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| Hauptseite > Publikationsdatenbank > Speeding up complex multivariate data analysis in Borexino with parallel computing based on Graphics Processing Unit > print |
| Hauptseite > Publikationsdatenbank > Speeding up complex multivariate data analysis in Borexino with parallel computing based on Graphics Processing Unit > print |
| 001 | 890238 | ||
| 005 | 20250813203210.0 | ||
| 024 | 7 | _ | |a 10.1088/1742-6596/1342/1/012115 |2 doi |
| 024 | 7 | _ | |a Ding:2018xrr |2 INSPIRETeX |
| 024 | 7 | _ | |a inspire:1675254 |2 inspire |
| 024 | 7 | _ | |a 1742-6588 |2 ISSN |
| 024 | 7 | _ | |a 1742-6596 |2 ISSN |
| 024 | 7 | _ | |a arXiv:1805.11125 |2 arXiv |
| 024 | 7 | _ | |a 2128/27070 |2 Handle |
| 024 | 7 | _ | |a altmetric:42950417 |2 altmetric |
| 024 | 7 | _ | |a WOS:001432953400115 |2 WOS |
| 037 | _ | _ | |a FZJ-2021-00825 |
| 082 | _ | _ | |a 530 |
| 100 | 1 | _ | |a Ding, X. F. |b 0 |
| 111 | 2 | _ | |a 15th International Conference on Topics in Astroparticle and Underground Physics |g TAUP 2017 |c Sudbury |d 2017-07-24 - 2017-07-28 |w Canada |
| 245 | _ | _ | |a Speeding up complex multivariate data analysis in Borexino with parallel computing based on Graphics Processing Unit |
| 260 | _ | _ | |a Bristol |c 2020 |b IOP Publ.87703 |
| 264 | _ | 1 | |3 print |2 Crossref |b IOP Publishing |c 2020-01-01 |
| 264 | _ | 1 | |3 print |2 Crossref |b IOP Publishing |c 2020-01-01 |
| 300 | _ | _ | |a 5 |
| 336 | 7 | _ | |a CONFERENCE_PAPER |2 ORCID |
| 336 | 7 | _ | |a Conference Paper |0 33 |2 EndNote |
| 336 | 7 | _ | |a Journal Article |0 PUB:(DE-HGF)16 |2 PUB:(DE-HGF) |m journal |
| 336 | 7 | _ | |a INPROCEEDINGS |2 BibTeX |
| 336 | 7 | _ | |a conferenceObject |2 DRIVER |
| 336 | 7 | _ | |a Output Types/Conference Paper |2 DataCite |
| 336 | 7 | _ | |a Contribution to a conference proceedings |b contrib |m contrib |0 PUB:(DE-HGF)8 |s 1754992079_25206 |2 PUB:(DE-HGF) |
| 500 | _ | _ | |a 5 pages, 2 figures, proceeding for TAUP 2017 XV International Conference on Topics in Astroparticle and Underground Physics |
| 520 | _ | _ | |a A spectral fitter based on the graphics processor unit (GPU) has been developed for Borexino solar neutrino analysis. It is able to shorten the fitting time to a superior level compared to the CPU fitting procedure. In Borexino solar neutrino spectral analysis, fitting usually requires around one hour to converge since it includes time-consuming convolutions in order to account for the detector response and pile-up effects. Moreover, the convergence time increases to more than two days when including extra computations for the discrimination of 11C and external γs. In sharp contrast, with the GPU-based fitter it takes less than 10 seconds and less than four minutes, respectively. This fitter is developed utilizing the GooFit project with customized likelihoods, pdfs and infrastructures supporting certain analysis methods. In this proceeding the design of the package, developed features and the comparison with the original CPU fitter are presented. |
| 536 | _ | _ | |a 612 - Cosmic Matter in the Laboratory (POF3-612) |0 G:(DE-HGF)POF3-612 |c POF3-612 |f POF III |x 0 |
| 542 | _ | _ | |i 2020-01-01 |2 Crossref |u http://creativecommons.org/licenses/by/3.0/ |
| 542 | _ | _ | |i 2020-01-01 |2 Crossref |u https://iopscience.iop.org/info/page/text-and-data-mining |
| 588 | _ | _ | |a Dataset connected to CrossRef, INSPIRE |
| 650 | _ | 7 | |a neutrino: solar |2 INSPIRE |
| 650 | _ | 7 | |a Borexino |2 INSPIRE |
| 650 | _ | 7 | |a spectral |2 INSPIRE |
| 650 | _ | 7 | |a graphics |2 INSPIRE |
| 650 | _ | 7 | |a pile-up |2 INSPIRE |
| 700 | 1 | _ | |a Vishneva, A. |0 A.Vishneva.2 |b 1 |
| 700 | 1 | _ | |a Penek, Ömer |0 P:(DE-Juel1)171602 |b 2 |e Corresponding author |
| 700 | 1 | _ | |a Marcocci, S. |0 S.Marcocci.1 |b 3 |
| 700 | 1 | _ | |a Borexino Collaboration |0 P:(DE-HGF)0 |b 4 |
| 773 | 1 | 8 | |a 10.1088/1742-6596/1342/1/012115 |b IOP Publishing |d 2020-01-01 |n 1 |p 012115 |3 journal-article |2 Crossref |t Journal of Physics: Conference Series |v 1342 |y 2020 |x 1742-6588 |
| 773 | _ | _ | |a 10.1088/1742-6596/1342/1/012115 |g Vol. 1342, no. 1, p. 012115 - |0 PERI:(DE-600)2166409-2 |n 1 |p 012115 |t Journal of physics / Conference Series |v 1342 |y 2020 |x 1742-6588 |
| 856 | 4 | _ | |u https://juser.fz-juelich.de/record/890238/files/Ding_2020_J._Phys.%20_Conf._Ser._1342_012115.pdf |y OpenAccess |
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| 910 | 1 | _ | |a Forschungszentrum Jülich |0 I:(DE-588b)5008462-8 |k FZJ |b 2 |6 P:(DE-Juel1)171602 |
| 913 | 1 | _ | |a DE-HGF |b Forschungsbereich Materie |l Materie und Universum |1 G:(DE-HGF)POF3-610 |0 G:(DE-HGF)POF3-612 |3 G:(DE-HGF)POF3 |2 G:(DE-HGF)POF3-600 |4 G:(DE-HGF)POF |v Cosmic Matter in the Laboratory |x 0 |
| 914 | 1 | _ | |y 2020 |
| 915 | _ | _ | |a Creative Commons Attribution CC BY 3.0 |0 LIC:(DE-HGF)CCBY3 |2 HGFVOC |
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| 999 | C | 5 | |1 Agostini |y 2017 |2 Crossref |o Agostini 2017 |
| 999 | C | 5 | |1 Agostini |y 2017 |2 Crossref |o Agostini 2017 |
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| 999 | C | 5 | |a 10.1038/nature13702 |9 -- missing cx lookup -- |1 Bellini |p 383 - |2 Crossref |t Nature |v 512 |y 2014 |
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| 999 | C | 5 | |1 Agostini |y 2017 |2 Crossref |o Agostini 2017 |
| 999 | C | 5 | |a 10.1007/JHEP08(2013)038 |9 -- missing cx lookup -- |1 Bellini |p 38 - |2 Crossref |t Journal of High Energy Physics |v 2013 |y 2013 |
| 999 | C | 5 | |a 10.1103/PhysRevD.89.112007 |9 -- missing cx lookup -- |1 Bellini |p 1 - |2 Crossref |t Physical Review D - Particles, Fields, Gravitation and Cosmology |v 89 |y 2014 |
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