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FADC signal reconstruction for the MAGIC telescope

dc.contributor.authorAntoranz Canales, Pedro
dc.contributor.authorBarrio Uña, Juan Abel
dc.contributor.authorContreras González, José Luis
dc.contributor.authorFonseca González, María Victoria
dc.contributor.authorLópez Moya, Marcos
dc.contributor.authorMiranda Pantoja, José Miguel
dc.contributor.authorNieto Castaño, Daniel
dc.date.accessioned2023-06-20T10:37:42Z
dc.date.available2023-06-20T10:37:42Z
dc.date.issued2008-09-11
dc.description© Elsevier Science. We would like to thank the IAC for the excellent working conditions at the Observatory de los Muchachos in La Palma. The support of the German BMBF and MPG, the Italian INFN and the Spanish CICYT is gratefully acknowledged. The MAGIC telescope is also supported by ETH Research Grant TH 34/04 3 and the Polish MNil Grant 1P03D01028.
dc.description.abstractUntil April 2007 the Major Atmospheric Gamma ray Imaging Cherenkov (MAGIC) telescope used a 300 MSamples/s flash analog-to-digital converter (FADC) system to sample the shaped photomultiplier tube (PMT) signals produced by the captured Cherenkov photons of air showers. Different algorithms to reconstruct the signal from the read-out samples (extractors) have been implemented and are described and compared. Criteria based on the obtained charge and time resolution/bias are defined and used to judge the different extractors, by applying them to calibration, cosmic and pedestal signals. The achievable charge and time resolution have been derived as functions of the number of incident photoelectrons. (C) 2008 Elsevier B.V. All rights reserved.
dc.description.departmentDepto. de Estructura de la Materia, Física Térmica y Electrónica
dc.description.facultyFac. de Ciencias Físicas
dc.description.refereedTRUE
dc.description.sponsorshipGerman BMBF
dc.description.sponsorshipGerman MPG
dc.description.sponsorshipItalian INFN
dc.description.sponsorshipSpanish CICYT
dc.description.sponsorshipETH
dc.description.sponsorshipPolish MNil
dc.description.statuspub
dc.eprint.idhttps://eprints.ucm.es/id/eprint/23105
dc.identifier.doi10.1016/j.nima.2008.06.043
dc.identifier.issn0168-9002
dc.identifier.officialurlhttp://dx.doi.org/10.1016/j.nima.2008.06.043
dc.identifier.relatedurlhttp://www.sciencedirect.com
dc.identifier.urihttps://hdl.handle.net/20.500.14352/50824
dc.issue.number3
dc.journal.titleNuclear instruments & methods in physics research. Section A, Accelerators spectrometers detectors and associated equipment
dc.language.isoeng
dc.page.final419
dc.page.initial407
dc.publisherElsevier Science BV
dc.relation.projectIDTH 34/04 3
dc.relation.projectID1P03D01028
dc.rights.accessRightsrestricted access
dc.subject.cdu537
dc.subject.cdu539.1
dc.subject.keywordGamma-Ray Astronomy
dc.subject.keywordCalibration
dc.subject.keywordSystem
dc.subject.keywordTests.
dc.subject.ucmElectrónica (Física)
dc.subject.ucmElectricidad
dc.subject.ucmFísica nuclear
dc.subject.unesco2202.03 Electricidad
dc.subject.unesco2207 Física Atómica y Nuclear
dc.titleFADC signal reconstruction for the MAGIC telescope
dc.typejournal article
dc.volume.number594
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