New results on νμ → ντ appearance with the OPERA experiment in the CNGS beam

N. Agafonova; A. Aleksandrov; A. Anokhina; S. Aoki; A. Ariga; T. Ariga; T. Asada; D. Autiero; A. Badertscher; A. Ben Dhahbi; D. Bender; A. Bertolin; C. Bozza; R. Brugnera; G. Brunetti; B. Büttner; S. Buontempo; L. Chaussard; M. Chernyavskiy; V. Chiarella; A. Chukanov; L. Consiglio; N. D'Ambrosio; P. Del Amo Sanchez; G. De Lellis; M. De Serio; A. Di Crescenzo; D. Di Ferdinando; N. Di Marco; S. Dmitrievski; M. Dracos; D. Duchesneau; S. Dusini; J. Ebert; A. Ereditato; J. Favier; T. Ferber; R. A. Fini; T. Fukuda; A. Garfagnini; G. Giacomelli; C. Goellnitz; J. Goldberg; Y. Gornushkin; G. Grella; F. Grianti; A. M. Guler; C. Gustavino; C. Hagner; K. Hakamata; T. Hara; T. Hayakawa; M. Hierholzer; A. Hollnagel; B. Hosseini; H. Ishida; K. Ishiguro; M. Ishikawa; K. Jakovcic; C. Jollet; C. Kamiscioglu; M. Kamiscioglu; T. Katsuragawa; H. Kawahara; J. Kawada; J. H. Kim; S. H. Kim; M. Kimura; N. Kitagawa; B. Klicek; K. Kodama; M. Komatsu; U. Kose; I. Kreslo; A. Lauria; J. Lenkeit; A. Ljubicic; A. Longhin; P. Loverre; A. Malgin; G. Mandrioli; J. Marteau; T. Matsuo; V. Matveev; N. Mauri; E. Medinaceli; A. Meregaglia; P. Migliozzi; S. Mikado; A. Minotti; M. Miyanishi; E. Miyashita; P. Monacelli; M. C. Montesi; K. Morishima; M. T. Muciaccia; N. Naganawa; T. Naka; M. Nakamura; T. Nakano; Y. Nakatsuka; K. Niwa; S. Ogawa; N. Okateva; A. Olshevsky; T. Omura; K. Ozaki; A. Paoloni; B. D. Park; I. G. Park; A. Pastore; L. Patrizii; E. Pennacchio; H. Pessard; C. Pistillo; D. Podgrudkov; N. Polukhina; M. Pozzato; K. Pretzl; F. Pupilli; R. Rescigno; M. Roda; T. Roganova; H. Rokujo; G. Rosa; I. Rostovtseva; A. Rubbia; A. Russo; O. Ryazhskaya; O. Sato; Y. Sato; A. Schembri; W. Schmidt-Parzefall; I. Shakiryanova; T. Schcedrina; A. Sheshukov; H. Shibuya; T. Shiraishi; G. Shoziyoev; S. Simone; M. Sioli; C. Sirignano; G. Sirri; M. Spinetti; L. Stanco; N. Starkov; S. M. Stellacci; M. Stipcevic; T. Strauss; P. Strolin; K. Suzuki; S. Takahashi; M. Tenti; F. Terranova; V. Tioukov; P. Tolun; S. Tufanli; P. Vilain; M. Vladimirov; L. Votano; J. L. Vuilleumier; G. Wilquet; B. Wonsak; C. S. Yoon; J. Yoshida; M. Yoshimoto; Y. Zaitsev; S. Zemskova; A. Zghiche

doi:10.1007/JHEP11(2013)036

New results on ν_μ → ν_τ appearance with the OPERA experiment in the CNGS beam

N. Agafonova, A. Aleksandrov, A. Anokhina, S. Aoki, A. Ariga, T. Ariga, T. Asada, D. Autiero, A. Badertscher, A. Ben Dhahbi, D. Bender, A. Bertolin, C. Bozza, R. Brugnera, G. Brunetti, B. Büttner, S. Buontempo, L. Chaussard, M. Chernyavskiy, V. ChiarellaA. Chukanov, L. Consiglio, N. D'Ambrosio, P. Del Amo Sanchez, G. De Lellis, M. De Serio, A. Di Crescenzo, D. Di Ferdinando, N. Di Marco, S. Dmitrievski, M. Dracos, D. Duchesneau, S. Dusini, J. Ebert, A. Ereditato, J. Favier, T. Ferber, R. A. Fini, T. Fukuda, A. Garfagnini, G. Giacomelli, C. Goellnitz, J. Goldberg, Y. Gornushkin, G. Grella, F. Grianti, A. M. Guler, C. Gustavino, C. Hagner, K. Hakamata, T. Hara, T. Hayakawa, M. Hierholzer, A. Hollnagel, B. Hosseini, H. Ishida, K. Ishiguro, M. Ishikawa, K. Jakovcic, C. Jollet, C. Kamiscioglu, M. Kamiscioglu, T. Katsuragawa, H. Kawahara, J. Kawada, J. H. Kim, S. H. Kim, M. Kimura, N. Kitagawa, B. Klicek, K. Kodama, M. Komatsu, U. Kose, I. Kreslo, A. Lauria, J. Lenkeit, A. Ljubicic, A. Longhin, P. Loverre, A. Malgin, G. Mandrioli, J. Marteau, T. Matsuo, V. Matveev, N. Mauri, E. Medinaceli, A. Meregaglia, P. Migliozzi, S. Mikado, A. Minotti, M. Miyanishi, E. Miyashita, P. Monacelli, M. C. Montesi, K. Morishima, M. T. Muciaccia, N. Naganawa, T. Naka, M. Nakamura, T. Nakano, Y. Nakatsuka, K. Niwa, S. Ogawa, N. Okateva, A. Olshevsky, T. Omura, K. Ozaki, A. Paoloni, B. D. Park, I. G. Park, A. Pastore, L. Patrizii, E. Pennacchio, H. Pessard, C. Pistillo, D. Podgrudkov, N. Polukhina, M. Pozzato, K. Pretzl, F. Pupilli, R. Rescigno, M. Roda, T. Roganova, H. Rokujo, G. Rosa, I. Rostovtseva, A. Rubbia, A. Russo, O. Ryazhskaya, O. Sato, Y. Sato, A. Schembri, W. Schmidt-Parzefall, I. Shakiryanova, T. Schcedrina, A. Sheshukov, H. Shibuya, T. Shiraishi, G. Shoziyoev, S. Simone, M. Sioli, C. Sirignano, G. Sirri, M. Spinetti, L. Stanco, N. Starkov, S. M. Stellacci, M. Stipcevic, T. Strauss, P. Strolin, K. Suzuki, S. Takahashi, M. Tenti, F. Terranova, V. Tioukov, P. Tolun, S. Tufanli, P. Vilain, M. Vladimirov, L. Votano, J. L. Vuilleumier, G. Wilquet, B. Wonsak, C. S. Yoon, J. Yoshida, M. Yoshimoto, Y. Zaitsev, S. Zemskova, A. Zghiche

SRIS - SR Core Research Division

Research output: Contribution to journal › Review article › peer-review

74 Citations (Scopus)

Abstract

The OPERA neutrino experiment is designed to perform the first observation of neutrino oscillations in direct appearance mode in the ν_μ → ν_τ channel, via the detection of the τ-leptons created in charged current ν_τ interactions. The detector, located in the underground Gran Sasso Laboratory, consists of an emulsion/lead target with an average mass of about 1.2 kt, complemented by electronic detectors. It is exposed to the CERN Neutrinos to Gran Sasso beam, with a baseline of 730 km and a mean energy of 17GeV. The observation of the first ν_τ candidate event and the analysis of the 2008-2009 neutrino sample have been reported in previous publications. This work describes substantial improvements in the analysis and in the evaluation of the detection efficiencies and backgrounds using new simulation tools. The analysis is extended to a sub-sample of 2010 and 2011 data, resulting from an electronic detector-based pre-selection, in which an additional ν_τ candidate has been observed. The significance of the two events in terms of a ν_μ → ν_τ oscillation signal is of 2.40σ.

Original language	English
Article number	36
Journal	Journal of High Energy Physics
Volume	2013
Issue number	11
DOIs	https://doi.org/10.1007/JHEP11(2013)036
Publication status	Published - 2013 Nov

Keywords

Neutrino detectors and telescopes
Oscillation

Access to Document

10.1007/JHEP11(2013)036

Cite this

Agafonova, N., Aleksandrov, A., Anokhina, A., Aoki, S., Ariga, A., Ariga, T., Asada, T., Autiero, D., Badertscher, A., Ben Dhahbi, A., Bender, D., Bertolin, A., Bozza, C., Brugnera, R., Brunetti, G., Büttner, B., Buontempo, S., Chaussard, L., Chernyavskiy, M., ... Zghiche, A. (2013). New results on ν_μ → ν_τ appearance with the OPERA experiment in the CNGS beam. Journal of High Energy Physics, 2013(11), Article 36. https://doi.org/10.1007/JHEP11(2013)036

@article{64607a0cdd5942e1bdfb792449eaa5f2,

title = "New results on νμ → ντ appearance with the OPERA experiment in the CNGS beam",

abstract = "The OPERA neutrino experiment is designed to perform the first observation of neutrino oscillations in direct appearance mode in the νμ → ντ channel, via the detection of the τ-leptons created in charged current ντ interactions. The detector, located in the underground Gran Sasso Laboratory, consists of an emulsion/lead target with an average mass of about 1.2 kt, complemented by electronic detectors. It is exposed to the CERN Neutrinos to Gran Sasso beam, with a baseline of 730 km and a mean energy of 17GeV. The observation of the first ντ candidate event and the analysis of the 2008-2009 neutrino sample have been reported in previous publications. This work describes substantial improvements in the analysis and in the evaluation of the detection efficiencies and backgrounds using new simulation tools. The analysis is extended to a sub-sample of 2010 and 2011 data, resulting from an electronic detector-based pre-selection, in which an additional ντ candidate has been observed. The significance of the two events in terms of a νμ → ντ oscillation signal is of 2.40σ.",

keywords = "Neutrino detectors and telescopes, Oscillation",

author = "N. Agafonova and A. Aleksandrov and A. Anokhina and S. Aoki and A. Ariga and T. Ariga and T. Asada and D. Autiero and A. Badertscher and {Ben Dhahbi}, A. and D. Bender and A. Bertolin and C. Bozza and R. Brugnera and G. Brunetti and B. B{\"u}ttner and S. Buontempo and L. Chaussard and M. Chernyavskiy and V. Chiarella and A. Chukanov and L. Consiglio and N. D'Ambrosio and {Del Amo Sanchez}, P. and {De Lellis}, G. and {De Serio}, M. and {Di Crescenzo}, A. and {Di Ferdinando}, D. and {Di Marco}, N. and S. Dmitrievski and M. Dracos and D. Duchesneau and S. Dusini and J. Ebert and A. Ereditato and J. Favier and T. Ferber and Fini, {R. A.} and T. Fukuda and A. Garfagnini and G. Giacomelli and C. Goellnitz and J. Goldberg and Y. Gornushkin and G. Grella and F. Grianti and Guler, {A. M.} and C. Gustavino and C. Hagner and K. Hakamata and T. Hara and T. Hayakawa and M. Hierholzer and A. Hollnagel and B. Hosseini and H. Ishida and K. Ishiguro and M. Ishikawa and K. Jakovcic and C. Jollet and C. Kamiscioglu and M. Kamiscioglu and T. Katsuragawa and H. Kawahara and J. Kawada and Kim, {J. H.} and Kim, {S. H.} and M. Kimura and N. Kitagawa and B. Klicek and K. Kodama and M. Komatsu and U. Kose and I. Kreslo and A. Lauria and J. Lenkeit and A. Ljubicic and A. Longhin and P. Loverre and A. Malgin and G. Mandrioli and J. Marteau and T. Matsuo and V. Matveev and N. Mauri and E. Medinaceli and A. Meregaglia and P. Migliozzi and S. Mikado and A. Minotti and M. Miyanishi and E. Miyashita and P. Monacelli and Montesi, {M. C.} and K. Morishima and Muciaccia, {M. T.} and N. Naganawa and T. Naka and M. Nakamura and T. Nakano and Y. Nakatsuka and K. Niwa and S. Ogawa and N. Okateva and A. Olshevsky and T. Omura and K. Ozaki and A. Paoloni and Park, {B. D.} and Park, {I. G.} and A. Pastore and L. Patrizii and E. Pennacchio and H. Pessard and C. Pistillo and D. Podgrudkov and N. Polukhina and M. Pozzato and K. Pretzl and F. Pupilli and R. Rescigno and M. Roda and T. Roganova and H. Rokujo and G. Rosa and I. Rostovtseva and A. Rubbia and A. Russo and O. Ryazhskaya and O. Sato and Y. Sato and A. Schembri and W. Schmidt-Parzefall and I. Shakiryanova and T. Schcedrina and A. Sheshukov and H. Shibuya and T. Shiraishi and G. Shoziyoev and S. Simone and M. Sioli and C. Sirignano and G. Sirri and M. Spinetti and L. Stanco and N. Starkov and Stellacci, {S. M.} and M. Stipcevic and T. Strauss and P. Strolin and K. Suzuki and S. Takahashi and M. Tenti and F. Terranova and V. Tioukov and P. Tolun and S. Tufanli and P. Vilain and M. Vladimirov and L. Votano and Vuilleumier, {J. L.} and G. Wilquet and B. Wonsak and Yoon, {C. S.} and J. Yoshida and M. Yoshimoto and Y. Zaitsev and S. Zemskova and A. Zghiche",

year = "2013",

month = nov,

doi = "10.1007/JHEP11(2013)036",

language = "English",

volume = "2013",

journal = "Journal of High Energy Physics",

issn = "1029-8479",

publisher = "Springer Verlag",

number = "11",

}

Agafonova, N, Aleksandrov, A, Anokhina, A, Aoki, S, Ariga, A, Ariga, T, Asada, T, Autiero, D, Badertscher, A, Ben Dhahbi, A, Bender, D, Bertolin, A, Bozza, C, Brugnera, R, Brunetti, G, Büttner, B, Buontempo, S, Chaussard, L, Chernyavskiy, M, Chiarella, V, Chukanov, A, Consiglio, L, D'Ambrosio, N, Del Amo Sanchez, P, De Lellis, G, De Serio, M, Di Crescenzo, A, Di Ferdinando, D, Di Marco, N, Dmitrievski, S, Dracos, M, Duchesneau, D, Dusini, S, Ebert, J, Ereditato, A, Favier, J, Ferber, T, Fini, RA, Fukuda, T, Garfagnini, A, Giacomelli, G, Goellnitz, C, Goldberg, J, Gornushkin, Y, Grella, G, Grianti, F, Guler, AM, Gustavino, C, Hagner, C, Hakamata, K, Hara, T, Hayakawa, T, Hierholzer, M, Hollnagel, A, Hosseini, B, Ishida, H, Ishiguro, K, Ishikawa, M, Jakovcic, K, Jollet, C, Kamiscioglu, C, Kamiscioglu, M, Katsuragawa, T, Kawahara, H, Kawada, J, Kim, JH, Kim, SH, Kimura, M, Kitagawa, N, Klicek, B, Kodama, K, Komatsu, M, Kose, U, Kreslo, I, Lauria, A, Lenkeit, J, Ljubicic, A, Longhin, A, Loverre, P, Malgin, A, Mandrioli, G, Marteau, J, Matsuo, T, Matveev, V, Mauri, N, Medinaceli, E, Meregaglia, A, Migliozzi, P, Mikado, S, Minotti, A, Miyanishi, M, Miyashita, E, Monacelli, P, Montesi, MC, Morishima, K, Muciaccia, MT, Naganawa, N, Naka, T, Nakamura, M, Nakano, T, Nakatsuka, Y, Niwa, K, Ogawa, S, Okateva, N, Olshevsky, A, Omura, T, Ozaki, K, Paoloni, A, Park, BD, Park, IG, Pastore, A, Patrizii, L, Pennacchio, E, Pessard, H, Pistillo, C, Podgrudkov, D, Polukhina, N, Pozzato, M, Pretzl, K, Pupilli, F, Rescigno, R, Roda, M, Roganova, T, Rokujo, H, Rosa, G, Rostovtseva, I, Rubbia, A, Russo, A, Ryazhskaya, O, Sato, O, Sato, Y, Schembri, A, Schmidt-Parzefall, W, Shakiryanova, I, Schcedrina, T, Sheshukov, A, Shibuya, H, Shiraishi, T, Shoziyoev, G, Simone, S, Sioli, M, Sirignano, C, Sirri, G, Spinetti, M, Stanco, L, Starkov, N, Stellacci, SM, Stipcevic, M, Strauss, T, Strolin, P, Suzuki, K, Takahashi, S, Tenti, M, Terranova, F, Tioukov, V, Tolun, P, Tufanli, S, Vilain, P, Vladimirov, M, Votano, L, Vuilleumier, JL, Wilquet, G, Wonsak, B, Yoon, CS, Yoshida, J, Yoshimoto, M, Zaitsev, Y, Zemskova, S & Zghiche, A 2013, 'New results on ν_μ → ν_τ appearance with the OPERA experiment in the CNGS beam', Journal of High Energy Physics, vol. 2013, no. 11, 36. https://doi.org/10.1007/JHEP11(2013)036

TY - JOUR

T1 - New results on νμ → ντ appearance with the OPERA experiment in the CNGS beam

AU - Agafonova, N.

AU - Aleksandrov, A.

AU - Anokhina, A.

AU - Aoki, S.

AU - Ariga, A.

AU - Ariga, T.

AU - Asada, T.

AU - Autiero, D.

AU - Badertscher, A.

AU - Ben Dhahbi, A.

AU - Bender, D.

AU - Bertolin, A.

AU - Bozza, C.

AU - Brugnera, R.

AU - Brunetti, G.

AU - Büttner, B.

AU - Buontempo, S.

AU - Chaussard, L.

AU - Chernyavskiy, M.

AU - Chiarella, V.

AU - Chukanov, A.

AU - Consiglio, L.

AU - D'Ambrosio, N.

AU - Del Amo Sanchez, P.

AU - De Lellis, G.

AU - De Serio, M.

AU - Di Crescenzo, A.

AU - Di Ferdinando, D.

AU - Di Marco, N.

AU - Dmitrievski, S.

AU - Dracos, M.

AU - Duchesneau, D.

AU - Dusini, S.

AU - Ebert, J.

AU - Ereditato, A.

AU - Favier, J.

AU - Ferber, T.

AU - Fini, R. A.

AU - Fukuda, T.

AU - Garfagnini, A.

AU - Giacomelli, G.

AU - Goellnitz, C.

AU - Goldberg, J.

AU - Gornushkin, Y.

AU - Grella, G.

AU - Grianti, F.

AU - Guler, A. M.

AU - Gustavino, C.

AU - Hagner, C.

AU - Hakamata, K.

AU - Hara, T.

AU - Hayakawa, T.

AU - Hierholzer, M.

AU - Hollnagel, A.

AU - Hosseini, B.

AU - Ishida, H.

AU - Ishiguro, K.

AU - Ishikawa, M.

AU - Jakovcic, K.

AU - Jollet, C.

AU - Kamiscioglu, C.

AU - Kamiscioglu, M.

AU - Katsuragawa, T.

AU - Kawahara, H.

AU - Kawada, J.

AU - Kim, J. H.

AU - Kim, S. H.

AU - Kimura, M.

AU - Kitagawa, N.

AU - Klicek, B.

AU - Kodama, K.

AU - Komatsu, M.

AU - Kose, U.

AU - Kreslo, I.

AU - Lauria, A.

AU - Lenkeit, J.

AU - Ljubicic, A.

AU - Longhin, A.

AU - Loverre, P.

AU - Malgin, A.

AU - Mandrioli, G.

AU - Marteau, J.

AU - Matsuo, T.

AU - Matveev, V.

AU - Mauri, N.

AU - Medinaceli, E.

AU - Meregaglia, A.

AU - Migliozzi, P.

AU - Mikado, S.

AU - Minotti, A.

AU - Miyanishi, M.

AU - Miyashita, E.

AU - Monacelli, P.

AU - Montesi, M. C.

AU - Morishima, K.

AU - Muciaccia, M. T.

AU - Naganawa, N.

AU - Naka, T.

AU - Nakamura, M.

AU - Nakano, T.

AU - Nakatsuka, Y.

AU - Niwa, K.

AU - Ogawa, S.

AU - Okateva, N.

AU - Olshevsky, A.

AU - Omura, T.

AU - Ozaki, K.

AU - Paoloni, A.

AU - Park, B. D.

AU - Park, I. G.

AU - Pastore, A.

AU - Patrizii, L.

AU - Pennacchio, E.

AU - Pessard, H.

AU - Pistillo, C.

AU - Podgrudkov, D.

AU - Polukhina, N.

AU - Pozzato, M.

AU - Pretzl, K.

AU - Pupilli, F.

AU - Rescigno, R.

AU - Roda, M.

AU - Roganova, T.

AU - Rokujo, H.

AU - Rosa, G.

AU - Rostovtseva, I.

AU - Rubbia, A.

AU - Russo, A.

AU - Ryazhskaya, O.

AU - Sato, O.

AU - Sato, Y.

AU - Schembri, A.

AU - Schmidt-Parzefall, W.

AU - Shakiryanova, I.

AU - Schcedrina, T.

AU - Sheshukov, A.

AU - Shibuya, H.

AU - Shiraishi, T.

AU - Shoziyoev, G.

AU - Simone, S.

AU - Sioli, M.

AU - Sirignano, C.

AU - Sirri, G.

AU - Spinetti, M.

AU - Stanco, L.

AU - Starkov, N.

AU - Stellacci, S. M.

AU - Stipcevic, M.

AU - Strauss, T.

AU - Strolin, P.

AU - Suzuki, K.

AU - Takahashi, S.

AU - Tenti, M.

AU - Terranova, F.

AU - Tioukov, V.

AU - Tolun, P.

AU - Tufanli, S.

AU - Vilain, P.

AU - Vladimirov, M.

AU - Votano, L.

AU - Vuilleumier, J. L.

AU - Wilquet, G.

AU - Wonsak, B.

AU - Yoon, C. S.

AU - Yoshida, J.

AU - Yoshimoto, M.

AU - Zaitsev, Y.

AU - Zemskova, S.

AU - Zghiche, A.

PY - 2013/11

Y1 - 2013/11

N2 - The OPERA neutrino experiment is designed to perform the first observation of neutrino oscillations in direct appearance mode in the νμ → ντ channel, via the detection of the τ-leptons created in charged current ντ interactions. The detector, located in the underground Gran Sasso Laboratory, consists of an emulsion/lead target with an average mass of about 1.2 kt, complemented by electronic detectors. It is exposed to the CERN Neutrinos to Gran Sasso beam, with a baseline of 730 km and a mean energy of 17GeV. The observation of the first ντ candidate event and the analysis of the 2008-2009 neutrino sample have been reported in previous publications. This work describes substantial improvements in the analysis and in the evaluation of the detection efficiencies and backgrounds using new simulation tools. The analysis is extended to a sub-sample of 2010 and 2011 data, resulting from an electronic detector-based pre-selection, in which an additional ντ candidate has been observed. The significance of the two events in terms of a νμ → ντ oscillation signal is of 2.40σ.

AB - The OPERA neutrino experiment is designed to perform the first observation of neutrino oscillations in direct appearance mode in the νμ → ντ channel, via the detection of the τ-leptons created in charged current ντ interactions. The detector, located in the underground Gran Sasso Laboratory, consists of an emulsion/lead target with an average mass of about 1.2 kt, complemented by electronic detectors. It is exposed to the CERN Neutrinos to Gran Sasso beam, with a baseline of 730 km and a mean energy of 17GeV. The observation of the first ντ candidate event and the analysis of the 2008-2009 neutrino sample have been reported in previous publications. This work describes substantial improvements in the analysis and in the evaluation of the detection efficiencies and backgrounds using new simulation tools. The analysis is extended to a sub-sample of 2010 and 2011 data, resulting from an electronic detector-based pre-selection, in which an additional ντ candidate has been observed. The significance of the two events in terms of a νμ → ντ oscillation signal is of 2.40σ.

KW - Neutrino detectors and telescopes

KW - Oscillation

UR - http://www.scopus.com/inward/record.url?scp=84893056114&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=84893056114&partnerID=8YFLogxK

U2 - 10.1007/JHEP11(2013)036

DO - 10.1007/JHEP11(2013)036

M3 - Review article

AN - SCOPUS:84893056114

SN - 1029-8479

VL - 2013

JO - Journal of High Energy Physics

JF - Journal of High Energy Physics

IS - 11

M1 - 36

ER -

New results on ν_μ → ν_τ appearance with the OPERA experiment in the CNGS beam

Abstract

Keywords

Access to Document

Other files and links

Fingerprint

Cite this