Calorimetry triggering in ATLAS

doi:10.1088/1742-6596/160/1/012061

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Igonkina O et al 2009 J. Phys.: Conf. Ser. 160 012061 doi:10.1088/1742-6596/160/1/012061

Calorimetry triggering in ATLAS

Igonkina O³², Achenbach R¹⁵, Adragna P³⁷, Aharrouche M²⁴, Alexandre G¹¹, Andrei V¹⁵, Anduaga X²¹, Aracena I⁴¹, Backlund S⁷, Baines J³⁸, Barnett B M³⁸, Bauss B²⁴, Bee C²⁶, Behera P¹⁹, Bell P²⁵, Bendel M²⁴, Benslama K³⁹, Berry T¹⁶, Bogaerts A⁷, Bohm C⁴³, Bold T^44,9, Booth J R A⁵, Bosman M⁴, Boyd J⁷, Bracinik J⁵, Brawn I P³⁸, Brelier B²⁸, Brooks W⁴⁷, Brunet S¹⁰, Bucci F¹¹, Casadei D³¹, Casado P⁴, Cerri A⁷, Charlton D G⁵, Childers J T¹⁵, Collins N J⁵, Conde Muino P²⁰, Coura Torres R⁴⁰, Cranmer K³¹, Curtis C J⁵, Czyczula Z³⁰, Dam M³⁰, Damazio D³, Davis A O³⁸, De Santo A¹⁶, Degenhardt J³⁶, Delsart P-A²⁸, Demers S⁴¹, Demirkoz B⁷, Di Mattia A²³, Diaz M⁴², Djilkibaev R³¹, Dobson E³⁴, Dova M T²¹, Dufour M-A²⁷, Eckweiler S²⁴, Ehrenfeld W^14,10, Eifert T¹¹, Eisenhandler E³⁷, Ellis N⁷, Emeliyanov D³⁸, Enoque Ferreira de, Lima D⁴⁰, Faulkner P J W⁵, Ferland J²⁸, Flacher H⁷, Fleckner J E¹⁵, Flowerdew M²², Fonseca-Martin T¹⁶, Fratina S³⁶, Fhlisch F¹⁵, Gadomski S¹¹, Gallacher M P⁵, Garitaonandia Elejabarrieta H³², Gee C N P³⁸, George S¹⁶, Gillman A R³⁸, Goncalo R¹⁶, Grabowska-Bold I⁹, Groll M²⁴, Gringer C²⁴, Hadley D R⁵, Haller J^14,10, Hamilton A¹¹, Hanke P¹⁵, Hauser R²³, Hellman S⁴³, Hidvgi A⁴³, Hillier S J⁵, Hryn'ova T⁷, Idarraga J²⁸, Johansen M⁴³, Johns K², Kalinowski A³⁹, Khoriauli G³⁹, Kirk J³⁸, Klous S³², Kluge E-E¹⁵, Koeneke K¹⁰, Konoplich R³¹, Konstantinidis N⁴⁵, Kwee R¹⁷, Landon M³⁷, LeCompte T¹, Ledroit F¹³, Lei X², Lendermann V¹⁵, Lilley J N⁵, Losada M⁶, Maettig S^14,10, Mahboubi K¹⁵, Mahout G⁵, Maltrana D⁴², Marino C¹⁸, Masik J²⁵, Meier K¹⁵, Middleton R P³⁸, Mincer A³¹, Moa T⁴³, Monticelli F²¹, Moreno D⁶, Morris J D³⁷, Mller F¹⁵, Navarro G A⁶, Negri A³⁵, Nemethy P³¹, Neusiedl A²⁴, Oltmann B²⁴, Olvito D³⁶, Osuna C⁴, Padilla C⁴, Panes B⁴², Parodi F¹², Perera V J O³⁸, Perez E⁴, Perez Reale V⁸, Petersen B⁷, Pinzon G⁶, Potter C²⁷, Prieur D P F³⁸, Prokishin F⁴⁷, Qian W³⁸, Quinonez F⁴², Rajagopalan S³, Reinsch A³³, Rieke S²⁴, Riu I⁴, Robertson S²⁷, Rodriguez D⁶, Rogriquez Y⁶, Rhr F¹⁵, Saavedra A⁴⁶, Sankey D P C³⁸, Santamarina C²⁷, Santamarina Rios C²⁷, Scannicchio D³⁵, Schiavi C¹², Schmitt K¹⁵, Schultz-Coulon H-C¹⁵, Schfer U²⁴, Segura E⁴, Silverstein D⁴¹, Silverstein S⁴³, Sivoklokov S²⁹, Sjlin J⁴³, Staley R J⁵, Stamen R¹⁵, Stelzer J¹⁰, Stockton M C⁵, Straessner A¹¹, Strom D³³, Sushkov S⁴, Sutton M⁴⁵, Tamsett M¹⁶, Tan C L A⁵, Tapprogge S²⁴, Thomas J P⁵, Thompson P D⁵, Torrence E³³, Tripiana M²¹, Urquijo P¹¹, Urrejola P⁴², Vachon B²⁷, Vercesi V³⁵, Vorwerk V⁴, Wang M³⁹, Watkins P M⁵, Watson A⁵, Weber P¹⁵, Weidberg T³⁴, Werner P⁷, Wessels M¹⁵, Wheeler-Ellis S⁴⁴, Whiteson D⁴⁴, Wiedenmann W⁴⁸, Wielers M³⁸, Wildt M²⁴, Winklmeier F⁷, Wu X¹¹, Xella S³⁰, Zhao L³¹, Zobernig H⁴⁸, de Seixas J M⁴⁰, dos Anjos A⁴⁸, As man B⁴³ and Özcan E⁴⁵

Show affiliations

Olga.Igonkina@cern.ch

¹ Argonne National Laboratory, Argonne, Illinois
² University of Arizona, Tucson, Arizona
³ Brookhaven National Laboratory (BNL), Upton, New York
⁴ Institut de Fsica d'Altes Energies (IFAE), Universitat Autnoma de Barcelona, Bellaterra (Barcelona)
⁵ School of Physics and Astronomy, The University of Birmingham, Birmingham
⁶ Universidad Antonio Narino, Bogot, Colmbia
⁷ European Laboratory for Particle Physics (CERN), Geneva
⁸ Nevis Laboratory, Columbia University, Irvington, New York
⁹ Faculty of Physics and Applied Computer Science, AGH University of Science and Technology, Cracow
¹⁰ Deutsches Elektronen-Synchrotron (DESY), Hamburg and Zeuthen
¹¹ Section de Physique, Universit de Genve, Geneva
¹² Dipartimento di Fisica dell' Universit di Genova e I.N.F.N., Genova
¹³ Laboratoire de Physique Subatomique et de Cosmologie de Grenoble (LPSC), IN2P3-CNRS-Universit Joseph Fourier, Grenoble
¹⁴ University of Hamburg, Germany
¹⁵ Kirchhoff Institut fr Physik, Universitt Heidelberg, Heidelberg
¹⁶ Department of Physics, Royal Holloway and Bedford New College, Egham
¹⁷ Institut fr Physik, Humboldt-Universitt, Berlin
¹⁸ Indiana University, Bloomington, Indiana
¹⁹ Iowa State University, Ames, Iowa
²⁰ Laboratorio de Instrumentaao e Fisica Experimental, Lisboa
²¹ Universidad Nacional de La Plata, La Plata
²² University of Liverpool, Liverpool
²³ Michigan State University, Department of Physics and Astronomy, East Lansing, Michigan
²⁴ Institut fr Physik, Universitt Mainz, Mainz
²⁵ School of Physics and Astronomy, University of Manchester, Manchester
²⁶ Centre de Physique des Particules de Marseille, IN2P3-CNRS, Marseille
²⁷ Department of Physics, McGill University, Montreal
²⁸ University of Montreal, Montreal
²⁹ Moscow State University, Moscow
³⁰ Niels Bohr Institute, University of Copenhagen, Copenhagen
³¹ Department of Physics, New York University, New York
³² Nikhef National Institute for Subatomic Physics, Amsterdam
³³ University of Oregon, Eugene, Oregon
³⁴ Department of Physics, Oxford University, Oxford
³⁵ Universit di Pavia, Dipartimento di Fisica Nucleare e Teorica, Pavia
³⁶ Department of Physics, University of Pennsylvania, Philadelphia, Pennsylvania
³⁷ Physics Department, Queen Mary, University of London, London
³⁸ STFC Rutherford Appleton Laboratory, Harwell Science and Innovation Campus, Didcot, Oxon
³⁹ University of Regina, Regina
⁴⁰ Universidade Federal do Rio de Janeiro, COPPE/EE/IF, Rio de Janeiro
⁴¹ Stanford Linear Accelerator Center (SLAC), Stanford
⁴² Pontificia Universidad Catlica, Santiago
⁴³ Fysikum, Stockholm University, Stockholm
⁴⁴ Department of Physics and Astronomy, University of California, Irvine, California
⁴⁵ Department of Physics and Astronomy, University College London, London
⁴⁶ University of Sydney, Sydney
⁴⁷ Universidad tecnica Federico Santa Maria, Valparaso
⁴⁸ Department of Physics, University of Wisconsin, Madison, Wisconsin

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Abstract References

The ATLAS experiment is preparing for data taking at 14 TeV collision energy. A rich discovery physics program is being prepared in addition to the detailed study of Standard Model processes which will be produced in abundance. The ATLAS multi-level trigger system is designed to accept one event in 2 mid 10⁵ to enable the selection of rare and unusual physics events. The ATLAS calorimeter system is a precise instrument, which includes liquid Argon electro-magnetic and hadronic components as well as a scintillator-tile hadronic calorimeter. All these components are used in the various levels of the trigger system. A wide physics coverage is ensured by inclusively selecting events with candidate electrons, photons, taus, jets or those with large missing transverse energy. The commissioning of the trigger system is being performed with cosmic ray events and by replaying simulated Monte Carlo events through the trigger and data acquisition system.

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