H. Kornmayer MAGIC-Grid EGEE, Panel discussion, Pisa, 26-10-2005 - 1 Monte Carlo Production for the MAGIC telescope A generic application of EGEE Towards.

Slides:



Advertisements
Similar presentations
M.Martinez IFAE Barcelona ASPERA HIGH ENERGY GAMMA RAYS Working Group 1 Conveners: W.Hofmann and M.Martinez.
Advertisements

Results of MAGIC first observation cycle on Galactic sources Javier Rico for the MAGIC Collaboration Institut de Física d’Altes Energies Barcelona, Spain.
H.E.S.S. Phases I and II Paula Chadwick, Dept. of Physics University of Durham.
Observations of the AGN 1ES with the MAGIC telescope The MAGIC Telescope 1ES Results from the observations Conclusion The MAGIC Telescope.
Introduction to Grids and Grid applications Gergely Sipos MTA SZTAKI
EGEE-III Enabling Grids for E-sciencE EGEE and gLite are registered trademarks Andreas Gellrich, DESY The Grid – The Future of Scientific.
EGEE-II INFSO-RI Enabling Grids for E-sciencE EGEE and gLite are registered trademarks Applications on the EGEE Grid infrastructure.
Jiri Chudoba for the Pierre Auger Collaboration Institute of Physics of the CAS and CESNET.
E-Science Workshop, Santiago de Chile, 23./ KIT ( Frank Schmitz Forschungszentrum Karlsruhe Institut.
Large Magellanic Cloud, 1987 (51.4 kparsec) SN 1987a after before 2006 Hubble.
Dr. Harald Kornmayer A distributed, Grid-based analysis system for the MAGIC telescope, CHEP 2004, Interlaken1 H. Kornmayer, IWR, Forschungszentrum Karlsruhe.
H. Kornmayer MAGIC-GRID Status report EGAAP meeting, Athens, 21th April EnablingGrids for E-sciencE Benefits of the MAGIC Grid Status report of.
Incontri di Fisica delle Alte Energie IFAE 2006 Pavia Vincenzo Vitale Recent Results in Gamma Ray Astronomy with IACTs.
3 rd DPHEP Workshop CERN, 7-8 December 2009 G. LAMANNA CTA C herenkov Telescope Array Giovanni Lamanna LAPP - Laboratoire d'Annecy-le-Vieux de Physique.
Observations of 3C 279 with the MAGIC telescope M.Teshima 1, E.Prandini 2, M.Errando, D. Kranich 4, P.Majumdar 1, M.Mariotti 2 and V.Scalzotto 2 for the.
INFSO-RI Enabling Grids for E-sciencE iASTRO MC MEETING&WORKSHOP, 27-30, APRIL, 2005,SOFIA, BULGARIA Introduction to Grid Technologies.
INFSO-RI Enabling Grids for E-sciencE Geant4 Physics Validation: Use of the GRID Resources Patricia Mendez Lorenzo CERN (IT-GD)
H. Kornmayer MAGIC-GRID Status report EGAAP meeting, Athens, 21th April EnablingGrids for E-siencE Generic Application: Monte Carlo Production.
MAGIC observations of Galactic sources
EGEE is a project funded by the European Union under contract IST Plan for ROC verification Hélène Cordier - Alistair Mills IN2P3, CRNS, France.
F. Goebel, MPI München, 14. June 2004, EGAAP, CERN Florian Goebel Max-Planck-Institut für Physik (Werner-Heisenberg-Institut) München for the MAGIC collaboration.
SouthGrid SouthGrid SouthGrid is a distributed Tier 2 centre, one of four setup in the UK as part of the GridPP project. SouthGrid.
Tier-2  Data Analysis  MC simulation  Import data from Tier-1 and export MC data CMS GRID COMPUTING AT THE SPANISH TIER-1 AND TIER-2 SITES P. Garcia-Abia.
GridPP Deployment & Operations GridPP has built a Computing Grid of more than 5,000 CPUs, with equipment based at many of the particle physics centres.
Bob Jones Technical Director CERN - August 2003 EGEE is proposed as a project to be funded by the European Union under contract IST
Development of Ideas in Ground-based Gamma-ray Astronomy, Status of Field and Scientific Expectations from HESS, VERITAS, MAGIC and CANGAROO Trevor C.
Analysis chain for MAGIC Telescope data Daniel Mazin and Nadia Tonello Max-Planck-Institut für Physik München D.Mazin, N.Tonello MPI for Physics, Munich.
Migration of Monte Carlo Simulation of High Energy Atmospheric Showers to GRID Infrastructure Migration of Monte Carlo Simulation of High Energy Atmospheric.
CTA The next generation ultimate gamma ray observatory M. Teshima Max-Planck-Institute for Physics.
M.Teshima MPI für Physik, München (Werner-Heisenberg-Institut) for MAGIC collaboration MAGIC.
Computing at MAGIC: present and future Javier Rico Institució Catalana de Recerca I Estudis Avançats & Institut de Física d’Altes Energies Barcelona, Spain.
The MAGIC Telescope MAGIC
EGEE-II INFSO-RI Enabling Grids for E-sciencE EGEE and gLite are registered trademarks Large Simulations using EGEE Grid for the.
EGEE-III INFSO-RI Enabling Grids for E-sciencE EGEE and gLite are registered trademarks EGI Operations Tiziana Ferrari EGEE User.
Status Organization Overview of Program of Work Education, Training It’s the People who make it happen & make it Work.
Introduction Data analyzed Analysis method Preliminary results
Highlights of MAGIC results Rome Int. Conf. on Astroparticle Physics – La Sapienza, June 20th 2007 – Denis Bastieri – Univ. & INFN Padova Highlights of.
INFSO-RI Enabling Grids for E-sciencE The EGEE Project Status Ian Bird EGEE Operations Manager CERN Geneva, Switzerland ISGC, Taipei.
EGEE-III INFSO-RI Enabling Grids for E-sciencE EGEE and gLite are registered trademarks Christos Kanellopoulos Activity Manager.
Outline Cosmic Rays and Super-Nova Remnants
NOY TAZA Neutrino Observatory Project in TAZA A. Hoummada University HASSAN II CASABLANCA On behalf of NOY collaboration D. Lebrun & F. Montanet LPSC -
June 6, 2006 CALOR 2006 E. Hays University of Chicago / Argonne National Lab VERITAS Imaging Calorimetry at Very High Energies.
WLCG Laura Perini1 EGI Operation Scenarios Introduction to panel discussion.
05/02/031 Next Generation Ground- based  -ray Telescopes Frank Krennrich April,
Abstract Since the beginning of its operation in April 2005, the MAGIC telescope was able to observe ten different GRB events since their early emission.
Università di Perugia Enabling Grids for E-sciencE Status of and requirements for Computational Chemistry NA4 – SA1 Meeting – 6 th April.
INFSO-RI Enabling Grids for E-sciencE Comp Chem and MAGIC (based on info from Den Haag and follow-up since) F Harris on behalf of.
Sources emitting gamma-rays observed in the MAGIC field of view Jelena-Kristina Željeznjak , Zagreb.
INFSO-RI Enabling Grids for E-sciencE The EGEE Project Owen Appleton EGEE Dissemination Officer CERN, Switzerland Danish Grid Forum.
EGEE-II INFSO-RI Enabling Grids for E-sciencE EGEE and gLite are registered trademarks Simulations and Offline Data Processing for.
IAG – Israel Academic Grid, EGEE and HEP in Israel Prof. David Horn Tel Aviv University.
EGEE-III INFSO-RI Enabling Grids for E-sciencE EGEE and gLite are registered trademarks User Support for Distributed Computing Infrastructures.
Status of the MAGIC Telescope Project Presented by Razmick Mirzoyan On behalf of the MAGIC Collaboration Max-Planck-Institute for Physics (Werner-Heisenberg-Institute)
ICFA DDW'06 - Cracow1 (HEP) GRID Activities in Hungary Csaba Hajdu KFKI RMKI Budapest.
Jiri Chudoba for the Pierre Auger Collaboration Institute of Physics of the CAS and CESNET.
INFSO-RI Enabling Grids for E-sciencE VOCE & AUGER User Support a Current State & Future Plans Jan Kmuníček, Jiří Chudoba CESNET.
EGEE is a project funded by the European Union under contract IST Compchem VO's user support EGEE Workshop for VOs Karlsruhe (Germany) March.
RI EGI-InSPIRE RI Astronomy and Astrophysics Dr. Giuliano Taffoni Dr. Claudio Vuerli.
EGEE-II INFSO-RI Enabling Grids for E-sciencE Practical using EGEE middleware: Putting it all together!
Tobias Jogler Max – Planck Institut für Physik The MAGIC view of our Galaxy Tobias Jogler for the MAGIC Collaboration.
EGI-InSPIRE RI EGI-InSPIRE EGI-InSPIRE RI Pierre Auger Observatory Jiří Chudoba Institute of Physics and CESNET, Prague.
INFSO-RI Enabling Grids for E-sciencE The t-Infrastructure, Gilda Dr. Rüdiger Berlich, Forschungszentrum Karlsruhe / Germany Dr.
Introduction to Grid and Grid applications Peter Kacsuk MTA SZTAKI
Tobias Jogler Max-Planck Institut für Physik IMPRS YSW Ringberg 2007 VHE emission from binary systems Outline Binary systems Microquasar Pulsar binaries.
CTA Cerenkov Telescope Array G. Lamanna (1), C. Vuerli (2) (1) CNRS/IN2P3/LAPP, Annecy (FR) (2) INAF – Istituto Nazionale di Astrofisica, Trieste (IT)
The MAGIC Data Center storage and computing infrastructures in Grid
HAWC Science Survey of 2p sr up to 100 TeV energies Extended Sources
Instrumentation and Methods in Astroparticle Physics Physics 801
Gamma Ray Satellites Simulations with Geant4
SNRs as PeVatron candidates for CTA
Presentation transcript:

H. Kornmayer MAGIC-Grid EGEE, Panel discussion, Pisa, Monte Carlo Production for the MAGIC telescope A generic application of EGEE Towards the MAGIC Grid Harald Kornmayer, Toni Coarasa; Mirco Mazzucato, Manuel Delfino Forschungszentrum Karlsruhe; Max-Planck-Institut für Physik, München; CNAF/INFN Bologna; PIC, Barcelona In cooperation with the MAGIC collaboration In cooperation with the EGEE project

H. Kornmayer MAGIC-Grid EGEE, Panel discussion, Pisa, What kind of MAGIC? Physics Goals: Origin of VHE  rays Gamma ray: 30 GeV - TeV Active Galactic Nuclei (AGN) Supernova Remnants Unidentified EGRET sources Gamma Ray Burst ~ 10 km Particle shower ~ 1 o Cherenkov light ~ 120 m  ray MAGIC collaboration: - International (21 partners) - main partners in Italy, Spain and Germany - still a small collaboration IFAE Barcelona, UAB Barcelona, Humboldt U. Berlin, UC Davis, U. Lodz, UC Madrid, MPI München, INFN / U. Padova, INFN / U. Pisa, U. Potchefstrom, INFN / U. Siena, Tuorla Observatory, INFN / U. Udine, U. Würzburg, Yerevan Physics Inst., ETH Zürich GLAST (~ 1 m 2 ) Huge hadronic background  MC simulations

H. Kornmayer MAGIC-Grid EGEE, Panel discussion, Pisa, I need 1.5 million hadronic showers with Energy E, Direction (theta, phi),... As background sample for observation of „Crab nebula“ Run Magic MonteCarlo Simulation and register output data Run Magic Monte Carlo Simulation (MMCS) and register output data Simulate the Telescope Geometry with the reflector program for all interesting MMCS files and register output data Simulate the Starlight Background for a given position in the sky and register output data Simulate the response of the MAGIC camera for all interesting reflector files and register output data Merge the shower simulation and the StarLight simulation and produce a MonteCarlo data sample MAGIC Grid – MC Workflow

H. Kornmayer MAGIC-Grid EGEE, Panel discussion, Pisa, MAGIC Grid – the idea A lot of MC simulation needed to reduce the hadronic background to got scientific results at low energies –to simulate the background of one night, 70 CPUs (P4 2GHz) needs to run days Observation data are big too!! –Requirement: Easy accessible at different sites –MAGIC telescope II will start 2007 (scalability)  MAGIC Grid: –Use the three national Grid centers as a backbone All are members of EGEE –Connect MAGIC resources to enable collaboration –( Get resources for free! ) MAGIC MC simulation was accepted as Generic application by EGAAP

H. Kornmayer MAGIC-Grid EGEE, Panel discussion, Pisa, MAGIC Grid – the reality Good : -MAGIC VO in operation -MAGIC Grid consists of (>) 21 sites -MAGIC Grid is operational - GGUS User -MC Data are stored at PIC - Sustainability is given -Training performed - First Magicans become adicted by the EGEE Grid - They want more training! Good : -MAGIC VO in operation -MAGIC Grid consists of (>) 21 sites -MAGIC Grid is operational - GGUS User -MC Data are stored at PIC - Sustainability is given -Training performed - First Magicans become adicted by the EGEE Grid - They want more training! Good : -Three data challenges: - Mar/Apr 2005: 10% failure - July 2005: 3.9%failure - Sept 2005: 3.4% failure - Improvements: -Underlying Middleware -Operation of Services -A lot of material available! Good : -Three data challenges: - Mar/Apr 2005: 10% failure - July 2005: 3.9%failure - Sept 2005: 3.4% failure - Improvements: -Underlying Middleware -Operation of Services -A lot of material available!

H. Kornmayer MAGIC-Grid EGEE, Panel discussion, Pisa, MAGIC Grid – the reality II Issues: Communication in a complex environment One spents a lot of time to find the right person Many board to participate Account Manager for generic VOs not available! Installation of MW stack Still a complex enterprise Integration of new sites - # of supported OS = 1 - Installation is complex - Integration of small sites not effective Issues: Communication in a complex environment One spents a lot of time to find the right person Many board to participate Account Manager for generic VOs not available! Installation of MW stack Still a complex enterprise Integration of new sites - # of supported OS = 1 - Installation is complex - Integration of small sites not effective Issues: Uncertainty about the MW LCG-2.Y vs gLite-1.Y? What will be the MW of LCG? What is about GT4? WSRF? Interoperability Virtual obervatories are not based on EGEE MW Workflows? Data sustainability Do I need a „non-Grid“ copy of my data? TCO of the MAGIC Grid When will the bill arrive? Issues: Uncertainty about the MW LCG-2.Y vs gLite-1.Y? What will be the MW of LCG? What is about GT4? WSRF? Interoperability Virtual obervatories are not based on EGEE MW Workflows? Data sustainability Do I need a „non-Grid“ copy of my data? TCO of the MAGIC Grid When will the bill arrive?

H. Kornmayer MAGIC-Grid EGEE, Panel discussion, Pisa, MAGIC Grid – future prospects MAGIC Grid is reality Start with production of MC using MAGIC Grid resources soon! –We plan to ask (temporarily) for more CPU! MAGIC collaboration built a task-force to evaluate Grid as the backbone for MAGIC II –2 telescopes with a new DAQ system with faster FADCs –MC and real data! MAGIC Grid is reality Start with production of MC using MAGIC Grid resources soon! –We plan to ask (temporarily) for more CPU! MAGIC collaboration built a task-force to evaluate Grid as the backbone for MAGIC II –2 telescopes with a new DAQ system with faster FADCs –MC and real data! MAGIC is a good example to do e-Science to use the e-Infrastructure to exploit Grid-Technology „Towards a virtual observatory for VHE  -rays“ proceeding for Cherenkov 2005 MAGIC is a good example to do e-Science to use the e-Infrastructure to exploit Grid-Technology „Towards a virtual observatory for VHE  -rays“ proceeding for Cherenkov 2005 HESS/Africa Veritas/US MAGIC/EU Kangaroo - AUS/JP

H. Kornmayer MAGIC-Grid EGEE, Panel discussion, Pisa, Notizen Middleware limited to one OS system dialect Installation still a big use, no out of the box Data accessibility, data provisioning, etc. (Still scientists want to know where the data are What is the right MW to chose? Is EGEE the right track? What is about GT4? What is about Interoperability?