guest ::
| Home > Publications database > The NectarCAM timing system > print |
| Home > Publications database > The NectarCAM timing system > print |
| 001 | 586762 | ||
| 005 | 20250724131902.0 | ||
| 024 | 7 | _ | |a 10.1016/j.nima.2023.168398 |2 doi |
| 024 | 7 | _ | |a Bradascio:2023lwj |2 INSPIRETeX |
| 024 | 7 | _ | |a inspire:2628530 |2 inspire |
| 024 | 7 | _ | |a 0167-5087 |2 ISSN |
| 024 | 7 | _ | |a 0168-9002 |2 ISSN |
| 024 | 7 | _ | |a 1872-9576 |2 ISSN |
| 024 | 7 | _ | |a arXiv:2301.13828 |2 arXiv |
| 024 | 7 | _ | |a 10.3204/PUBDB-2023-04000 |2 datacite_doi |
| 024 | 7 | _ | |a altmetric:142002534 |2 altmetric |
| 024 | 7 | _ | |a WOS:001040635400001 |2 WOS |
| 024 | 7 | _ | |a openalex:W4319991384 |2 openalex |
| 037 | _ | _ | |a PUBDB-2023-04000 |
| 041 | _ | _ | |a English |
| 082 | _ | _ | |a 530 |
| 088 | _ | _ | |a arXiv:2301.13828 |2 arXiv |
| 100 | 1 | _ | |a Bradascio, F. |0 P:(DE-H253)PIP1022296 |b 0 |e Corresponding author |u desy |
| 245 | _ | _ | |a The NectarCAM timing system |
| 260 | _ | _ | |a Amsterdam |c 2023 |b North-Holland Publ. Co. |
| 336 | 7 | _ | |a article |2 DRIVER |
| 336 | 7 | _ | |a Output Types/Journal article |2 DataCite |
| 336 | 7 | _ | |a Journal Article |b journal |m journal |0 PUB:(DE-HGF)16 |s 1688543169_3479727 |2 PUB:(DE-HGF) |
| 336 | 7 | _ | |a ARTICLE |2 BibTeX |
| 336 | 7 | _ | |a JOURNAL_ARTICLE |2 ORCID |
| 336 | 7 | _ | |a Journal Article |0 0 |2 EndNote |
| 500 | _ | _ | |a 8 pages, 13 figures |
| 520 | _ | _ | |a NectarCAM is a Cherenkov camera which is going to equip the Medium-Sized Telescopes (MST) of the northern site of the Cherenkov Telescope Array Observatory (CTAO). NectarCAM is equipped with 265 modules, each consisting of 7 photo-multiplier tubes (PMTs), a Front-End Board and a local camera trigger system used for data acquisition. This paper addresses the timing performance of NectarCAM which are crucial to reduce the noise in shower images and improve image cleaning as well as to discriminate between gamma-ray photons and cosmic-ray background and finally to allow coincidence identification with neighboring telescopes for stereoscopic operations. Verification tests of the system have been performed in a dark room using various light sources to illuminate the first NectarCAM unit. The resulting timing precision and accuracy of the trigger arrival relative to a laser source, of individual and multiple pixel signals have been studied and are shown to comply to CTAO requirements. |
| 536 | _ | _ | |a 613 - Matter and Radiation from the Universe (POF4-613) |0 G:(DE-HGF)POF4-613 |c POF4-613 |f POF IV |x 0 |
| 588 | _ | _ | |a Dataset connected to CrossRef, INSPIRE, Journals: bib-pubdb1.desy.de |
| 650 | _ | 7 | |a trigger |2 INSPIRE |
| 650 | _ | 7 | |a observatory |2 INSPIRE |
| 650 | _ | 7 | |a laser |2 INSPIRE |
| 650 | _ | 7 | |a background |2 INSPIRE |
| 650 | _ | 7 | |a photomultiplier |2 INSPIRE |
| 650 | _ | 7 | |a showers |2 INSPIRE |
| 650 | _ | 7 | |a tube |2 INSPIRE |
| 650 | _ | 7 | |a photon |2 INSPIRE |
| 650 | _ | 7 | |a data acquisition |2 INSPIRE |
| 650 | _ | 7 | |a site |2 INSPIRE |
| 650 | _ | 7 | |a Cherenkov Telescope Array |2 INSPIRE |
| 650 | _ | 7 | |a noise |2 INSPIRE |
| 650 | _ | 7 | |a gamma ray |2 INSPIRE |
| 650 | _ | 7 | |a performance |2 INSPIRE |
| 650 | _ | 7 | |a Cherenkov |2 INSPIRE |
| 650 | _ | 7 | |a cosmic radiation |2 INSPIRE |
| 650 | _ | 7 | |a pixel |2 INSPIRE |
| 650 | _ | 7 | |a NectarCAM |2 autogen |
| 650 | _ | 7 | |a Gamma ray |2 autogen |
| 650 | _ | 7 | |a Cherenkov |2 autogen |
| 650 | _ | 7 | |a CTAO |2 autogen |
| 650 | _ | 7 | |a Timing resolution |2 autogen |
| 650 | _ | 7 | |a PMT transit time |2 autogen |
| 650 | _ | 7 | |a Trigger |2 autogen |
| 693 | _ | _ | |0 EXP:(DE-H253)CTA-20150101 |5 EXP:(DE-H253)CTA-20150101 |e Cherenkov Telescope Array |x 0 |
| 700 | 1 | _ | |a Rueda, H. |b 1 |
| 700 | 1 | _ | |a Barrio, J. A. |b 2 |
| 700 | 1 | _ | |a Biteau, J. |b 3 |
| 700 | 1 | _ | |a Brun, F. |b 4 |
| 700 | 1 | _ | |a Champion, C. |b 5 |
| 700 | 1 | _ | |a Glicenstein, J.-F. |b 6 |
| 700 | 1 | _ | |a Hoffmann, D. |b 7 |
| 700 | 1 | _ | |a Jean, P. |b 8 |
| 700 | 1 | _ | |a Lenain, J. P. |b 9 |
| 700 | 1 | _ | |a Louis, F. |b 10 |
| 700 | 1 | _ | |a Perez, A. |b 11 |
| 700 | 1 | _ | |a Punch, M. |b 12 |
| 700 | 1 | _ | |a Sizun, P. |b 13 |
| 700 | 1 | _ | |a Sulanke, K.-H. |0 P:(DE-H253)PIP1003716 |b 14 |u desy |
| 700 | 1 | _ | |a Tejedor, L. A. |b 15 |
| 700 | 1 | _ | |a Vallage, B. |b 16 |
| 773 | _ | _ | |a 10.1016/j.nima.2023.168398 |g Vol. 1054, p. 168398 - |0 PERI:(DE-600)1466532-3 |p 168398 |t Nuclear instruments & methods in physics research / A |v 1054 |y 2023 |x 0167-5087 |
| 787 | 0 | _ | |a Bradascio, F. et.al. |d 2022 |i IsParent |0 PUBDB-2023-00869 |r arXiv:2301.13828 |t The NectarCAM Timing System |
| 856 | 4 | _ | |u https://bib-pubdb1.desy.de/record/586762/files/1-s2.0-S0168900223003881-main.pdf |
| 856 | 4 | _ | |y OpenAccess |u https://bib-pubdb1.desy.de/record/586762/files/2301.13828v2.pdf |
| 856 | 4 | _ | |x pdfa |u https://bib-pubdb1.desy.de/record/586762/files/1-s2.0-S0168900223003881-main.pdf?subformat=pdfa |
| 856 | 4 | _ | |y OpenAccess |x pdfa |u https://bib-pubdb1.desy.de/record/586762/files/2301.13828v2.pdf?subformat=pdfa |
| 909 | C | O | |o oai:bib-pubdb1.desy.de:586762 |p openaire |p open_access |p VDB |p driver |p dnbdelivery |
| 910 | 1 | _ | |a Deutsches Elektronen-Synchrotron |0 I:(DE-588b)2008985-5 |k DESY |b 0 |6 P:(DE-H253)PIP1022296 |
| 910 | 1 | _ | |a Deutsches Elektronen-Synchrotron |0 I:(DE-588b)2008985-5 |k DESY |b 14 |6 P:(DE-H253)PIP1003716 |
| 913 | 1 | _ | |a DE-HGF |b Forschungsbereich Materie |l Matter and the Universe |1 G:(DE-HGF)POF4-610 |0 G:(DE-HGF)POF4-613 |3 G:(DE-HGF)POF4 |2 G:(DE-HGF)POF4-600 |4 G:(DE-HGF)POF |v Matter and Radiation from the Universe |x 0 |
| 914 | 1 | _ | |y 2023 |
| 915 | _ | _ | |a DBCoverage |0 StatID:(DE-HGF)0160 |2 StatID |b Essential Science Indicators |d 2023-03-30 |
| 915 | _ | _ | |a Creative Commons Attribution-NonCommercial-NoDerivs CC BY-NC-ND 4.0 |0 LIC:(DE-HGF)CCBYNCND4 |2 HGFVOC |
| 915 | _ | _ | |a WoS |0 StatID:(DE-HGF)0113 |2 StatID |b Science Citation Index Expanded |d 2023-03-30 |
| 915 | _ | _ | |a OpenAccess |0 StatID:(DE-HGF)0510 |2 StatID |
| 915 | _ | _ | |a Nationallizenz |0 StatID:(DE-HGF)0420 |2 StatID |d 2023-08-25 |w ger |
| 915 | _ | _ | |a DBCoverage |0 StatID:(DE-HGF)0300 |2 StatID |b Medline |d 2023-08-25 |
| 915 | _ | _ | |a DBCoverage |0 StatID:(DE-HGF)0199 |2 StatID |b Clarivate Analytics Master Journal List |d 2023-08-25 |
| 915 | _ | _ | |a DBCoverage |0 StatID:(DE-HGF)0150 |2 StatID |b Web of Science Core Collection |d 2023-08-25 |
| 915 | _ | _ | |a DBCoverage |0 StatID:(DE-HGF)1160 |2 StatID |b Current Contents - Engineering, Computing and Technology |d 2023-08-25 |
| 915 | _ | _ | |a DBCoverage |0 StatID:(DE-HGF)1150 |2 StatID |b Current Contents - Physical, Chemical and Earth Sciences |d 2023-08-25 |
| 915 | _ | _ | |a JCR |0 StatID:(DE-HGF)0100 |2 StatID |b NUCL INSTRUM METH A : 2022 |d 2023-08-25 |
| 915 | _ | _ | |a DBCoverage |0 StatID:(DE-HGF)0200 |2 StatID |b SCOPUS |d 2023-08-25 |
| 915 | _ | _ | |a DBCoverage |0 StatID:(DE-HGF)0600 |2 StatID |b Ebsco Academic Search |d 2023-08-25 |
| 915 | _ | _ | |a Peer Review |0 StatID:(DE-HGF)0030 |2 StatID |b ASC |d 2023-08-25 |
| 915 | _ | _ | |a IF < 5 |0 StatID:(DE-HGF)9900 |2 StatID |d 2023-08-25 |
| 920 | 1 | _ | |0 I:(DE-H253)CTAI-20201126 |k CTAI |l CTAI |x 0 |
| 980 | _ | _ | |a journal |
| 980 | _ | _ | |a VDB |
| 980 | _ | _ | |a UNRESTRICTED |
| 980 | _ | _ | |a I:(DE-H253)CTAI-20201126 |
| 980 | 1 | _ | |a FullTexts |
| Library | Collection | CLSMajor | CLSMinor | Language | Author |
|---|