The offline software framework of the Pierre Auger Observatory
Creators
- 1. INFN and University of Torino, Via P. Giuria 1, I-10125 Turin (Italy)
- 2. Centro Brasileiro de Pesquisas Fisicas, Rua Dr. Xavier Sigaud, 150, Rio de Janeiro-RJ, CEP 22290 180 (Brazil)
- 3. Northeastern University, 360 Huntington Ave., Boston, MA 02115 (United States)
- 4. Departamento de Fisica de Altas Energias, Instituto de Ciencias Nucleares, Universidad Nacional Autonoma de Mexico, Mexico D.F., C.P. 04510 (Mexico)
- 5. Santa Cruz Institute for Particle Physics, University of California, Santa Cruz, CA 95046 (United States)
- 6. Louisiana State University, Baton Rouge, LA 70803 (United States)
- 7. Instituto de Fisica Gleb Wataghin, Universidade Estadual de Campinas UNICAMP, Campinas-SP, CP 6165, CEP 13083 970 (Brazil)
- 8. Karlsruhe Institute of Technology KIT, University and Forschungszentrum Karlsruhe, P.O. Box 3640, D-76021 Karlsruhe (Germany)
- 9. University of Nova Gorica, Vipavska 13, P.O. Box 301, SI-5001 Nova Gorica (Slovenia)
Description
The Pierre Auger Observatory is designed to unveil the nature and the origins of the highest energy cosmic rays. The large and geographically dispersed collaboration of physicists and the wide-ranging collection of simulation and reconstruction tasks pose some special challenges for the offline analysis software. We have designed and implemented a general purpose framework which allows collaborators to contribute algorithms and sequencing instructions to build up the variety of applications they require. The framework includes machinery to manage these user codes, to organize the abundance of user-contributed configuration files, to facilitate multi-format file handling, and to provide access to event and time-dependent detector information which can reside in various data sources. A number of utilities are also provided, including a novel geometry package which allows manipulation of abstract geometrical objects independent of coordinate system choice. The framework is implemented in C++, and takes advantage of object oriented design and common open source tools, while keeping the user side simple enough for C++ novices to learn in a reasonable time. The distribution system incorporates unit and acceptance testing in order to support rapid development of both the core framework and contributed user code
Availability note (English)
Available from http://dx.doi.org/10.1016/j.nima.2007.07.010Additional details
Identifiers
- DOI
- 10.1016/j.nima.2007.07.010;
- arXiv
- arXiv:0707.1652v1;
- PII
- S0168-9002(07)01410-6;
Publishing Information
- Journal Title
- Nuclear Instruments and Methods in Physics Research. Section A, Accelerators, Spectrometers, Detectors and Associated Equipment
- Journal Volume
- 580
- Journal Issue
- 3
- Journal Page Range
- p. 1485-1496
- ISSN
- 0168-9002
- CODEN
- NIMAER
INIS
- Country of Publication
- Netherlands
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 39062327
- Subject category
- S46: INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY;
- Descriptors DEI
- ALGORITHMS; COMPUTER CODES; CONFIGURATION; COORDINATES; COSMIC RADIATION; DESIGN; DISTRIBUTION; GEOMETRY; MACHINERY; SIMULATION; TIME DEPENDENCE
- Descriptors DEC
- EQUIPMENT; IONIZING RADIATIONS; MATHEMATICAL LOGIC; MATHEMATICS; RADIATIONS
Optional Information
- Copyright
- Copyright (c) 2007 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.