000454025 001__ 454025
000454025 005__ 20211110162456.0
000454025 0247_ $$2doi$$a10.1393/ncc/i2020-20090-7
000454025 0247_ $$2INSPIRETeX$$aPillera:2020apt
000454025 0247_ $$2inspire$$ainspire:1829192
000454025 0247_ $$2datacite_doi$$a10.3204/PUBDB-2021-00382
000454025 0247_ $$2WOS$$aWOS:000582927900068
000454025 037__ $$aPUBDB-2021-00382
000454025 041__ $$aEnglish
000454025 082__ $$a530
000454025 1001_ $$aPillera, R.$$b0
000454025 1112_ $$a18th Incontri di Fisica delle Alte Energie$$cNaples$$d2019-04-08 - 2019-08-10$$gIFAE 2019$$wItaly
000454025 245__ $$aA fast muon tagger method for Imaging Atmospheric Cherenkov Telescopes
000454025 260__ $$aBologna [u.a.]$$bEd. Compositori$$c2020
000454025 300__ $$a3
000454025 3367_ $$2ORCID$$aCONFERENCE_PAPER
000454025 3367_ $$033$$2EndNote$$aConference Paper
000454025 3367_ $$0PUB:(DE-HGF)16$$2PUB:(DE-HGF)$$aJournal Article$$mjournal
000454025 3367_ $$2BibTeX$$aINPROCEEDINGS
000454025 3367_ $$2DRIVER$$aconferenceObject
000454025 3367_ $$2DataCite$$aOutput Types/Conference Paper
000454025 3367_ $$0PUB:(DE-HGF)8$$2PUB:(DE-HGF)$$aContribution to a conference proceedings$$bcontrib$$mcontrib$$s1611845618_11159
000454025 520__ $$aThe Cherenkov Telescope Array (CTA) will be the next major observatory for Very High Energy (VHE) γ-ray astronomy. Its optical throughput calibration relies on muon Cherenkov rings. This work is aimed at developing a fast and efficient muon tagger at the camera level for the CTA telescopes. A novel technique to tag muons using the capabilities of silicon photomultiplier Compact High-Energy Camera CHEC-S, one of the design options for the camera of the Small Size Telescopes (SSTs), has been developed, studying and comparing different algorithms such as circle fitting, machine learning and simple pixel counting. Their performance in terms of efficiency and computation speed was investigated using simulations with varying levels of night sky background light. The application of the best performing method to the Large Size Telescope (LST) camera has been also studied, with the goal of improving the speed of the muon preselection.
000454025 536__ $$0G:(DE-HGF)POF3-613$$a613 - Matter and Radiation from the Universe (POF3-613)$$cPOF3-613$$fPOF III$$x0
000454025 588__ $$aDataset connected to INSPIRE
000454025 650_7 $$2INSPIRE$$aphoton: detector
000454025 650_7 $$2INSPIRE$$aimaging
000454025 650_7 $$2INSPIRE$$amuon: particle identification
000454025 650_7 $$2INSPIRE$$aCherenkov Telescope Array
000454025 650_7 $$2INSPIRE$$adata analysis method
000454025 650_7 $$2INSPIRE$$anumerical calculations
000454025 650_7 $$2INSPIRE$$aartificial intelligence
000454025 650_7 $$2INSPIRE$$aperformance
000454025 650_7 $$2INSPIRE$$aefficiency
000454025 650_7 $$2INSPIRE$$aphotomultiplier: silicon
000454025 693__ $$0EXP:(DE-H253)CTA-20150101$$5EXP:(DE-H253)CTA-20150101$$eCherenkov Telescope Array$$x0
000454025 7001_ $$aDi Venere, L.$$b1
000454025 7001_ $$0P:(DE-H253)PIP1018949$$aGiavitto, Gianluca$$b2$$eCorresponding author
000454025 7001_ $$0R.Lopez.Coto.5$$aLopez Coto, R.$$b3
000454025 7001_ $$0P:(DE-HGF)0$$aCTA Collaboration$$b4$$eCollaboration author
000454025 773__ $$0PERI:(DE-600)2556226-5$$a10.1393/ncc/i2020-20090-7$$p90$$tIl nuovo cimento / C$$v43$$x0390-5551$$y2020
000454025 8564_ $$uhttps://bib-pubdb1.desy.de/record/454025/files/10.1393_ncc_i2020-20090-7.pdf$$yOpenAccess
000454025 8564_ $$uhttps://bib-pubdb1.desy.de/record/454025/files/10.1393_ncc_i2020-20090-7.gif?subformat=icon$$xicon$$yOpenAccess
000454025 8564_ $$uhttps://bib-pubdb1.desy.de/record/454025/files/10.1393_ncc_i2020-20090-7.jpg?subformat=icon-1440$$xicon-1440$$yOpenAccess
000454025 8564_ $$uhttps://bib-pubdb1.desy.de/record/454025/files/10.1393_ncc_i2020-20090-7.jpg?subformat=icon-180$$xicon-180$$yOpenAccess
000454025 8564_ $$uhttps://bib-pubdb1.desy.de/record/454025/files/10.1393_ncc_i2020-20090-7.jpg?subformat=icon-640$$xicon-640$$yOpenAccess
000454025 8564_ $$uhttps://bib-pubdb1.desy.de/record/454025/files/10.1393_ncc_i2020-20090-7.pdf?subformat=pdfa$$xpdfa$$yOpenAccess
000454025 909CO $$ooai:bib-pubdb1.desy.de:454025$$pdnbdelivery$$pdriver$$pVDB$$popen_access$$popenaire
000454025 9101_ $$0I:(DE-588b)2008985-5$$6P:(DE-H253)PIP1018949$$aDeutsches Elektronen-Synchrotron$$b2$$kDESY
000454025 9131_ $$0G:(DE-HGF)POF3-613$$1G:(DE-HGF)POF3-610$$2G:(DE-HGF)POF3-600$$3G:(DE-HGF)POF3$$4G:(DE-HGF)POF$$aDE-HGF$$bForschungsbereich Materie$$lMaterie und Universum$$vMatter and Radiation from the Universe$$x0
000454025 9141_ $$y2020
000454025 915__ $$0StatID:(DE-HGF)0200$$2StatID$$aDBCoverage$$bSCOPUS$$d2020-08-26
000454025 915__ $$0LIC:(DE-HGF)CCBY4$$2HGFVOC$$aCreative Commons Attribution CC BY 4.0
000454025 915__ $$0StatID:(DE-HGF)0112$$2StatID$$aWoS$$bEmerging Sources Citation Index$$d2020-08-26
000454025 915__ $$0StatID:(DE-HGF)0150$$2StatID$$aDBCoverage$$bWeb of Science Core Collection$$d2020-08-26
000454025 915__ $$0StatID:(DE-HGF)0510$$2StatID$$aOpenAccess
000454025 915__ $$0StatID:(DE-HGF)0300$$2StatID$$aDBCoverage$$bMedline$$d2020-08-26
000454025 915__ $$0StatID:(DE-HGF)0420$$2StatID$$aNationallizenz$$d2020-08-26$$wger
000454025 915__ $$0StatID:(DE-HGF)0199$$2StatID$$aDBCoverage$$bClarivate Analytics Master Journal List$$d2020-08-26
000454025 9201_ $$0I:(DE-H253)ZEU-EL-20120731$$kZEU-EL$$lElektronik$$x0
000454025 9201_ $$0I:(DE-H253)ZEU-CTA-20120731$$kZEU-CTA$$lCherenkov Telescope Array$$x1
000454025 980__ $$acontrib
000454025 980__ $$aVDB
000454025 980__ $$aUNRESTRICTED
000454025 980__ $$ajournal
000454025 980__ $$aI:(DE-H253)ZEU-EL-20120731
000454025 980__ $$aI:(DE-H253)ZEU-CTA-20120731
000454025 9801_ $$aFullTexts