Mini Tower Preliminary Results

Slides:



Advertisements
Similar presentations
GLAST The GLAST Balloon Flight experiment was performed with the collaboration of NASA Goddard Space Flight Center, Stanford Linear Accelerator Center,
Advertisements

Status of DHCAL Slice Test Data Analysis Lei Xia ANL-HEP All results preliminary.
GLAST LAT Project I&T Meeting – Jan 20,2004 E. do Couto e Silva 1 GLAST Large Area Telescope: EM1 Data Analysis and Calibration Summary Report Eduardo.
GLAST LAT ProjectISOC CDR, 4 August 2004 Document: LAT-PR-04500Section 3.31 GLAST Large Area Telescope: Instrument Science Operations Center CDR Section.
SVAC/ISOCInstrument Analysis Meeting, April 14, 2006 Anders W. Borgland 1 The LAT In Every Which Way You Want It! Anders W. Borgland Science Verification,
GLAST LAT ProjectIA Workshop 6 – Feb28,2006 Preliminary Studies on the dependence of Arrival Time distributions in the LAT using CAL Low Energy Trigger.
GLAST LAT Project11/18/04 I&T Two Tower IRR 1 GLAST Large Area Telescope: Integration and Test Two Tower Integration Readiness Review Particle Test Elliott.
A.Chekhtman1 GLAST LAT ProjectCalibration and Analysis group meeting, April, 3, 2006 CAL on-orbit calibration with protons. Alexandre Chekhtman NRL/GMU.
GLAST LAT Project 1 Tracker “mini-tower” Full Size Calorimeter module Face to Face IDT meeting March 20, 2002 Convener: E. do Couto e Silva Engineering.
The performance of LHCf calorimeter was tested at CERN SPS in For electron of GeV, the energy resolution is < 5% and the position resolution.
GLAST LAT Project Instrument Analysis Workshop June 7, 2004 E. do Couto e Silva 1/19 Introduction to the Workshop Series Eduardo do Couto e Silva Instrument.
GLAST LAT Project LAT Instrument Analysis Meeting – May 26, 2006 Hiro Tajima, TKR Efficiency Trending 1 GLAST Large Area Telescope: TKR Efficiency Trending.
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 Project Software vrvs meeting X. Chen 1 GLAST LAT Project Software vrvs meeting X. Chen 1 Analyses of Muon Calibration Data Xin Chen.
GLAST LAT ProjectIA Workshop 6 – Feb28,2006 E. do Couto e Silva 1 Final Data Taking with SLAC (Data for Instrument Analysis Workshop 7) Eduardo do.
GLAST LAT Project Analysis Meeting March 22, 2004 E. do Couto e Silva 1/8 LAT Instrument Test Analysis Eduardo do Couto e Silva March 23, 2004.
GLAST LAT Project11/18/04 I&T Two Tower IRR 1 GLAST Large Area Telescope: Integration and Test Two Tower Integration Readiness Review Particle Test Gary.
IA meeting, Feb. 3, 2006 Mutsumi Sugizaki TKR Noise Stdudy 1 LAT TKR Noise Study Current Status Mutusmi Sugizaki (and short comment about TOT=255 event)
GLAST LAT ProjectTest Planning Meeting Aug 2, 2004 E. do Couto e Silva 1/6 SVAC EM2 Goals Develop distributions for E2E tests that involve comparison of.
GLAST LAT Project ISOC Peer Review - March 2, 2004 Document: LAT-PR Section 7.1 Pre-launch Operation and Calibration 1 Gamma-ray Large Area Space.
In order to acquire the full physics potential of the LHC, the ATLAS electromagnetic calorimeter must be able to efficiently identify photons and electrons.
GLAST LAT Project SE Test Planning meeting October 4, 2004 E. do Couto e Silva 1/13 SVAC Data Taking during LAT SLAC Oct 4, 2004 Eduardo.
GLAST LAT ProjectDOE/NASA Status Review, March 30 & 31, 2004 Integration and Test 1 Integration, Facilities, Configuration, and Test (IFCT) Flow Procedure.
30 Ge & Si Crystals Arranged in verticals stacks of 6 called “towers” Shielding composed of lead, poly, and a muon veto not described. 7.6 cm diameter.
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.
GLAST LAT ProjectI&T&C Pre PDR, October 2, 2001 E. do Couto e Silva1 I&T&C Organization Chart I&T&C Manager Elliott Bloom WBS I&T Engineer B. Grist.
Preliminary analysis of p-Pb data update n. 6 Lorenzo Bonechi LHCf Catania meeting – 19 December 2013.
Geant4 simulation for Balloon Flight Jan. 16, 2001 Software Workshop at SLAC Tsunefumi Mizuno.
GLAST LAT Project LAT Instrument Analysis Workshop – Feb 27, 2006 Hiro Tajima, TKR Data Processing Overview 1 GLAST Large Area Telescope: TKR Data Processing.
1 Stepping in everyone’s toes ( but for a good cause….) Eduardo do Couto e Silva Software Meeting – January 2001.
Feb. 7, 2007First GLAST symposium1 Measuring the PSF and the energy resolution with the GLAST-LAT Calibration Unit Ph. Bruel on behalf of the beam test.
Aa GLAST Particle Astrophysics Collaboration Instrument Managed and Integrated at SLAC/Stanford University The Gamma-ray Large Area Space Telescope (GLAST)
All Experimenters MeetingDmitri Denisov Week of July 7 to July 15 Summary  Delivered luminosity and operating efficiency u Delivered: 1.4pb -1 u Recorded:
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,
All Experimenters MeetingDmitri Denisov Week of September 9 to September 16 D0 Summary  Delivered luminosity and operating efficiency u Delivered: 4.0pb.
GLAST LAT Project CU Beam Test Workshop 3/20/2006 C. Sgro’, L. Baldini, J. Bregeon1 Glast LAT Calibration Unit Beam Test Status Report on Online Monitor.
The Detector Performance Study for the Barrel Section of the ATLAS Semiconductor Tracker (SCT) with Cosmic Rays Yoshikazu Nagai (Univ. of Tsukuba) For.
LHCf Detectors Sampling Calorimeter W 44 r.l, 1.6λ I Scintilator x 16 Layers Position Detector Scifi x 4 (Arm#1) Scilicon Tracker x 4(Arm#2) Detector size.
1 Study of Data from the GLAST Balloon Prototype Based on a Geant4 Simulator Tsunefumi Mizuno February 22, Geant4 Work Shop The GLAST Satellite.
Feb. 3, 2007IFC meeting1 Beam test report Ph. Bruel on behalf of the beam test working group Gamma-ray Large Area Space Telescope.
A New Upper Limit for the Tau-Neutrino Magnetic Moment Reinhard Schwienhorst      ee ee
QWG Sept 20-22, Jundong Huang Indiana University 1 DØ Quarkonium Production at DØ Jundong Huang Indiana University Quarkonium Workshop FermiLab September.
1 Methods of PSD energy calibration. 2 Dependence of energy resolution on many factors Constant term is essential only for energy measurement of single.
GLAST LAT ProjectNovember 18, 2004 I&T Two Tower IRR 1 GLAST Large Area Telescope: Integration and Test Two Tower Integration Readiness Review SVAC Elliott.
EPS HEP 2007 Manchester -- Thilo Pauly July The ATLAS Level-1 Trigger Overview and Status Report including Cosmic-Ray Commissioning Thilo.
GLAST LAT Project SE Test Planning Dec 7, 2004 E. do Couto e Silva 1/27 Trigger and SVAC Tests During LAT integration Su Dong, Eduardo do Couto e Silva.
Mini-Tower test results
DAMPE: first data from space
Comparison of GAMMA-400 and Fermi-LAT telescopes
The Status of the Data Analysis of the Beam Test at FZJ
GLAST LAT tracker signal simulation and trigger timing study
GLAST Large Area Telescope:
Gamma-ray Large Area Space Telescope
GLAST Large Area Telescope Instrument Science Operations Center
The Silicon Track Trigger (STT) at DØ
Instrument Analysis Workshop Series
Overview Goal Study GEM variables in SVAC ntuple
Imaging crystals with TKR
Beam Dump Experiments with Photon and Electron Beams
GEANT Simulations and Track Reconstruction
MAP 2014 Spring Workshop Fermilab May, 2014
CR Photon Working Group
Integration and Test Organization Chart
Eduardo do Couto e Silva Feb 28, 2006
Studies of the Time over Threshold
Analysis of GLAST Balloon Experiment Data
Problems in π0 Reconstruction
Overview of Beam Test Benoit, Ronaldo and Eduardo Nov 8 , 2005 thanks to Steve and Bill for helping to consolidate all the information.
Presentation transcript:

Mini Tower Preliminary Results Xin Chen and Eduardo do Couto e Silva July 14 , 2003 Ground Software Workshop

Minitower Test All results are PRELIMINARY These data are not intended for MC validation but to debug the data analysis chain and to study the experimental set-up

The Minitower Geometry LAT-TD-00582-02 Maintained by X. Chen 3% W GTFE Si layer GTRC F G Y3 X3 X2 Y2 Y1 X1 X0 Y0 V3 V5 no silicon detectors no silicon detectors There are 8 layers instrumented with Front-End Electronics (MCMs) but only 6 layers instrumented with silicon detectors

Data Taking Configurations Cosmic Rays Cosmic Rays minitower minitower 17.6 MeV g Vertical position Expected CR trigger rate 13 Hz Horizontal position Expected CR trigger rate ~ 4 Hz Expected g trigger rate ~ 0.02 Hz

The Experimental Setup minitower BGO crystals Cosmic ray telescope VDG beam pipe EGSE (VME crate)

Position VDG pipe at negative X and Y coordinates The Coordinate System X Based on position of disabled or dead channels in every layer, this region (~1/8 of minitower active area) is expected to have the highest trigger efficiency Y Z Position VDG pipe at negative X and Y coordinates

Event rates – TKR trigger Run ID Run type DATA Trigger rate (Hz) MC Reconstructed rate MC Reconstructed rate 030613022805 Muons with vertical tracker ~ 0.94 ~ 0.83 ~0.88 ~ 0.74 030604013515 Muons with horizontal tracker ~ 0.42 ~ 0.38 ~ 0.36 ~ 0.33 There is reasonable agreement between MC and DATA since we assume about 20% uncertainty in the MC rates due to the knowledge of the flux.

Strip Map Y layers X layers This layer with about 300 “live” strips, strongly constraints the parameter space available for triggering

Muons with vertical tracker – TKR trigger only Hit Multiplicity Normalized rates in Hz DATA MC

Muons with vertical tracker – TKR trigger only TOT in each layer Normalized rates in Hz DATA MC

Muons with vertical tracker – TKR trigger only Track multiplicity Normalized rates in Hz

Dead Channel list from DATA is used as input for MC Muons with vertical tracker Dead Channel list from DATA is used as input for MC Reconstructed direction DATA MC X X Y Y Z Z

Dead Channel list from DATA is used as input for MC Muons with vertical tracker Dead Channel list from DATA is used as input for MC MC Reconstructed direction DATA X X Y Y Z Z

Dead Channel list from DATA is used as input for MC Muons with horizontal tracker Dead Channel list from DATA is used as input for MC MC Reconstructed direction DATA X X Y Y Z Z

Dead Channel list from DATA is used as input for MC Muons with horizontal tracker X Z Dead Channel list from DATA is used as input for MC MC Reconstructed Position DATA X X Y Y Z Z

VDG DATA Taking Mode P + Li ---> Be ---> Be + gamma ( 66% 17.6 MeV, 33% 14.6 MeV ) Experiment x Mini tower Pb shield z proton Li target MC Simulation photons Only the Pb shield is implemented in the simulation

Photons + Muons with horizontal tracker MC (photons only) Reconstructed Direction DATA (photons + muons) X X Y Y Z Z

Photons + Muons with horizontal tracker MC (photons only) DATA (photons + muons) Reconstructed Position X X Y Y Z Z

measured spectrum with BGO crystals VDG Calibration Minitower : ebf0306040204959 46002 events 8158 s Rate 5.6 Hz BGO crystals : VG13.dat 46907 events 6160 s Rate 7.6 Hz calculated spectrum Used the BGO and estimate the photon rate in the minitower to be 5.7 Hz ± 30% (preliminary) measured spectrum with BGO crystals G. Godfrey Energy (MeV) cosmics

Signal + Background (1) (mm) (mm) VDG g signal + C.R. background ~ 2 hours of data taking Trigger rate VDG + C.R. ~ 5.6 Hz C.R. ~ 0.5 Hz Cosmic ray background (mm) (mm) We understand the coordinate system of our set-up since both X and Y reconstructed positions are negative 58% of triggered signal + background events were reconstructed 81% of triggered cosmic ray background events were reconstructed The VDG provides valuable DATA to study reconstruction efficiencies of photons

Photons impinging on top face of minitower Signal + Background (2) VDG g signal + C.R. background Y m Z g Cosmic ray background cos(q) Photons impinging on top face of minitower

Photon candidate Y Z View X Z View Reconstructed photon direction Top of minitower Top of minitower Reconstructed photon direction Y Z View X Z View

Plans Continue to look at these data until the next hardware (TKR+CAL) is delivered (mid to end of August) Analyzing the TKR data at different detector thresholds Studying possible time effects The focus now is to develop all the online and offline infrastructure necessary for the next mini tower tests