Cosmic Ray Background Removal With Deep Neural Networks in SBND

R. Acciarri; C. Adams; C. Andreopoulos; J. Asaadi; M. Babicz; C. Backhouse; W. Badgett; L. Bagby; D. Barker; V. Basque; M. C.Q. Bazetto; M. Betancourt; A. Bhanderi; A. Bhat; C. Bonifazi; D. Brailsford; A. G. Brandt; T. Brooks; M. F. Carneiro; Y. Chen; H. Chen; G. Chisnall; J. I. Crespo-Anadón; E. Cristaldo; C. Cuesta; I. L. de Icaza Astiz; A. De Roeck; G. de Sá Pereira; M. Del Tutto; V. Di Benedetto; A. Ereditato; J. J. Evans; A. C. Ezeribe; R. S. Fitzpatrick; B. T. Fleming; W. Foreman; D. Franco; I. Furic; A. P. Furmanski; S. Gao; D. Garcia-Gamez; H. Frandini; G. Ge; I. Gil-Botella; S. Gollapinni; O. Goodwin; P. Green; W. C. Griffith; R. Guenette; P. Guzowski; T. Ham; J. Henzerling; A. Holin; B. Howard; R. S. Jones; D. Kalra; G. Karagiorgi; L. Kashur; W. Ketchum; M. J. Kim; V. A. Kudryavtsev; J. Larkin; H. Lay; I. Lepetic; B. R. Littlejohn; W. C. Louis; A. A. Machado; M. Malek; D. Mardsen; C. Mariani; F. Marinho; A. Mastbaum; K. Mavrokoridis; N. McConkey; V. Meddage; D. P. Méndez; T. Mettler; K. Mistry; A. Mogan; J. Molina; M. Mooney; L. Mora; C. A. Moura; J. Mousseau; A. Navrer-Agasson; F. J. Nicolas-Arnaldos; J. A. Nowak; O. Palamara; V. Pandey; J. Pater; L. Paulucci; V. L. Pimentel; F. Psihas; G. Putnam; X. Qian; E. Raguzin; H. Ray; M. Reggiani-Guzzo; D. Rivera; M. Roda; M. Ross-Lonergan; G. Scanavini; A. Scarff; D. W. Schmitz; A. Schukraft; E. Segreto; M. Soares Nunes; M. Soderberg; S. Söldner-Rembold; J. Spitz; N. J.C. Spooner; M. Stancari; G. V. Stenico; A. Szelc; W. Tang; J. Tena Vidal; D. Torretta; M. Toups; C. Touramanis; M. Tripathi; S. Tufanli; E. Tyley; G. A. Valdiviesso; E. Worcester; M. Worcester; G. Yarbrough; J. Yu; B. Zamorano; J. Zennamo; A. Zglam

doi:10.3389/frai.2021.649917

Cosmic Ray Background Removal With Deep Neural Networks in SBND

R. Acciarri, C. Adams, C. Andreopoulos, J. Asaadi, M. Babicz, C. Backhouse, W. Badgett, L. Bagby, D. Barker, V. Basque, M. C.Q. Bazetto, M. Betancourt, A. Bhanderi, A. Bhat, C. Bonifazi, D. Brailsford, A. G. Brandt, T. Brooks, M. F. Carneiro, Y. ChenH. Chen, G. Chisnall, J. I. Crespo-Anadón, E. Cristaldo, C. Cuesta, I. L. de Icaza Astiz, A. De Roeck, G. de Sá Pereira, M. Del Tutto, V. Di Benedetto, A. Ereditato, J. J. Evans, A. C. Ezeribe, R. S. Fitzpatrick, B. T. Fleming, W. Foreman, D. Franco, I. Furic, A. P. Furmanski, S. Gao, D. Garcia-Gamez, H. Frandini, G. Ge, I. Gil-Botella, S. Gollapinni, O. Goodwin, P. Green, W. C. Griffith, R. Guenette, P. Guzowski, T. Ham, J. Henzerling, A. Holin, B. Howard, R. S. Jones, D. Kalra, G. Karagiorgi, L. Kashur, W. Ketchum, M. J. Kim, V. A. Kudryavtsev, J. Larkin, H. Lay, I. Lepetic, B. R. Littlejohn, W. C. Louis, A. A. Machado, M. Malek, D. Mardsen, C. Mariani, F. Marinho, A. Mastbaum, K. Mavrokoridis, N. McConkey, V. Meddage, D. P. Méndez, T. Mettler, K. Mistry, A. Mogan, J. Molina, M. Mooney, L. Mora, C. A. Moura, J. Mousseau, A. Navrer-Agasson, F. J. Nicolas-Arnaldos, J. A. Nowak, O. Palamara, V. Pandey, J. Pater, L. Paulucci, V. L. Pimentel, F. Psihas, G. Putnam, X. Qian, E. Raguzin, H. Ray, M. Reggiani-Guzzo, D. Rivera, M. Roda, M. Ross-Lonergan, G. Scanavini, A. Scarff, D. W. Schmitz, A. Schukraft, E. Segreto, M. Soares Nunes, M. Soderberg, S. Söldner-Rembold, J. Spitz, N. J.C. Spooner, M. Stancari, G. V. Stenico, A. Szelc, W. Tang, J. Tena Vidal, D. Torretta, M. Toups, C. Touramanis, M. Tripathi, S. Tufanli, E. Tyley, G. A. Valdiviesso, E. Worcester, M. Worcester, G. Yarbrough, J. Yu, B. Zamorano, J. Zennamo, A. Zglam

Physics

Producción científica: Contribución a una revista › Artículo › revisión exhaustiva

6 Citas (Scopus)

Resumen

In liquid argon time projection chambers exposed to neutrino beams and running on or near surface levels, cosmic muons, and other cosmic particles are incident on the detectors while a single neutrino-induced event is being recorded. In practice, this means that data from surface liquid argon time projection chambers will be dominated by cosmic particles, both as a source of event triggers and as the majority of the particle count in true neutrino-triggered events. In this work, we demonstrate a novel application of deep learning techniques to remove these background particles by applying deep learning on full detector images from the SBND detector, the near detector in the Fermilab Short-Baseline Neutrino Program. We use this technique to identify, on a pixel-by-pixel level, whether recorded activity originated from cosmic particles or neutrino interactions.

Idioma original	Inglés
Número de artículo	649917
Publicación	Frontiers in Artificial Intelligence
Volumen	4
DOI	https://doi.org/10.3389/frai.2021.649917
Estado	Publicada - ago. 24 2021

Nota bibliográfica

Publisher Copyright:
© 2021 Acciarri, Adams, Andreopoulos, Asaadi.

!!!ASJC Scopus Subject Areas

Inteligencia artificial

Acceder al documento

10.3389/frai.2021.649917

Otros archivos y enlaces

Citar esto

Acciarri, R., Adams, C., Andreopoulos, C., Asaadi, J., Babicz, M., Backhouse, C., Badgett, W., Bagby, L., Barker, D., Basque, V., Bazetto, M. C. Q., Betancourt, M., Bhanderi, A., Bhat, A., Bonifazi, C., Brailsford, D., Brandt, A. G., Brooks, T., Carneiro, M. F., ... Zglam, A. (2021). Cosmic Ray Background Removal With Deep Neural Networks in SBND. Frontiers in Artificial Intelligence, 4, Artículo 649917. https://doi.org/10.3389/frai.2021.649917

@article{fcad6a5d3121428e8b06a8066a0518f0,

title = "Cosmic Ray Background Removal With Deep Neural Networks in SBND",

abstract = "In liquid argon time projection chambers exposed to neutrino beams and running on or near surface levels, cosmic muons, and other cosmic particles are incident on the detectors while a single neutrino-induced event is being recorded. In practice, this means that data from surface liquid argon time projection chambers will be dominated by cosmic particles, both as a source of event triggers and as the majority of the particle count in true neutrino-triggered events. In this work, we demonstrate a novel application of deep learning techniques to remove these background particles by applying deep learning on full detector images from the SBND detector, the near detector in the Fermilab Short-Baseline Neutrino Program. We use this technique to identify, on a pixel-by-pixel level, whether recorded activity originated from cosmic particles or neutrino interactions.",

keywords = "SBN program, SBND, UNet, deep learning, liquid Ar detectors, neutrino physics",

author = "R. Acciarri and C. Adams and C. Andreopoulos and J. Asaadi and M. Babicz and C. Backhouse and W. Badgett and L. Bagby and D. Barker and V. Basque and Bazetto, {M. C.Q.} and M. Betancourt and A. Bhanderi and A. Bhat and C. Bonifazi and D. Brailsford and Brandt, {A. G.} and T. Brooks and Carneiro, {M. F.} and Y. Chen and H. Chen and G. Chisnall and Crespo-Anad{\'o}n, {J. I.} and E. Cristaldo and C. Cuesta and {de Icaza Astiz}, {I. L.} and {De Roeck}, A. and {de S{\'a} Pereira}, G. and {Del Tutto}, M. and {Di Benedetto}, V. and A. Ereditato and Evans, {J. J.} and Ezeribe, {A. C.} and Fitzpatrick, {R. S.} and Fleming, {B. T.} and W. Foreman and D. Franco and I. Furic and Furmanski, {A. P.} and S. Gao and D. Garcia-Gamez and H. Frandini and G. Ge and I. Gil-Botella and S. Gollapinni and O. Goodwin and P. Green and Griffith, {W. C.} and R. Guenette and P. Guzowski and T. Ham and J. Henzerling and A. Holin and B. Howard and Jones, {R. S.} and D. Kalra and G. Karagiorgi and L. Kashur and W. Ketchum and Kim, {M. J.} and Kudryavtsev, {V. A.} and J. Larkin and H. Lay and I. Lepetic and Littlejohn, {B. R.} and Louis, {W. C.} and Machado, {A. A.} and M. Malek and D. Mardsen and C. Mariani and F. Marinho and A. Mastbaum and K. Mavrokoridis and N. McConkey and V. Meddage and M{\'e}ndez, {D. P.} and T. Mettler and K. Mistry and A. Mogan and J. Molina and M. Mooney and L. Mora and Moura, {C. A.} and J. Mousseau and A. Navrer-Agasson and Nicolas-Arnaldos, {F. J.} and Nowak, {J. A.} and O. Palamara and V. Pandey and J. Pater and L. Paulucci and Pimentel, {V. L.} and F. Psihas and G. Putnam and X. Qian and E. Raguzin and H. Ray and M. Reggiani-Guzzo and D. Rivera and M. Roda and M. Ross-Lonergan and G. Scanavini and A. Scarff and Schmitz, {D. W.} and A. Schukraft and E. Segreto and {Soares Nunes}, M. and M. Soderberg and S. S{\"o}ldner-Rembold and J. Spitz and Spooner, {N. J.C.} and M. Stancari and Stenico, {G. V.} and A. Szelc and W. Tang and {Tena Vidal}, J. and D. Torretta and M. Toups and C. Touramanis and M. Tripathi and S. Tufanli and E. Tyley and Valdiviesso, {G. A.} and E. Worcester and M. Worcester and G. Yarbrough and J. Yu and B. Zamorano and J. Zennamo and A. Zglam",

note = "Publisher Copyright: {\textcopyright} 2021 Acciarri, Adams, Andreopoulos, Asaadi.",

year = "2021",

month = aug,

day = "24",

doi = "10.3389/frai.2021.649917",

language = "English",

volume = "4",

journal = "Frontiers in Artificial Intelligence",

issn = "2624-8212",

publisher = "Frontiers Media",

}

Acciarri, R, Adams, C, Andreopoulos, C, Asaadi, J, Babicz, M, Backhouse, C, Badgett, W, Bagby, L, Barker, D, Basque, V, Bazetto, MCQ, Betancourt, M, Bhanderi, A, Bhat, A, Bonifazi, C, Brailsford, D, Brandt, AG, Brooks, T, Carneiro, MF, Chen, Y, Chen, H, Chisnall, G, Crespo-Anadón, JI, Cristaldo, E, Cuesta, C, de Icaza Astiz, IL, De Roeck, A, de Sá Pereira, G, Del Tutto, M, Di Benedetto, V, Ereditato, A, Evans, JJ, Ezeribe, AC, Fitzpatrick, RS, Fleming, BT, Foreman, W, Franco, D, Furic, I, Furmanski, AP, Gao, S, Garcia-Gamez, D, Frandini, H, Ge, G, Gil-Botella, I, Gollapinni, S, Goodwin, O, Green, P, Griffith, WC, Guenette, R, Guzowski, P, Ham, T, Henzerling, J, Holin, A, Howard, B, Jones, RS, Kalra, D, Karagiorgi, G, Kashur, L, Ketchum, W, Kim, MJ, Kudryavtsev, VA, Larkin, J, Lay, H, Lepetic, I, Littlejohn, BR, Louis, WC, Machado, AA, Malek, M, Mardsen, D, Mariani, C, Marinho, F, Mastbaum, A, Mavrokoridis, K, McConkey, N, Meddage, V, Méndez, DP, Mettler, T, Mistry, K, Mogan, A, Molina, J, Mooney, M, Mora, L, Moura, CA, Mousseau, J, Navrer-Agasson, A, Nicolas-Arnaldos, FJ, Nowak, JA, Palamara, O, Pandey, V, Pater, J, Paulucci, L, Pimentel, VL, Psihas, F, Putnam, G, Qian, X, Raguzin, E, Ray, H, Reggiani-Guzzo, M, Rivera, D, Roda, M, Ross-Lonergan, M, Scanavini, G, Scarff, A, Schmitz, DW, Schukraft, A, Segreto, E, Soares Nunes, M, Soderberg, M, Söldner-Rembold, S, Spitz, J, Spooner, NJC, Stancari, M, Stenico, GV, Szelc, A, Tang, W, Tena Vidal, J, Torretta, D, Toups, M, Touramanis, C, Tripathi, M, Tufanli, S, Tyley, E, Valdiviesso, GA, Worcester, E, Worcester, M, Yarbrough, G, Yu, J, Zamorano, B, Zennamo, J & Zglam, A 2021, 'Cosmic Ray Background Removal With Deep Neural Networks in SBND', Frontiers in Artificial Intelligence, vol. 4, 649917. https://doi.org/10.3389/frai.2021.649917

TY - JOUR

T1 - Cosmic Ray Background Removal With Deep Neural Networks in SBND

AU - Acciarri, R.

AU - Adams, C.

AU - Andreopoulos, C.

AU - Asaadi, J.

AU - Babicz, M.

AU - Backhouse, C.

AU - Badgett, W.

AU - Bagby, L.

AU - Barker, D.

AU - Basque, V.

AU - Bazetto, M. C.Q.

AU - Betancourt, M.

AU - Bhanderi, A.

AU - Bhat, A.

AU - Bonifazi, C.

AU - Brailsford, D.

AU - Brandt, A. G.

AU - Brooks, T.

AU - Carneiro, M. F.

AU - Chen, Y.

AU - Chen, H.

AU - Chisnall, G.

AU - Crespo-Anadón, J. I.

AU - Cristaldo, E.

AU - Cuesta, C.

AU - de Icaza Astiz, I. L.

AU - De Roeck, A.

AU - de Sá Pereira, G.

AU - Del Tutto, M.

AU - Di Benedetto, V.

AU - Ereditato, A.

AU - Evans, J. J.

AU - Ezeribe, A. C.

AU - Fitzpatrick, R. S.

AU - Fleming, B. T.

AU - Foreman, W.

AU - Franco, D.

AU - Furic, I.

AU - Furmanski, A. P.

AU - Gao, S.

AU - Garcia-Gamez, D.

AU - Frandini, H.

AU - Ge, G.

AU - Gil-Botella, I.

AU - Gollapinni, S.

AU - Goodwin, O.

AU - Green, P.

AU - Griffith, W. C.

AU - Guenette, R.

AU - Guzowski, P.

AU - Ham, T.

AU - Henzerling, J.

AU - Holin, A.

AU - Howard, B.

AU - Jones, R. S.

AU - Kalra, D.

AU - Karagiorgi, G.

AU - Kashur, L.

AU - Ketchum, W.

AU - Kim, M. J.

AU - Kudryavtsev, V. A.

AU - Larkin, J.

AU - Lay, H.

AU - Lepetic, I.

AU - Littlejohn, B. R.

AU - Louis, W. C.

AU - Machado, A. A.

AU - Malek, M.

AU - Mardsen, D.

AU - Mariani, C.

AU - Marinho, F.

AU - Mastbaum, A.

AU - Mavrokoridis, K.

AU - McConkey, N.

AU - Meddage, V.

AU - Méndez, D. P.

AU - Mettler, T.

AU - Mistry, K.

AU - Mogan, A.

AU - Molina, J.

AU - Mooney, M.

AU - Mora, L.

AU - Moura, C. A.

AU - Mousseau, J.

AU - Navrer-Agasson, A.

AU - Nicolas-Arnaldos, F. J.

AU - Nowak, J. A.

AU - Palamara, O.

AU - Pandey, V.

AU - Pater, J.

AU - Paulucci, L.

AU - Pimentel, V. L.

AU - Psihas, F.

AU - Putnam, G.

AU - Qian, X.

AU - Raguzin, E.

AU - Ray, H.

AU - Reggiani-Guzzo, M.

AU - Rivera, D.

AU - Roda, M.

AU - Ross-Lonergan, M.

AU - Scanavini, G.

AU - Scarff, A.

AU - Schmitz, D. W.

AU - Schukraft, A.

AU - Segreto, E.

AU - Soares Nunes, M.

AU - Soderberg, M.

AU - Söldner-Rembold, S.

AU - Spitz, J.

AU - Spooner, N. J.C.

AU - Stancari, M.

AU - Stenico, G. V.

AU - Szelc, A.

AU - Tang, W.

AU - Tena Vidal, J.

AU - Torretta, D.

AU - Toups, M.

AU - Touramanis, C.

AU - Tripathi, M.

AU - Tufanli, S.

AU - Tyley, E.

AU - Valdiviesso, G. A.

AU - Worcester, E.

AU - Worcester, M.

AU - Yarbrough, G.

AU - Yu, J.

AU - Zamorano, B.

AU - Zennamo, J.

AU - Zglam, A.

PY - 2021/8/24

Y1 - 2021/8/24

N2 - In liquid argon time projection chambers exposed to neutrino beams and running on or near surface levels, cosmic muons, and other cosmic particles are incident on the detectors while a single neutrino-induced event is being recorded. In practice, this means that data from surface liquid argon time projection chambers will be dominated by cosmic particles, both as a source of event triggers and as the majority of the particle count in true neutrino-triggered events. In this work, we demonstrate a novel application of deep learning techniques to remove these background particles by applying deep learning on full detector images from the SBND detector, the near detector in the Fermilab Short-Baseline Neutrino Program. We use this technique to identify, on a pixel-by-pixel level, whether recorded activity originated from cosmic particles or neutrino interactions.

AB - In liquid argon time projection chambers exposed to neutrino beams and running on or near surface levels, cosmic muons, and other cosmic particles are incident on the detectors while a single neutrino-induced event is being recorded. In practice, this means that data from surface liquid argon time projection chambers will be dominated by cosmic particles, both as a source of event triggers and as the majority of the particle count in true neutrino-triggered events. In this work, we demonstrate a novel application of deep learning techniques to remove these background particles by applying deep learning on full detector images from the SBND detector, the near detector in the Fermilab Short-Baseline Neutrino Program. We use this technique to identify, on a pixel-by-pixel level, whether recorded activity originated from cosmic particles or neutrino interactions.

KW - SBN program

KW - SBND

KW - UNet

KW - deep learning

KW - liquid Ar detectors

KW - neutrino physics

UR - http://www.scopus.com/inward/record.url?scp=85118213576&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=85118213576&partnerID=8YFLogxK

U2 - 10.3389/frai.2021.649917

DO - 10.3389/frai.2021.649917

M3 - Article

AN - SCOPUS:85118213576

SN - 2624-8212

VL - 4

JO - Frontiers in Artificial Intelligence

JF - Frontiers in Artificial Intelligence

M1 - 649917

ER -

Cosmic Ray Background Removal With Deep Neural Networks in SBND

Resumen

Nota bibliográfica

!!!ASJC Scopus Subject Areas

Acceder al documento

Otros archivos y enlaces

Huella

Citar esto