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001     315091
005     20211110140033.0
020 _ _ |a 978-3-945931-08-0
024 7 _ |2 datacite_doi
|a 10.3204/DESY-PROC-2016-05/22
024 7 _ |2 ISSN
|a 1435-8077
037 _ _ |a PUBDB-2016-05626
041 _ _ |a English
100 1 _ |0 P:(DE-HGF)0
|a Caminata, A.
|b 0
111 2 _ |0 C16-03-17
|2 inspire
|a Magellan Workshop
|c Hamburg
|d 2016-03-17 - 2016-03-18
|w Germany
245 _ _ |a The SOX experiment: understanding the detector behavior using calibration sources
260 _ _ |a Hamburg
|b Verlag Deutsches Elektronen-Synchrotron
|c 2016
295 1 0 |a Caminata, A. "The SOX experiment: understanding the detector behavior using calibration sources" in Proceedings, Magellan Workshop: Connecting Neutrino Physics and Astronomy / Dahmke, Stefan K.G., Meyer, Mikko, Vanhoefer, Laura (eds.), Deutsches Elektronen-Synchrotron, DESY : 2016 ; Magellan Workshop, 2016-03-17 - 2016-03-18, Hamburg
300 _ _ |a 175-180
336 7 _ |2 ORCID
|a CONFERENCE_PAPER
336 7 _ |0 33
|2 EndNote
|a Conference Paper
336 7 _ |2 BibTeX
|a INPROCEEDINGS
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336 7 _ |2 DataCite
|a Output Types/Conference Paper
336 7 _ |0 PUB:(DE-HGF)8
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|a Contribution to a conference proceedings
|b contrib
|m contrib
|s 1480328666_21385
336 7 _ |0 PUB:(DE-HGF)7
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|a Contribution to a book
|m contb
490 0 _ |0 PERI:(DE-600)2450075-6
|a DESY-PROC
520 _ _ |a The SOX experiment investigates the existence of light sterile neutrinos. A solid signal would mean the discovery of the first particles beyond the Standard Electroweak Model and would have profound implications in our understanding of the Universe and of fundamental particle physics. In case of a negative result, it is able to close a long standing debate about the reality of the neutrino anomalies. The SOX experiment will use a $^{144}Ce-^{144}Pr$ antineutrino generator placed 8.5~m below the Borexino liquid scintillator detector. In view of the SOX experiment, a precise knowledge of the energy response and the spatial reconstruction of the antineutrino events is very important. Consequently, a calibration campaign of the Borexino detector is foreseen before the beginning of the SOX data taking. This paper briefly reviews the techniques used for calibrate the Borexino detector.
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787 0 _ |0 PUBDB-2016-05604
|a Dahmke, Stefan K.G. et. al.
|d Deutsches Elektronen-Synchrotron, DESY
|i isPartOf
|r DESY-PROC-2016-05
|t Proceedings, Magellan Workshop: Connecting Neutrino Physics and Astronomy: Hamburg, Germany, March 17-18, 2016
856 4 _ |u https://bib-pubdb1.desy.de/record/315091/files/fulltext.pdf
|y OpenAccess
909 C O |o oai:bib-pubdb1.desy.de:315091
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|b 72
910 1 _ |0 I:(DE-HGF)0
|6 P:(DE-HGF)0
|a St. Petersburg, INP
|b 73
910 1 _ |0 I:(DE-HGF)0
|6 P:(DE-HGF)0
|a Genoa U.
|b 74
910 1 _ |0 I:(DE-HGF)0
|6 P:(DE-HGF)0
|a INFN, Genoa
|b 74
910 1 _ |0 I:(DE-HGF)0
|6 P:(DE-HGF)0
|a Munich, Tech. U., Universe
|b 75
910 1 _ |0 I:(DE-HGF)0
|6 P:(DE-HGF)0
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|b 76
910 1 _ |0 I:(DE-HGF)0
|6 P:(DE-HGF)0
|a APC, Paris
|b 77
910 1 _ |0 I:(DE-HGF)0
|6 P:(DE-HGF)0
|a Perugia U.
|b 78
910 1 _ |0 I:(DE-HGF)0
|6 P:(DE-HGF)0
|a INFN, Perugia
|b 78
910 1 _ |0 I:(DE-HGF)0
|6 P:(DE-HGF)0
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|b 79
910 1 _ |0 I:(DE-HGF)0
|6 P:(DE-HGF)0
|a INFN, Genoa
|b 79
910 1 _ |0 I:(DE-HGF)0
|6 P:(DE-HGF)0
|a Munich, Tech. U., Universe
|b 80
910 1 _ |0 I:(DE-HGF)0
|6 P:(DE-HGF)0
|a Genoa U.
|b 81
910 1 _ |0 I:(DE-HGF)0
|6 P:(DE-HGF)0
|a INFN, Genoa
|b 81
910 1 _ |0 I:(DE-HGF)0
|6 P:(DE-HGF)0
|a Massachusetts U., Amherst
|b 82
910 1 _ |0 I:(DE-HGF)0
|6 P:(DE-HGF)0
|a Milan U.
|b 83
910 1 _ |0 I:(DE-HGF)0
|6 P:(DE-HGF)0
|a INFN, Milan
|b 83
910 1 _ |0 I:(DE-HGF)0
|6 P:(DE-H253)PIP1030037
|a Gran Sasso
|b 84
910 1 _ |0 I:(DE-HGF)0
|6 P:(DE-HGF)0
|a Milan U.
|b 85
910 1 _ |0 I:(DE-HGF)0
|6 P:(DE-HGF)0
|a INFN, Milan
|b 85
910 1 _ |0 I:(DE-HGF)0
|6 P:(DE-HGF)0
|a Perugia U.
|b 86
910 1 _ |0 I:(DE-HGF)0
|6 P:(DE-HGF)0
|a INFN, Perugia
|b 86
910 1 _ |0 I:(DE-HGF)0
|6 P:(DE-H253)PIP1009110
|a Gran Sasso
|b 87
910 1 _ |0 I:(DE-HGF)0
|6 P:(DE-H253)PIP1009110
|a APC, Paris
|b 87
910 1 _ |0 I:(DE-HGF)0
|6 P:(DE-HGF)0
|a Gran Sasso
|b 88
910 1 _ |0 I:(DE-HGF)0
|6 P:(DE-HGF)0
|a Munich, Tech. U., Universe
|b 89
910 1 _ |0 I:(DE-HGF)0
|6 P:(DE-HGF)0
|a IRFU, Saclay
|b 90
910 1 _ |0 I:(DE-HGF)0
|6 P:(DE-HGF)0
|a St. Petersburg, INP
|b 91
910 1 _ |0 I:(DE-HGF)0
|6 P:(DE-HGF)0
|a Heidelberg, Max Planck Inst.
|b 92
910 1 _ |0 I:(DE-HGF)0
|6 P:(DE-HGF)0
|a Kurchatov Inst., Moscow
|b 93
910 1 _ |0 I:(DE-HGF)0
|6 P:(DE-HGF)0
|a Moscow Phys. Eng. Inst.
|b 93
910 1 _ |0 I:(DE-HGF)0
|6 P:(DE-HGF)0
|a Dubna, JINR
|b 94
910 1 _ |0 I:(DE-HGF)0
|6 P:(DE-HGF)0
|a Dubna, JINR
|b 95
910 1 _ |0 I:(DE-HGF)0
|6 P:(DE-HGF)0
|a St. Petersburg, INP
|b 96
910 1 _ |0 I:(DE-HGF)0
|6 P:(DE-HGF)0
|a Gran Sasso
|b 97
910 1 _ |0 I:(DE-HGF)0
|6 P:(DE-HGF)0
|a Genoa U.
|b 98
910 1 _ |0 I:(DE-HGF)0
|6 P:(DE-HGF)0
|a INFN, Genoa
|b 98
910 1 _ |0 I:(DE-HGF)0
|6 P:(DE-HGF)0
|a Dresden, Tech. U.
|b 99
910 1 _ |0 I:(DE-HGF)0
|6 P:(DE-HGF)0
|a Kurchatov Inst., Moscow
|b 100
910 1 _ |0 I:(DE-HGF)0
|6 P:(DE-HGF)0
|a IRFU, Saclay
|b 101
910 1 _ |0 I:(DE-HGF)0
|6 P:(DE-HGF)0
|a IRFU, Saclay
|b 102
910 1 _ |0 I:(DE-HGF)0
|6 P:(DE-HGF)0
|a St. Petersburg, INP
|b 103
910 1 _ |0 I:(DE-HGF)0
|6 P:(DE-HGF)0
|a Virginia Tech.
|b 104
910 1 _ |0 I:(DE-HGF)0
|6 P:(DE-HGF)0
|a Munich, Tech. U., Universe
|b 105
910 1 _ |0 I:(DE-HGF)0
|6 P:(DE-H253)PIP1030266
|a UCLA
|b 106
910 1 _ |0 I:(DE-HGF)0
|6 P:(DE-HGF)0
|a U. Mainz, PRISMA
|b 107
910 1 _ |0 I:(DE-HGF)0
|6 P:(DE-H253)PIP1027911
|a U. Mainz, PRISMA
|b 108
910 1 _ |0 I:(DE-HGF)0
|6 P:(DE-HGF)0
|a Jagiellonian U.
|b 109
910 1 _ |0 I:(DE-HGF)0
|6 P:(DE-H253)PIP1014226
|a U. Mainz, PRISMA
|b 110
910 1 _ |0 I:(DE-HGF)0
|6 P:(DE-HGF)0
|a Virginia Tech.
|b 111
910 1 _ |0 I:(DE-HGF)0
|6 P:(DE-HGF)0
|a Dubna, JINR
|b 112
910 1 _ |0 I:(DE-HGF)0
|6 P:(DE-HGF)0
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|b 113
910 1 _ |0 I:(DE-HGF)0
|6 P:(DE-HGF)0
|a INFN, Genoa
|b 113
910 1 _ |0 I:(DE-HGF)0
|6 P:(DE-HGF)0
|a Dresden, Tech. U.
|b 114
910 1 _ |0 I:(DE-HGF)0
|6 P:(DE-HGF)0
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|b 115
910 1 _ |0 I:(DE-HGF)0
|6 P:(DE-HGF)0
|a Kurchatov Inst., Moscow
|b 116
910 1 _ |0 I:(DE-HGF)0
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|b 116
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