GLAST LAT SLAC DoE Review June 13, 2007 R.Dubois1 GLAST Large Area Telescope: Science Analysis Systems and Collaboration Computing Needs Robert Cameron,

Slides:



Advertisements
Similar presentations
GLAST Science Support CenterAugust 9, 2004 Overview of Analyzing GLAST Data David Band (GLAST SSC—GSFC/UMBC)
Advertisements

Operations Testing in the ISOC Service Challenges are a successor and extension to the successful Data Challenge model Broader set of objectives Continue.
Experiences From The Fermi Data Archive Dr. Thomas Stephens Wyle IS/Fermi Science Support Center.
GLAST LAT ProjectManager’s Face to Face - ISOC, 17 March GLAST Large Area Telescope WBS 4.1.B Instrument Science Operations Center Manager’s Face.
GLAST LAT ProjectDOE/NASA Review of the GLAST/LAT Project, Feb , 2001 IOC – S.Williams SAS - R.Dubois 1 Instrument Operations Center (IOC) and Science.
GLAST LAT ProjectISOC CDR, 4 August 2004 Document: LAT-PR-04500Section 3.31 GLAST Large Area Telescope: Instrument Science Operations Center CDR Section.
GLAST LAT ProjectISOC CDR, 4 August 2004 Document: LAT-PR-04500Section 3.11 GLAST Large Area Telescope: Instrument Science Operations Center CDR Section.
GLAST LAT ISOCMonthly Status Review - ISOC, 1 August GLAST Large Area Telescope Instrument Science Operations Center Monthly Status Review 1 August.
GLAST Large Area Telescope - OperationsDOE Review, 15 June GLAST Large Area Telescope Operations Review Rob Cameron Instrument Science Operations.
GLAST LAT ProjectISOC Peer Review - March 2, 2004 Document: LAT-PR Section 2.1 Requirements 1 Gamma-ray Large Area Space Telescope GLAST Large.
GLAST LAT Project 1S. Ritz Discussion: To Where From Here? DC2 Closeout Meeting 2 June, 2006 S. Ritz Gamma-ray Large Area Space Telescope.
GLAST LAT Project 1S. Ritz Discussion: To Where From Here? DC1 Closeout Meeting February 13, 2004 S. Ritz Gamma-ray Large Area Space Telescope.
GLAST LAT ProjectDC1 Closeout Workshop, Feb , Post-DC1 Work Seth Digel (HEPL/Stanford Univ.) Post-DC1 Work.
GLAST LAT Project ISOC Peer Review - March 2, 2004 Document: LAT-PR Section 2.3 Verification and Validation 1 Gamma-ray Large Area Space Telescope.
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.
Section 15-1GLAST Ground System Design Review August 18&19, 2004 ISOC Organization ISOC Manager R Cameron Commanding, H&S Timeline Planning Command Generation.
GLAST LAT ProjectISOC CDR, 4 August 2004 Document: LAT-PR-04500Section 4.11 GLAST Large Area Telescope: Instrument Science Operations Center CDR Section.
The CU Beam Test at CERN Status Report and highlights from workshop II Luca Latronico LAT C&A Meeting May
GLAST LAT Project ISOC Peer Review - March 2, 2004 Section Gamma-ray Large Area Space Telescope GLAST Large Area Telescope ISOC Peer Review 7.2.
GLAST LAT ProjectISOC CDR, 4 August 2004 Document: LAT-PR-04500Section 21 GLAST Large Area Telescope: Instrument Science Operations Center CDR Section.
GLAST ADASS London Sept, 2007 R.Dubois1/24 GLAST Large Area Telescope: A Fusion of HEP and Astro Computing Richard Dubois Stanford Linear Accelerator Center.
GLAST LAT Project 1S. Ritz DC1 Closeout Introduction February 2004 Steven Ritz Gamma-ray Large Area Space Telescope.
GLAST LAT Project LAT Monthly Apr SAS 1 Gamma-ray Large Area Space Telescope GLAST Large Area Telescope WBS 4.1.D SAS LAT Monthly Managerfest.
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?)
GLAST LAT ProjectOnline Peer Review – July 21, Integration and Test L. Miller 1 GLAST Large Area Telescope: I&T Integration Readiness Review.
R.Dubois Sim/Recon Overview 1/10 GLAST LAT ProjectSoftware Workshop July, SLAC Sim/Recon Overview Elements of Simulation/Reconstruction Development,
Hall D Online Data Acquisition CEBAF provides us with a tremendous scientific opportunity for understanding one of the fundamental forces of nature. 75.
October 24, 2000Milestones, Funding of USCMS S&C Matthias Kasemann1 US CMS Software and Computing Milestones and Funding Profiles Matthias Kasemann Fermilab.
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.
GLAST LAT ProjectDOE/NASA Baseline-Preliminary Design Review, January 8, 2002 K.Young 1 LAT Data Processing Facility Automatically process Level 0 data.
IXYZ Frank Marshall NASA/GSFC 25 April 2012 April 25, 20121Implementing Portals of the Universe.
Implementing a dual readout calorimeter in SLIC and testing Geant4 Physics Hans Wenzel Fermilab Friday, 2 nd October 2009 ALCPG 2009.
The GLAST Science Support Center’s Role in Supporting the User Community [24.10] Thomas E. Stephens (GSFC/L-3GSI) for the GLAST Science Support Center.
Julie McEnery1 Data Challenge II Logo by Stefano Ciprini.
GLAST LAT ProjectFace to Face Managers Meeting 04/14/ Integration and Test 1 GLAST Large Area Telescope: I & T Input to Face to Face Managers.
1 Japan-US collaboration to develop the “End-to-End simulator” Tsunefumi Mizuno Mar 12, 2003.
Heather Kelly PPA Scientific Computing Apps LAT was launched as part of the Fermi Gamma-ray Space Telescope on June 11 th 2008.
Serving Data to the GLAST User Community Don Horner (L3 GSI/GSFC) and the GLAST Science Support Center Team Data Properties and Impact on Data Serving.
Source catalog generation Aim: Build the LAT source catalog (1, 3, 5 years) Jean Ballet, CEA SaclayGSFC, 29 June 2005 Four main functions: Find unknown.
ESAC_3_24_05.ppt 1 GLAST Large Area Telescope Overview and Science Update Peter F. Michelson Stanford University GLAST User’s Committee.
GLAST Science Support Center June 21, 2007 Getting Involved with GLAST GLAST Guest Investigator Program David Band, GSSC CRESST/GSFC/UMBC.
GLAST LAT Project 1S. Ritz Data Challenge Planning Overview Purpose Boundary conditions Plan: –scope and progression of data challenges –schedule summary.
1 Getting Involved with GLAST Workshop, CFA, 06/21/ C. Shrader, NASA/GSFC GLAST Data & Software Release plans + Science Support Center Services C.
GLAST Large Area Telescope – ISOC Overview and StatusDOE Annual Review, 13 June GLAST Large Area Telescope Instrument Science Operations Center.
GLAST LAT Project DC2 Software Workshop, GSFC, June 27-29, Analytical Objectives for Science Tools for DC2 for DC2 S. W. Digel Stanford Linear Accelerator.
June 27-29, DC2 Software Workshop - 1 Tom Stephens GSSC Database Programmer GSSC Data Servers for DC2.
GLAST Science Support Center May 8, 2006 GUC Meeting AI#28. SAE Release Schedule David Band (GSSC/JCA-UMBC) Julie McEnery (GSFC)
GLAST Science Support Center November 8, 2005 GUC Action Item #15 AI#15: Pre-Launch GI Proposal Tools David Band (GSSC/JCA-UMBC)
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.
Source catalog generation Aim: Build the LAT source catalog (1, 3, 5 years) Jean Ballet, CEA SaclaySLAC, 23 May 2005 Four main functions: Find unknown.
The GLAST Science Support Center
GLAST Large Area Telescope Instrument Science Operations Center
GLAST Large Area Telescope:
“Running Monte Carlo for the Fermi Telescope using the SLAC farm”
GLAST Large Area Telescope
Lessons Learned: The Organizers
Prospects for Observations of Microquasars with GLAST LAT
Proposal for LAT Year 1 Data Release Plan
GLAST Large Area Telescope Instrument Science Operations Center
GLAST Large Area Telescope
LAT Data Server Serve what?
GLAST Large Area Telescope
GLAST Large Area Telescope
Data Challenge 2: Aims and Status
LAT Instrument Operations Center
Data Challenge 1 Closeout Lessons Learned Already
Status Report and highlights from workshop II
Level 1 Processing Pipeline
GLAST Large Area Telescope Instrument Science Operations Center
Presentation transcript:

GLAST LAT SLAC DoE Review June 13, 2007 R.Dubois1 GLAST Large Area Telescope: Science Analysis Systems and Collaboration Computing Needs Robert Cameron, Richard Dubois Stanford Linear Accelerator Center Gamma-ray Large Area Space Telescope

GLAST LAT SLAC DoE Review June 13, 2007 R.Dubois2 Outline SAS Overview Service Challenge update –Support for LAT Collaboration Science Groups –Support for ISOC Operations Testing Computing Resource Projections

GLAST LAT SLAC DoE Review June 13, 2007 R.Dubois3 SAS: Fusion of HEP & Astro 1 Gev Gamma Incident Gamma e-e- e+e+ Radiated Gammas Note energy flow in direction of incident Gamma ~8.5 Radiation Lengths Full simulation/reconstruction of 1 GeV gamma Event Interpretation “Science Tools” Collection of tools for detection and characterization of gamma-ray sources (point sources and extended sources) source finding max likelihood fitting (binned/unbinned) parameterized instrument response exposure maps comparisons to model (observation sim) periodicity searches, light curves Science Tools are FITS/FTOOLS based for dissemination to astro community + full code development environment on linux, windows (mac imminent), code and data distribution, automated code builds, documentation etc etc

GLAST LAT SLAC DoE Review June 13, 2007 R.Dubois4 Data Challenges A progression of data challenges. –DC1 in simulated week all-sky survey simulation. find the sources, including GRBs a few physics surprises –DC2 in 2006, completed in June. 55 simulated days (1 orbit precession period) of all-sky survey. First generation of LAT source catalogue Added source variability (AGN flares, pulsars). lightcurves and spectral studies. correlations with other wavelengths. add GBM. study detection algorithms. benchmark data processing/volumes/reliability. 200k batch jobs - worked out reliability issues (< 0.1% failure rate now) Data challenges provided excellent testbeds for science analysis software. Full observation, instrument, and data processing simulation. Team uses data and tools to find the science. “Truth” revealed at the end.

GLAST LAT SLAC DoE Review June 13, 2007 R.Dubois5 Post DC: Service Challenge Coordinate simulation studies –will need a common set of simulations plus a near-constant stream of simulations to support special studies. Develop capabilities outside SLAC as needed using collaboration resources. Operations readiness testing coordinated with the mission- level End-To-End tests. –leverage off the ETE tests for internal-to-LAT readiness –a sequence of “service challenges” for readiness testing serves these needs better than what is needed for systematic studies by science topic. Organize by area –Science groups, led by LAT Analysis Coordinator –ISOC, led by ISOC managers

GLAST LAT SLAC DoE Review June 13, 2007 R.Dubois6 SC Work to be Done: Responsibilities Systematic & Sensitivity Studies –pt sources, extended sources, transients; upper limits –diffuse analyses –variability (incl. pulsars) –neighboring sources –flaring & diffuse effects –focus on 1st papers analyses Operations Readiness Tests –digital data problems –instrument problems (bad channels, wrong rates, recognizing a few wrong constants, …) –Automated science processing –receiving data dumps, running the pipeline, benchmarking resources and times, reliability –idiosyncrasies vs. problems –day(s) in the life –performance monitoring –documentation Other Studies –PSR (“handoff review”) performance –analysis tuning (signal/bkgd, quality knobs by topic) –update simulation (s/c model, tune from beam test and IA data…) –first light observations (simulate point, then scan); early ops analyses –effects of burst repoints –sky survey strategy checks –background fluxes evaluation early ops Analysis Coordinator and Science groups ISOC C&A group and ISOC jointly Collaboration participation needed

GLAST LAT SLAC DoE Review June 13, 2007 R.Dubois7 SC: Connection to Science Groups Several datasets have been identified for the Science Groups use: –1 year survey simulation, using obssim science tool (completed) Fast Monte-Carlo with parameterized responses and efficiencies Early testing of sky model; opportunity for Science Groups to exercise analyses on realistic sky with long observations –55 day simulation using GLEAM (LAT event simulator) (imminent!) Full simulation Earth occultation not currently in exposure calculations Autonomous Repoint Requests LAT/SC misalignment Background interleave for pointed observations –1 year GLEAM simulation Final pre-launch science performance Potentially huge backgrounds run needed Targeting use of Lyon, Italian computer farms –Plus a few smaller scale specialty runs as needed Plan on delivering obssim and 55 day runs for the end-July LAT collaboration meeting; 1 yr Gleam run in August. –Milestone for next versions of Data Catalogue, LAT Data Servers

GLAST LAT SLAC DoE Review June 13, 2007 R.Dubois8 SC: Operations Testing for the ISOC Strategy defined from ISOC Science Operations and Service Challenge workshop –Use ETE tests for control room type functions Shift log, Level1 pipeline, Data Catalogue, Monitoring –SAS products –Use simulations to prep for ETE & provide realistic science data, extended running Simulate Level0 science data –Prep for ETE Level1 pipeline usage –Realistic science data for response distributions, resource usage, latencies etc –Downlink simulations for instrument readiness tests, such as calibrations, failed sensors etc. –Demonstrated, but need background interleave scheme for big datasets 55 day, 1 year orbit runs –Extended run to test Automated Science Processing –Time trending of instrument quantities

GLAST LAT SLAC DoE Review June 13, 2007 R.Dubois9 Simplified Diagram for ISOC Data Flow Merge Events Extract Context Extract EBF MOC FastCopy L0 Archive Ingest L0 data Create digi files Analyze charge injection data (LCI) Create recon files and perform event classification Analyze calibration data (LPA) MOOD/MOOT (config DB) Get Calibration from DB Create data analysis ntuples Automated Science Processing Data Receiving Calibrations and L1 processing Output Data Products to LAT Collaboration and GSSC S S S S S S S S S S - testable with simulations

GLAST LAT SLAC DoE Review June 13, 2007 R.Dubois10 Data Access: LAT Data Portal Provide collaboration access to both summary “photon” data and full digi/recon/(MC) data –Provide data in both FITS and Root format Main components –Astro Data Server select events based on position in the sky, energy, time, or event class –Data Skimmer Select events based on “TCut” able to access full merit tuple (400+ columns) Access full data for list of runs/events –Event Display (WIRED) View detailed detector response for list of runs/events –Data Catalogue is underpinning with all the dataset bookkeeping File locations Flexible user definable meta data Under revision for the 55 day run

GLAST LAT SLAC DoE Review June 13, 2007 R.Dubois11 Current Computing Resources at SLAC Starting 3 rd year of projected annual $300k Capital Equipment Projects –Supplying batch farm disk & CPU, as well as dedicated servers –Optimize purchases based on best deals SCCS can come up with 150 TB disk (45 TB still available) –LAT Commissioning –DC2/SC –LAT Beamtest –Infrastructure needs (code builds; system tests; user disk) Tremendous use of SLAC Batch farm –160 cores (40 dual core, dual CPU boxes) owned by GLAST Leveraged to > 300 cores during extended simulations runs –Will have 400 cores at SLAC Not looking good for quad core CPUs to be available this year

GLAST LAT SLAC DoE Review June 13, 2007 R.Dubois12 Known Liens on Resources GLAST/LAT Data taking at General Dynamics –EMI/EMC testing is underway for 30 days –Thermal-vacuum testing in late summer, ~40 days 55 Day run –One week processing time; 5 TB disk Service Challenge 1-year run in August –40 days 300+ cores –~30 TB disk (Note: disk space needs are reduced compared to on-orbit data taking due to use of background interleave scheme) ETEs –Small data volumes on this scale Launch –Estimate ~100 cores needed to process a 3-hour downlinked dataset in about an hour –400 cores will provide a pool of cores for prompt processing & monitoring; reprocessing; and simulations –Will order 150 TB disk to be on hand at launch

GLAST LAT SLAC DoE Review June 13, 2007 R.Dubois13 Computing: Planned Acquisitions SLAC –Order for 50 TB disk and 240 cores in process –ship date is end June (from Sun); to be installed mid July –Additional 150 TB to be acquired for launch readiness –Funds from SLAC & LAT Operations Collaboration Fund Univ of Washington (in use now) –~100 physics dept lab CPUs on cycle-available basis (when students are not using them) –Used for CPU intensive simulations Lyon –IN2P3 is providing 100 CPUs, 50 TB disk porting LAT processing pipeline infrastructure (Pipeline2) to Lyon now CNAF –INFN has submitted proposal for 100 CPUs, 25 TB (in 07) Approved –Will be required to access via GRID tools

GLAST LAT SLAC DoE Review June 13, 2007 R.Dubois14 What to Take Away Service Challenge + End-To-End tests –Being used to hone the tools, complete development and test end- to-end operations Computing resources: prudent approach is being implemented –Acquire ~400 cores at SLAC available for GLAST Lesson learned from 5-ring circus of DC2, LAT Beam Test, I&T –Keep full event details on disk in ‘08 : ~175 TB –GLAST will do better science the more compute power it has access to Have not hit the plateau yet! Extending LAT processing pipeline to France and Italy