1 Japan-US collaboration to develop the “End-to-End simulator” Tsunefumi Mizuno Mar 12, 2003.

Slides:



Advertisements
Similar presentations
The MAGIC telescope and the GLAST satellite La Palma, Roque de los Muchacos (28.8° latitude ° longitude, 2225 m asl) INAUGURATION: 10/10/2003 LAT.
Advertisements

GLAST The GLAST Balloon Flight experiment was performed with the collaboration of NASA Goddard Space Flight Center, Stanford Linear Accelerator Center,
Gamma-ray Mapping of the Interstellar Medium and Cosmic Rays in the Galactic Plane with GLAST Yasushi Fukazawa 1, T. Kamae 1,2, T. Ohsugi 1, T. Mizuno.
FMOS Observations and Data 14 January 2004 FMOS Science Workshop.
O. Stézowski IPN Lyon AGATA Week September 2003 Legnaro Data Analysis – Team #3 ROOT as a framework for AGATA.
GLAST Large Area Telescope - OperationsDOE Review, 15 June GLAST Large Area Telescope Operations Review Rob Cameron Instrument Science Operations.
CHANDRA X-RAY OBSERVATORY The Universe in a Whole New Light Kim Arcand Visualization Coordinator X-ray Data in a Digital Environment.
GLAST LAT ProjectDC1 Closeout Workshop, Feb , Post-DC1 Work Seth Digel (HEPL/Stanford Univ.) Post-DC1 Work.
GLAST LAT ProjectISOC CDR, 4 August 2004 Document: LAT-PR-04500Section 4.11 GLAST Large Area Telescope: Instrument Science Operations Center CDR Section.
Eduardo do Couto e Silva - ATC/LM Colloquium, June How many neutralinos are there? Expansion of universe Depletion of neutralinos Creation of neutralinos.
Advanced Technology Center 1 HMI Rasmus Larsen / Processing Modules Stanford University HMI Team Meeting – May 2003 Processing Module Development Rasmus.
GLAST Telescope Network Archiving System Tim Graves Gordon Spear Lynn Cominsky SSU EPO Team.
GLAST LAT Project 1S. Ritz Purposes of the Data Challenges “End-to-end” testing of analysis software. –define the ends –define the tests (what is success?)
IFTSUV: an Imaging Fourier Transform Spectrometer in the UV Anne Millard, 3 rd year PhD student, directed by P. Lemaire and J.-C. Vial.
SLAC March 1 st 2006 GLAST LAT Software F.Longo GLAST LAT GLAST LAT SW Overview of Cookbook Examples Francesco Longo University and INFN, Trieste, Italy.
Status of MC Simulation Huaimin Liu BESIII Collaboration meeting IHEP, Beijing, Jan. 12, 2006.
Shuei MEG review meeting, 2 July MEG Software Status MEG Software Group Framework Large Prototype software updates Database ROME Monte Carlo.
Characterisation Data Model applied to simulated data Mireille Louys, CDS and LSIIT Strasbourg.
At A Glance VOLT is a freeware, platform independent tool set that coordinates cross-mission observation planning and scheduling among one or more space.
10/20/2005 GLAST Lunch Seminar Deconvolution of ASCA Images1 Deconvolution of ASCA Images of Galaxy Clusters and SNRs Mutsumi Sugizaki, Tune Kamae SLAC.
HPS Online Software Discussion Jeremy McCormick, SLAC Status and Plans.
Gamma-Ray Telescopes. Brief History of Gamma Ray Astronomy 1961 EXPLORER-II: First detection of high-energy  -rays from space 1967 VELA satelllites:
Scheduling Blocks: a generic description Andy Biggs (ESO, Garching)
GLAST Geant4 Simulation Francesco Longo University of Trieste and INFN-Trieste On the behalf of the GLAST Software Group Udine 30/01/03.
CBM Software Workshop for Future Challenges in Tracking and Trigger Concepts, GSI, 9 June 2010 Volker Friese.
November 2013 Review Talks Morning Plenary Talk – CLAS12 Software Overview and Progress ( ) Current Status with Emphasis on Past Year’s Progress:
Detector Simulation Presentation # 3 Nafisa Tasneem CHEP,KNU  How to do HEP experiment  What is detector simulation?
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.
The CMS Simulation Software Julia Yarba, Fermilab on behalf of CMS Collaboration 22 m long, 15 m in diameter Over a million geometrical volumes Many complex.
Aa GLAST Particle Astrophysics Collaboration Instrument Managed and Integrated at SLAC/Stanford University The Gamma-ray Large Area Space Telescope (GLAST)
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,
Monte Carlo Simulation Study of In-orbit Background for the Soft Gamma-ray Detector onboard ASTRO-H Mizuno T., Hiragi K., Fukazawa Y., Umeki Y. (Hiroshima.
August 2003 At A Glance The IRC is a platform independent, extensible, and adaptive framework that provides robust, interactive, and distributed control.
Why A Software Review? Now have experience of real data and first major analysis results –What have we learned? –How should that change what we do next.
Jean-Roch Vlimant, CERN Physics Performance and Dataset Project Physics Data & MC Validation Group McM : The Evolution of PREP. The CMS tool for Monte-Carlo.
April , 2006 HEASARC Users Group Tom McGlynn The HEASARC On-line Services Tom McGlynn.
Progress report of the GLAST ACD Beam Test at CERN (Backsplash study) simulation and analysis Tsunefumi Mizuno, Hirofumi Mizushima (Hiroshima Univ.) and.
Comparison between BFEM data and G4 simulation October 18, 2001 Balloon Analysis VRVS meeting T. Mizuno, H. Mizushima, Y. Fukazawa, and T. Kamae
1 Getting Involved with GLAST Workshop, CFA, 06/21/ C. Shrader, NASA/GSFC GLAST Data & Software Release plans + Science Support Center Services C.
In high energy astrophysics observations, it is crucial to reduce the background effectively to achieve a high sensitivity, for the source intensity is.
HIFI Tutorial 1: Running the HIFI Pipelines and Adaptations A.P.Marston ESAC 27 June 2013.
Overview of PHENIX Muon Tracker Data Analysis PHENIX Muon Tracker Muon Tracker Software Muon Tracker Database Muon Event Display Performance Muon Reconstruction.
GLAST Science Support Center July 16, July Ground Software Workshop The Spacecraft Simulator David S. Davis, GSSC.
1 Study of Data from the GLAST Balloon Prototype Based on a Geant4 Simulator Tsunefumi Mizuno February 22, Geant4 Work Shop The GLAST Satellite.
Fermi Gamma-ray Space Telescope Searches for Dark Matter Signals Workshop for Science Writers Introduction S. Ritz UCSC Physics Dept. and SCIPP On behalf.
Feb. 3, 2007IFC meeting1 Beam test report Ph. Bruel on behalf of the beam test working group Gamma-ray Large Area Space Telescope.
Origami: Scientific Distributed Workflow in McIDAS-V Maciek Smuga-Otto, Bruce Flynn (also Bob Knuteson, Ray Garcia) SSEC.
PoGOLiteMC_ ppt 1 Updated MC Study of PoGOLite Trigger Rate/BG January 30, 2007 Tsunefumi Mizuno (Hiroshima Univ.)
+ UVIS Data Visualization UVIS Team Meeting Braunschweig, Deutschland June 18, 2012.
Massimiliano Razzano, Università di Pisa & INFN Pisa Gamma-ray Pulsar Simulations for the Gamma-ray Large Area Space Telescope (GLAST) Gamma-ray pulsars.
ArgonneResult_ ppt1 Results of PoGO Argonne Beam Test PoGO Collaboration meeting at SLAC, February 7, 2004 Tsunefumi Mizuno
O Tsunefumi Mizuno, Tuneyoshi Kamae, Jonny Ng, Hiroyasu Tajima (SLAC), John W. Mitchell, Robert Streitmatter (NASA GSFC), Richard C. Fernholz, Edward Groth.
1 GlueX Software Oct. 21, 2004 D. Lawrence, JLab.
Report of GLAST Balloon Flight October Annual meeting of Astronomical Society of Japan T. Mizuno and other GLAST Balloon Team
15 May 2012NA61 Collaboration Meeting, Budapest1 Shine: status and plans András László, for the Shine Group.
Towards a CTA high-level science analysis framework
Periodicity Search in X-ray data of RX J
GLAST Large Area Telescope:
The Fermi Mission Liz Hays (NASA GSFC) Fermi Symposium 2017.
Fermi & ASDC Elisabetta Cavazzuti on behalf ASDC Team Fermi Meeting
“Running Monte Carlo for the Fermi Telescope using the SLAC farm”
Prospects for Observations of Microquasars with GLAST LAT
LAT Software Quality Assurance
LHCb Detector Description Framework Radovan Chytracek CERN Switzerland
Simulation and Physics
Mini Tower Preliminary Results
Analysis of GLAST Balloon Experiment Data
LHCb Detector Description Framework Radovan Chytracek CERN Switzerland
Presentation transcript:

1 Japan-US collaboration to develop the “End-to-End simulator” Tsunefumi Mizuno Mar 12, 2003

2 Overview of the “End-to-End simulation” In most past X-ray and gamma ray observatory missions, observations were done in the pointing mode and the instrumental response had rarely been simulated in the temporal axis (e.g., ASCA, Chandra, XMM, and EGRET). Due to its large field of view (~20% of the whole sky) and scanning observational mode, GLAST Large Area Telescope is extremely different in its construction and operation, and requires a thorough simulation in the time axis as well as in the spatial and spectral axes. The simulation framework, called “End-to-End simulation,” is required to have following features. The simulator must run very fast and can simulate the detector response and background dynamically. It has high flexibility; we can change the source generator, detector simulator, digitization, reconstruction, etc. easily and independently.

3 Framework structure Master manager written in python Orbit information location and altitude (cut off rigidity) observation date (solar activity) satellite direction (source position) Calibration information bad channel list energy resolution Source generator Egret 3 rd catalogue Cosmic-ray Detector MC simulator BFEM Simulator EGRET Simulator LAT Simulator Digitization Data formatting Reconstruction Visualization Mapping histogramming data flow

4 Works to do (Mizuno’s thought) BFEM simulator Compare with a stand-alone BFEM simulator and data ->Validate the framework in one position and time and test the performance (speed). EGRET simulator Compare with EGRET Crab data and Beam test data ->Validate G4 simulator Develop the digitizer, formatter and reconstruction program. Compare with EGRET data ->Validate framework in any position and time and re-analyze the EGRET data. LAT simulator Update geometry information. Develop the interface program with XML geometry description -> Update detector geometry automatically. Run simulator in EtoE framework -> Study performance. Develop the digitizer and formatter -> Study the trigger rate, response and background, etc.

5 Task list and assignment Master manager (H. Tajima and others) Orbital information, coordinate translation (T. Kamae and others) EGRET catalogue generator (done) CR generator (T. Mizuno and others) BFEM simulator (done) EGRET simulator (to be assigned) LAT simulator (to be assigned) Digitizer/formatter for BFEM (done) Digitizer for EGRET (to be assigned) Digitizer/formatter for LAT (to be assigned) Reconstruction for BFEM/LAT (use the existing program developed by software team) Reconstruction for EGRET (to be assigned) Visualization, GUI interface (T. Kamae, H. Tajima and others)