLAST Large Area Telescope: Tracker Subsystem WBS A: Tracker Test Plan Overview.
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 ProjectDOE/NASA Review of the GLAST/LAT Project, Feb , 2001 S. Ritz 1 GLAST Large Area Telescope: Instrument Design Steven M. Ritz Goddard.
Gamma-ray Large Area Space Telescope IEEE Nuclear Science Symposium Wyndham El Conquistador Resort, Puerto Rico October , 2005 The Gamma Ray Large.
GLAST LAT ProjectMarch 24, C Tracker Peer Review, WBS GLAST Large Area Telescope: Tracker Subsystem WBS C: On-Orbit Calibration and.
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.
GLAST LAT Silicon Tracker Marcus ZieglerAPS April Meeting The GLAST Silicon Tracker Marcus Ziegler Santa Cruz Institute for Particle Physics University.
Eduardo do Couto e Silva - ATC/LM Colloquium, June How many neutralinos are there? Expansion of universe Depletion of neutralinos Creation of neutralinos.
1 Gamma-Ray Astronomy with GLAST May 24, 2008 Toby Burnett WALTA meeting.
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.
T. BurnettGeant Workshop user presentation 1 Geant4 and GLAST Description of the mission and instrument Simulation requirements How we are a little.
GLAST LAT Silicon Tracker Marcus ZieglerAPS April Meeting The GLAST Silicon Tracker Marcus Ziegler Santa Cruz Institute for Particle Physics University.
GLAST Simulations Theodore E. Hierath Louisiana State University August 20, 2001.
Particle Physics and Astrophysics (PPA) Mechanical Engineering Ken Fouts.
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.
1 Arecibo Synergy with GLAST (and other gamma-ray telescopes) Frontiers of Astronomy with the World’s Largest Radio Telescope 12 September 2007 Dave Thompson.
Hiroyasu Tajima Stanford Linear Accelerator Center VERTEX 2005 November 11, 2005 Chuzenji-lake, Japan GLAST Tracker Woodblock print by Hasui Kawase Kegon.
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.
Tom Tom Davinson School of Physics DESPEC DSSD Working Group Status & Open Issues.
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
Tracker Production Overview Readout Cables UCSC, SLAC (Parlex) SSD Procurement, Testing SLAC,Japan, Italy (HPK) Electronics Fabrication, burn-in, & Test.
GLAST LAT ProjectCDR/CD-3 Review May 12-16, 2003 Document: LAT-PR-01967Section 1 Introduction & Science Overview 1 GLAST Large Area Telescope: Introduction.
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.
National Aeronautics and Space Administration November 23, Gamma-ray Large Area Space Telescope (GLAST) Kevin Grady, Project Manager Steven Ritz,
1 Stepping in everyone’s toes ( but for a good cause….) Eduardo do Couto e Silva Software Meeting – January 2001.
GLAST Large Area Telescope (LAT) Overview Peter F. Michelson Instrument Principal Investigator Stanford University William E.
Aa GLAST Particle Astrophysics Collaboration Instrument Managed and Integrated at SLAC/Stanford University The Gamma-ray Large Area Space Telescope (GLAST)
GLAST LAT ProjectMarch 24, B Tracker Peer Review, WBS GLAST Large Area Telescope: Tracker Subsystem WBS B: EM Mini-Tower Robert Johnson.
Gamma Ray Large Area Space Telescope Balloon Flight: Data Handling Overview E. do Couto e Silva, R. Dubois, D. Flath, I. Gable,T. Kamae, A. Kavelaars,
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,
- Performance Studies & Production of the LHCb Silicon Tracker Stefan Koestner (University Zurich) on behalf of the Silicon Tracker Collaboration IT -
Fermi-LAT: A Retrospective on Design, Construction, and Operation and a Look Towards the Future Bill Atwood Dec 6, 2011 HSTD-8 1.
GLAST LAT ProjectMarch 24, C Tracker Peer Review, WBS GLAST Large Area Telescope: Tracker Subsystem WBS C: Electronics Module Testing.
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 ProjectMarch 24, B Tracker Peer Review, WBS GLAST Large Area Telescope: Tracker Subsystem WBS B: Electronic Parts & Materials.
GLAST LAT ProjectQuarterly Review, November 12, 2002 LAT-PR GLAST Large Area Telescope: Tracker Subsystem Robert Johnson Santa Cruz Institute for.
GLAST LAT ProjectMarch 24, 2003 HPS Tracker Peer Review, WBS Section 2-D 1 GLAST Large Area Telescope: Tracker Subsystem WBS Structural.
GLAST LAT ProjectMarch 24, A Tracker Peer Review, WBS GLAST Large Area Telescope: Tracker Subsystem WBS A: Introduction Robert Johnson.
GLAST LAT ProjectMarch 24, A Tracker Peer Review, WBS GLAST Large Area Telescope: Tracker Subsystem WBS A: Parts and Materials Procurement.
1 Study of Data from the GLAST Balloon Prototype Based on a Geant4 Simulator Tsunefumi Mizuno February 22, Geant4 Work Shop The GLAST Satellite.
Gamma-ray Large Area Space Telescope -France -Germany -Italy -Japan -Sweden -USA Energy Range 10 keV-300 GeV. GLAST : - An imaging gamma-ray telescope.
GLAST LAT ProjectPMT Procurement Review May 24, 2002 AntiCoincidence Detector Design Overview 1 GLAST Large Area Telescope: AntiCoincidence Detector (ACD)
DAMPE: now in orbit G. Ambrosi – DAMPE coll.. DAMPE: now in orbit G. Ambrosi – DAMPE coll.
Calorimeter Subsystem of GLAST Large Area Telescope
The Transition Radiation Detector for the PAMELA Experiment
Mini-Tower test results
Gamma-ray Large Area Space Telescope ACD Final Performance
Comparison of GAMMA-400 and Fermi-LAT telescopes
GLAST LAT tracker signal simulation and trigger timing study
Gamma-ray Large Area Space Telescope
GLAST Large Area Telescope:
GLAST Large Area Telescope:
GLAST Large Area Telescope:
GLAST Large Area Telescope:
GLAST Large Area Telescope:
GLAST Large Area Telescope:
GLAST Large Area Telescope:
Presentation transcript:

SPIE 4784A-35 GLAST LAT Silicon Tracker Robert P. JohnsonSPIE 47 th Annual Meeting1 GLAST Large Area Telescope Silicon-Strip Tracker Robert P. Johnson Santa Cruz Institute for Particle Physics Physics Department University of California at Santa Cruz LAT Tracker Subsystem Manager Representing the LAT Collaboration Gamma-ray Large Area Space Telescope

SPIE 4784A-35 GLAST LAT Silicon Tracker Robert P. JohnsonSPIE 47 th Annual Meeting2 Gamma-ray Large Area Space Telescope GLAST Mission  High-energy gamma-ray observatory with 2 instruments:  Large Area Telescope (LAT)  Gamma-ray Burst Monitor (GBM)  Launch vehicle: Delta-2 class  Orbit: 550 km, 28.5 o inclination  Lifetime: 5 years (minimum) GLAST Gamma-Ray Observatory: LAT ~20 MeV and up GBM 20 keV to 20 MeV Spacecraft bus Routine Data LAT GBM

SPIE 4784A-35 GLAST LAT Silicon Tracker Robert P. JohnsonSPIE 47 th Annual Meeting3 GLAST Science Opportunities  Active Galactic Nuclei  Isotropic Diffuse Background Radiation  Endpoints of Stellar Evolution  Neutron Stars/Pulsars  Black Holes  Cosmic Ray Production Sites  Gamma-Ray Bursts  Dark Matter  Solar Physics  DISCOVERY!   40 increase in sensitivity over the previous gamma-ray telescope: EGRET on the NASA Compton Gamma Ray Observatory (1991). EGRET’s view of the universe, in galactic coordinates.

SPIE 4784A-35 GLAST LAT Silicon Tracker Robert P. JohnsonSPIE 47 th Annual Meeting4 Pair-Conversion Telescope  Heavy metal foils (e.g. tungsten) convert high-energy gamma rays into electron- positron pairs.  Detectors interleaved with the converter foils track the charged particles. The gamma-ray direction is reconstructed from the tracks.  A calorimeter absorbs the electromagnetic shower and records the gamma-ray energy.  Veto counters reject background from the predominant charged cosmic rays (electrons, protons and heavy ions). Multiple- scattering limits angular resolution

SPIE 4784A-35 GLAST LAT Silicon Tracker Robert P. JohnsonSPIE 47 th Annual Meeting5 GLAST LAT Overview e+e+ e–e–  Si Tracker 8.8  10 5 channels 185 Watts Grid (& Thermal Radiators) Data acquisition 3000 kg, 650 W (allocation) 1.8 m  1.8 m  1.0 m Effective area ~1 m 2 CsI Calorimeter 8.4 radiation lengths 8 × 12 bars ACD Veto Counters Segmented scintillator tiles

SPIE 4784A-35 GLAST LAT Silicon Tracker Robert P. JohnsonSPIE 47 th Annual Meeting6 Silicon-Strip Detectors  ~80 m 2 of PIN diodes, with P implants segmented into narrow strips.  Reliable, well-developed technology from particle- physics applications.  A/C coupling and strip bias circuitry built in.  >2000 detectors already procured from Hamamatsu Photonics. Very high quality:  Leakage current < 2.5 nA/cm 2  Bad channels < 1/10,000  Full depletion < 100 V cm square Hamamatsu-Photonics SSD before cutting from the 6-inch wafer. The thickness is 400 microns, and the strip pitch is 228 microns.

SPIE 4784A-35 GLAST LAT Silicon Tracker Robert P. JohnsonSPIE 47 th Annual Meeting7 Solid-State Advantages  Thin detectors, placed immediately following the converter foils to minimize errors from multiple scattering.  Nearly 100% efficiency for MIPs, with very low noise:  Tracker can self trigger. No need to be followed by additional trigger counters that would constrict the field of view.  Angular resolution is optimized by guaranteeing a measurement in the first detector plane following the gamma conversion (minimize the lever arm from the multiple scattering).  Very fine segmentation yields detailed information near the conversion vertex, to aid in rejection of background and identification of poorly measured events.  Fast readout (tens of microseconds) prevents loss of data during gamma-ray bursts.  No consumables except for electrical power!  Robust and reliable: low voltage, no gas system, long life.

SPIE 4784A-35 GLAST LAT Silicon Tracker Robert P. JohnsonSPIE 47 th Annual Meeting8 Electronics Packaging Kapton readout cables. Tested SSDs procured from Hamamatsu Photonics 19 “trays” stack to form one of 16 Tracker modules. Electronics and SSDs assembled on composite panels. 4 SSDs bonded in series. Composite panels, with tungsten foils bonded to the bottom face , Carbon composite side panels Chip-on-board readout electronics modules. Electronics mount on the tray edges. “Tray”

SPIE 4784A-35 GLAST LAT Silicon Tracker Robert P. JohnsonSPIE 47 th Annual Meeting9 Electronics Packaging  Dead area within the tracking volume must be minimized.  Hence the 16 modules must be closely packed.  This is achieved by attaching the electronics to the tray sides.  Flex circuits with 1552 fine traces are bonded to a radius on the PWB to interconnect the detectors and electronics. Detector signals, 100 V bias, and ground reference are brought around the 90° corner by a Kapton circuit bonded to the PWB. Composite Panel High thermal conductivity transfer adhesive PWB attached by screws Detector Readout IC Machined corner radius with bonded flex circuit.

SPIE 4784A-35 GLAST LAT Silicon Tracker Robert P. JohnsonSPIE 47 th Annual Meeting10 Readout Electronics  Based on 2 ASICs developed exclusively for this project:  64-channel amplifier-discriminator chip (GTFE); 24 per module.  Readout controller chip (GTRC); 2 per module.  Two redundant readout and control paths for each GTFE chip (“left” or “right”) makes the system nearly immune to single-point failures.  Programmable channel masks and threshold DACs.  Internal, programmable charge-injection system.  Trigger implemented from OR of all channels/layer.

SPIE 4784A-35 GLAST LAT Silicon Tracker Robert P. JohnsonSPIE 47 th Annual Meeting11 Mechanical Structure  Carbon-fiber composite used for radiation transparency, stiffness, thermal stability, and thermal conductivity.  Honeycomb panels made from machined carbon-carbon closeouts, graphite/cyanate-ester face sheets, and aluminum cores.  High-performance graphite/cyanate-ester sidewalls carry the electronics heat to the base of the module.  Titanium flexure mounts allow differential thermal expansion between the aluminum base grid and the carbon-fiber tracker. SSDs Bias Circuits Tungsten Panel MCM Flexure Mounts Thermal Gasket Bottom Tray

SPIE 4784A-35 GLAST LAT Silicon Tracker Robert P. JohnsonSPIE 47 th Annual Meeting12 Performance  The LAT silicon tracker performance has been studied in several ways:  Detailed Monte Carlo simulation.  Beam tests and cosmic-ray studies with prototype detector assemblies.  A high-altitude balloon flight.  Data from the prototypes have been used to tune and validate the simulation model.

SPIE 4784A-35 GLAST LAT Silicon Tracker Robert P. JohnsonSPIE 47 th Annual Meeting Beam Test—Verify Simulation Model Small-aperture first prototype Operated in a tagged  beam at Stanford Data Monte Carlo Published in NIM A446 (2000), 444.

SPIE 4784A-35 GLAST LAT Silicon Tracker Robert P. JohnsonSPIE 47 th Annual Meeting14 Beam Test of a Complete Module  Full-scale Tracker module with 51,200 readout channels operated in positron, photon, and hadron beams at Stanford Linear Accelerator Center.  The Tracker power, noise, and efficiency requirements were met:  99% efficiency with <10  5 noise occupancy.  Only 200  W of power consumed per channel. Hit efficiency versus threshold for 5 GeV positrons. Operating Point NIM 457, 466, & 474

SPIE 4784A-35 GLAST LAT Silicon Tracker Robert P. JohnsonSPIE 47 th Annual Meeting15 Carbon-Composite Mechanical Prototype  First full-scale carbon-composite tracked module mechanical structure.  Thermal cycling, vacuum testing, and random vibration testing have been carried out at the tray and tower-module levels.  Results were satisfactory except that the joint between the corner flexures and the bottom tray failed at the highest vibration levels—work is in progress to reinforce the joint. Full module instrumented for thrust-axis vibration Bottom tray panel, electronics side Bottom tray panel, orthogonal side

SPIE 4784A-35 GLAST LAT Silicon Tracker Robert P. JohnsonSPIE 47 th Annual Meeting16 LAT Tracker Status and Schedule  January 2002: NASA PDR & DOE Baseline Review.  Present: complete the Engineering-Model tracker module:  Complete mechanical-thermal module with dummy silicon detectors.  4 fully instrumented and functional trays.  Winter 2003: Critical Design Review follows Engineering-Model testing.  First 2 of 18 tracker modules completed and ready for qualification testing by the end of  Final tracker modules completed by September  LAT Integration and Test until mid  Launch in 3 rd quarter of 2006.

SPIE 4784A-35 GLAST LAT Silicon Tracker Robert P. JohnsonSPIE 47 th Annual Meeting17 Conclusions  Solid-state detector technology and modern electronics enable us to improve on the previous generation gamma-ray telescope by well more than an order of magnitude in sensitivity.  The LAT tracker design uses well-established detector technology but has solved a number of engineering problems related to putting a 900,000 channel silicon-strip system in orbit:  Highly reliable SSD design for mass production  Very low power fault-tolerant electronics readout  Rigid, low-mass structure with passive cooling  Compact electronics packaging with minimal dead area  We have validated the design concepts with several prototype cycles and are now approaching the manufacturing stage.  We’re looking forward to a 2006 launch and a decade of exciting GLAST science!