The exposure of the hybrid detector of the Pierre Auger Observatory
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The exposure of the hybrid detector of the Pierre Auger Observatory

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Degut a la parada de sistemes pevista a la Universitat de València del 19 al 22 de Gener, Roderic també romadrá fora de servei des del 19 a les 21:00 hores fins al 22 a les 17:00 hores. Disculpeu les molèsties. _______________________________________________________________________________________ Debido a la parada de sistemas prevista en la Universitat de València del 19 al 22 de Enero, Roderic también permanecerá fuera de servicio desde el 19 a las 21:00 hasta el 22 a las 17:00. Disculpen las molestias.

The exposure of the hybrid detector of the Pierre Auger Observatory

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The Pierre Auger Collaboration; Pastor Carpi, Sergio
Aquest document és un/a article, creat/da en: 2011
The Pierre Auger Observatory is a detector for ultra-high energy cosmic rays. It consists of a surface array to measure secondary particles at ground level and a fluorescence detector to measure the development of air showers in the atmosphere above the array. The 'hybrid' detection mode combines the information from the two subsystems. We describe the determination of the hybrid exposure for events observed by the fluorescence telescopes in coincidence with at least one water-Cherenkov detector of the surface array. A detailed knowledge of the time dependence of the detection operations is crucial for an accurate evaluation of the exposure. We discuss the relevance of monitoring data collected during operations, such as the status of the fluorescence detector, background light and atmospheric conditions, that are used in both simulation and reconstruction.

    The Pierre Auger Collaboration Pastor Carpi, Sergio 2011 The exposure of the hybrid detector of the Pierre Auger Observatory Astroparticle Physics 34 6 368 381
http://dx.doi.org/10.1016/j.astropartphys.2010.10.001
distribuït sota llicència Creative Commons de Reconeixement-NoComercial 3.0 No adaptada

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