VUV-Sensitive Silicon Photomultipliers for Xenon Scintillation Light Detection in nEXO

A. Jamil; T. Ziegler; P. Hufschmidt; G. Li; L. Lupin-Jimenez; T. Michel; I. Ostrovskiy; F. Retière; J. Schneider; M. Wagenpfeil; A. Alamre; J. B. Albert; G. Anton; I. J. Arnquist; I. Badhrees; P. S. Barbeau; D. Beck; V. Belov; T. Bhatta; F. Bourque; J. P. Brodsky; E. Brown; T. Brunner; A. Burenkov; G. F. Cao; L. Cao; W. R. Cen; C. Chambers; S. A. Charlebois; M. Chiu; B. Cleveland; M. Coon; M. Côté; A. Craycraft; W. Cree; J. Dalmasson; T. Daniels; L. Darroch; S. J. Daugherty; J. Daughhetee; S. Delaquis; A. Der Mesrobian-Kabakian; R. DeVoe; J. Dilling; Y. Y. Ding; M. J. Dolinski; A. Dragone; J. Echevers; L. Fabris; D. Fairbank; W. Fairbank; J. Farine; S. Feyzbakhsh; R. Fontaine; D. Fudenberg; G. Gallina; G. Giacomini; R. Gornea; G. Gratta; E. V. Hansen; D. Harris; M. Hasan; M. Heffner; J. Hößl; E. W. Hoppe; A. House; M. Hughes; Y. Ito; A. Iverson; C. Jessiman; M. J. Jewell; X. S. Jiang; A. Karelin; L. J. Kaufman; T. Koffas; S. Kravitz; R. Krücken; A. Kuchenkov; K. S. Kumar; Y. Lan; A. Larson; D. S. Leonard; S. Li; Z. Li; C. Licciardi; Y. H. Lin; P. Lv; R. MacLellan; B. Mong; D. C. Moore; K. Murray; R. J. Newby; Z. Ning; O. Njoya; F. Nolet; O. Nusair; K. Odgers; A. Odian; M. Oriunno; J. L. Orrell; G. S. Ortega; C. T. Overman; S. Parent; A. Piepke; A. Pocar; J. F. Pratte; D. Qiu; V. Radeka; E. Raguzin; T. Rao; S. Rescia; A. Robinson; T. Rossignol; P. C. Rowson; N. Roy; R. Saldanha; S. Sangiorgio; S. Schmidt; A. Schubert; D. Sinclair; K. Skarpaas; A. K. Soma; G. St-Hilaire; V. Stekhanov; T. Stiegler; X. L. Sun; M. Tarka; J. Todd; T. Tolba; T. I. Totev; R. Tsang; T. Tsang; F. Vachon; B. Veenstra; V. Veeraraghavan; G. Visser; J. L. Vuilleumier; Q. Wang; J. Watkins; M. Weber; W. Wei; L. J. Wen; U. Wichoski; G. Wrede; S. X. Wu; W. H. Wu; Q. Xia; L. Yang; Y. R. Yen; O. Zeldovich; X. Zhang; J. Zhao; Y. Zhou

doi:10.1109/TNS.2018.2875668

VUV-Sensitive Silicon Photomultipliers for Xenon Scintillation Light Detection in nEXO

A. Jamil, T. Ziegler, P. Hufschmidt, G. Li, L. Lupin-Jimenez, T. Michel, I. Ostrovskiy, F. Retière, J. Schneider, M. Wagenpfeil, A. Alamre, J. B. Albert, G. Anton, I. J. Arnquist, I. Badhrees, P. S. Barbeau, D. Beck, V. Belov, T. Bhatta, F. BourqueJ. P. Brodsky, E. Brown, T. Brunner, A. Burenkov, G. F. Cao, L. Cao, W. R. Cen, C. Chambers, S. A. Charlebois, M. Chiu, B. Cleveland, M. Coon, M. Côté, A. Craycraft, W. Cree, J. Dalmasson, T. Daniels, L. Darroch, S. J. Daugherty, J. Daughhetee, S. Delaquis, A. Der Mesrobian-Kabakian, R. DeVoe, J. Dilling, Y. Y. Ding, M. J. Dolinski, A. Dragone, J. Echevers, L. Fabris, D. Fairbank, W. Fairbank, J. Farine, S. Feyzbakhsh, R. Fontaine, D. Fudenberg, G. Gallina, G. Giacomini, R. Gornea, G. Gratta, E. V. Hansen, D. Harris, M. Hasan, M. Heffner, J. Hößl, E. W. Hoppe, A. House, M. Hughes, Y. Ito, A. Iverson, C. Jessiman, M. J. Jewell, X. S. Jiang, A. Karelin, L. J. Kaufman, T. Koffas, S. Kravitz, R. Krücken, A. Kuchenkov, K. S. Kumar, Y. Lan, A. Larson, D. S. Leonard, S. Li, Z. Li, C. Licciardi, Y. H. Lin, P. Lv, R. MacLellan, B. Mong, D. C. Moore, K. Murray, R. J. Newby, Z. Ning, O. Njoya, F. Nolet, O. Nusair, K. Odgers, A. Odian, M. Oriunno, J. L. Orrell, G. S. Ortega, C. T. Overman, S. Parent, A. Piepke, A. Pocar, J. F. Pratte, D. Qiu, V. Radeka, E. Raguzin, T. Rao, S. Rescia, A. Robinson, T. Rossignol, P. C. Rowson, N. Roy, R. Saldanha, S. Sangiorgio, S. Schmidt, A. Schubert, D. Sinclair, K. Skarpaas, A. K. Soma, G. St-Hilaire, V. Stekhanov, T. Stiegler, X. L. Sun, M. Tarka, J. Todd, T. Tolba, T. I. Totev, R. Tsang, T. Tsang, F. Vachon, B. Veenstra, V. Veeraraghavan, G. Visser, J. L. Vuilleumier, Q. Wang, J. Watkins, M. Weber, W. Wei, L. J. Wen, U. Wichoski, G. Wrede, S. X. Wu, W. H. Wu, Q. Xia, L. Yang, Y. R. Yen, O. Zeldovich, X. Zhang, J. Zhao, Y. Zhou

Research output: Contribution to journal › Article › peer-review

30 Scopus citations

Abstract

Future ton-scale liquefied noble gas detectors depend on efficient light detection in the vacuum ultraviolet (VUV) range. In the past years, silicon photomultipliers (SiPMs) have emerged as a valid alternative to standard photomultiplier tubes or large-area avalanche photodiodes. The next-generation double-beta decay experiment, nEXO, with a 5-ton liquid xenon time projection chamber will use SiPMs for detecting the 175-nm xenon scintillation light, in order to achieve an energy resolution of σ/Q_ββ = 1%. This paper presents recent measurements of the VUV-HD generation SiPMs from Fondazione Bruno Kessler, Trento, Italy, in two complementary setups. It includes measurements of the photon-detection efficiency (PDE) with gaseous xenon scintillation light in a vacuum setup and dark measurements in a dry nitrogen gas setup. We report improved PDE at 175 nm compared to previous generation devices that would meet the criteria of nEXO. Furthermore, we present the projected nEXO detector light collection and energy resolution that could be achieved by using these SiPMs.

Original language	English
Article number	8490731
Pages (from-to)	2823-2833
Number of pages	11
Journal	IEEE Transactions on Nuclear Science
Volume	65
Issue number	11
DOIs	https://doi.org/10.1109/TNS.2018.2875668
State	Published - Nov 2018

Bibliographical note

Publisher Copyright:
© 2018 IEEE.

Funding

This work was supported in part by the Offices of Nuclear and High Energy Physics within DOEs Office of Science and NSF, USA, in part by NSERC, CFI, FRQNT, NRC, and the McDonald Institute (CFREF), Canada, in part by BaCaTeC, Germany, in part by SNF, Switzerland, in part by IBS, South Korea, in part by RFBR, Russia, in part by CAS and ISTCP, China, and in part by the Laboratory Directed Research and Development Programs at the Brookhaven National Laboratory, the Lawrence Livermore National Laboratory, the Oak Ridge National Laboratory, and the Pacific Northwest National Laboratory. ACKNOWLEDGMENT This work was supported in part by the Offices of Nuclear and High Energy Physics within DOEs Office of Science and NSF, USA, in part by NSERC, CFI, FRQNT, NRC, and the McDonald Institute (CFREF), Canada, in part by BaCaTeC, Germany, in part by SNF, Switzerland, in part by IBS, South Korea, in part by RFBR, Russia, in part by CAS and ISTCP, China, and in part by the Laboratory Directed Research and Development Programs at the Brookhaven National Laboratory, the Lawrence Livermore National Laboratory, the Oak Ridge National Laboratory, and the Pacific Northwest National Laboratory.

Funders	Funder number
Laboratory Directed Research and Development Programs at the Brookhaven National Laboratory
McDonald Institute
National Science Foundation	1812245, 1812377, 1506051
Oak Ridge National Laboratory
Laboratory Directed Research and Development
Cummings Foundation
Pacific Northwest National Laboratory
National Research Council
Natural Sciences and Engineering Research Council of Canada
Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung
Russian Foundation for Basic Research
Chinese Academy of Sciences
Fonds de recherche du Québec – Nature et technologies
Canada First Research Excellence Fund
International Science and Technology Cooperation Programme
Bayerisch-Kalifornischen Hochschulzentrum

Keywords

nEXO
photodetectors
silicon photomultiplier
vacuum ultraviolet (VUV) light
xenon detectors

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10.1109/TNS.2018.2875668

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Jamil, A., Ziegler, T., Hufschmidt, P., Li, G., Lupin-Jimenez, L., Michel, T., Ostrovskiy, I., Retière, F., Schneider, J., Wagenpfeil, M., Alamre, A., Albert, J. B., Anton, G., Arnquist, I. J., Badhrees, I., Barbeau, P. S., Beck, D., Belov, V., Bhatta, T., ... Zhou, Y. (2018). VUV-Sensitive Silicon Photomultipliers for Xenon Scintillation Light Detection in nEXO. IEEE Transactions on Nuclear Science, 65(11), 2823-2833. Article 8490731. https://doi.org/10.1109/TNS.2018.2875668

@article{5559fa637ac941b788c63193af072dcf,

title = "VUV-Sensitive Silicon Photomultipliers for Xenon Scintillation Light Detection in nEXO",

abstract = "Future ton-scale liquefied noble gas detectors depend on efficient light detection in the vacuum ultraviolet (VUV) range. In the past years, silicon photomultipliers (SiPMs) have emerged as a valid alternative to standard photomultiplier tubes or large-area avalanche photodiodes. The next-generation double-beta decay experiment, nEXO, with a 5-ton liquid xenon time projection chamber will use SiPMs for detecting the 175-nm xenon scintillation light, in order to achieve an energy resolution of σ/Qββ = 1%. This paper presents recent measurements of the VUV-HD generation SiPMs from Fondazione Bruno Kessler, Trento, Italy, in two complementary setups. It includes measurements of the photon-detection efficiency (PDE) with gaseous xenon scintillation light in a vacuum setup and dark measurements in a dry nitrogen gas setup. We report improved PDE at 175 nm compared to previous generation devices that would meet the criteria of nEXO. Furthermore, we present the projected nEXO detector light collection and energy resolution that could be achieved by using these SiPMs.",

keywords = "nEXO, photodetectors, silicon photomultiplier, vacuum ultraviolet (VUV) light, xenon detectors",

author = "A. Jamil and T. Ziegler and P. Hufschmidt and G. Li and L. Lupin-Jimenez and T. Michel and I. Ostrovskiy and F. Reti{\`e}re and J. Schneider and M. Wagenpfeil and A. Alamre and Albert, {J. B.} and G. Anton and Arnquist, {I. J.} and I. Badhrees and Barbeau, {P. S.} and D. Beck and V. Belov and T. Bhatta and F. Bourque and Brodsky, {J. P.} and E. Brown and T. Brunner and A. Burenkov and Cao, {G. F.} and L. Cao and Cen, {W. R.} and C. Chambers and Charlebois, {S. A.} and M. Chiu and B. Cleveland and M. Coon and M. C{\^o}t{\'e} and A. Craycraft and W. Cree and J. Dalmasson and T. Daniels and L. Darroch and Daugherty, {S. J.} and J. Daughhetee and S. Delaquis and Mesrobian-Kabakian, {A. Der} and R. DeVoe and J. Dilling and Ding, {Y. Y.} and Dolinski, {M. J.} and A. Dragone and J. Echevers and L. Fabris and D. Fairbank and W. Fairbank and J. Farine and S. Feyzbakhsh and R. Fontaine and D. Fudenberg and G. Gallina and G. Giacomini and R. Gornea and G. Gratta and Hansen, {E. V.} and D. Harris and M. Hasan and M. Heffner and J. H{\"o}{\ss}l and Hoppe, {E. W.} and A. House and M. Hughes and Y. Ito and A. Iverson and C. Jessiman and Jewell, {M. J.} and Jiang, {X. S.} and A. Karelin and Kaufman, {L. J.} and T. Koffas and S. Kravitz and R. Kr{\"u}cken and A. Kuchenkov and Kumar, {K. S.} and Y. Lan and A. Larson and Leonard, {D. S.} and S. Li and Z. Li and C. Licciardi and Lin, {Y. H.} and P. Lv and R. MacLellan and B. Mong and Moore, {D. C.} and K. Murray and Newby, {R. J.} and Z. Ning and O. Njoya and F. Nolet and O. Nusair and K. Odgers and A. Odian and M. Oriunno and Orrell, {J. L.} and Ortega, {G. S.} and Overman, {C. T.} and S. Parent and A. Piepke and A. Pocar and Pratte, {J. F.} and D. Qiu and V. Radeka and E. Raguzin and T. Rao and S. Rescia and A. Robinson and T. Rossignol and Rowson, {P. C.} and N. Roy and R. Saldanha and S. Sangiorgio and S. Schmidt and A. Schubert and D. Sinclair and K. Skarpaas and Soma, {A. K.} and G. St-Hilaire and V. Stekhanov and T. Stiegler and Sun, {X. L.} and M. Tarka and J. Todd and T. Tolba and Totev, {T. I.} and R. Tsang and T. Tsang and F. Vachon and B. Veenstra and V. Veeraraghavan and G. Visser and Vuilleumier, {J. L.} and Q. Wang and J. Watkins and M. Weber and W. Wei and Wen, {L. J.} and U. Wichoski and G. Wrede and Wu, {S. X.} and Wu, {W. H.} and Q. Xia and L. Yang and Yen, {Y. R.} and O. Zeldovich and X. Zhang and J. Zhao and Y. Zhou",

note = "Publisher Copyright: {\textcopyright} 2018 IEEE.",

year = "2018",

month = nov,

doi = "10.1109/TNS.2018.2875668",

language = "English",

volume = "65",

pages = "2823--2833",

journal = "IEEE Transactions on Nuclear Science",

issn = "0018-9499",

publisher = "Institute of Electrical and Electronics Engineers",

number = "11",

}

Jamil, A, Ziegler, T, Hufschmidt, P, Li, G, Lupin-Jimenez, L, Michel, T, Ostrovskiy, I, Retière, F, Schneider, J, Wagenpfeil, M, Alamre, A, Albert, JB, Anton, G, Arnquist, IJ, Badhrees, I, Barbeau, PS, Beck, D, Belov, V, Bhatta, T, Bourque, F, Brodsky, JP, Brown, E, Brunner, T, Burenkov, A, Cao, GF, Cao, L, Cen, WR, Chambers, C, Charlebois, SA, Chiu, M, Cleveland, B, Coon, M, Côté, M, Craycraft, A, Cree, W, Dalmasson, J, Daniels, T, Darroch, L, Daugherty, SJ, Daughhetee, J, Delaquis, S, Mesrobian-Kabakian, AD, DeVoe, R, Dilling, J, Ding, YY, Dolinski, MJ, Dragone, A, Echevers, J, Fabris, L, Fairbank, D, Fairbank, W, Farine, J, Feyzbakhsh, S, Fontaine, R, Fudenberg, D, Gallina, G, Giacomini, G, Gornea, R, Gratta, G, Hansen, EV, Harris, D, Hasan, M, Heffner, M, Hößl, J, Hoppe, EW, House, A, Hughes, M, Ito, Y, Iverson, A, Jessiman, C, Jewell, MJ, Jiang, XS, Karelin, A, Kaufman, LJ, Koffas, T, Kravitz, S, Krücken, R, Kuchenkov, A, Kumar, KS, Lan, Y, Larson, A, Leonard, DS, Li, S, Li, Z, Licciardi, C, Lin, YH, Lv, P, MacLellan, R, Mong, B, Moore, DC, Murray, K, Newby, RJ, Ning, Z, Njoya, O, Nolet, F, Nusair, O, Odgers, K, Odian, A, Oriunno, M, Orrell, JL, Ortega, GS, Overman, CT, Parent, S, Piepke, A, Pocar, A, Pratte, JF, Qiu, D, Radeka, V, Raguzin, E, Rao, T, Rescia, S, Robinson, A, Rossignol, T, Rowson, PC, Roy, N, Saldanha, R, Sangiorgio, S, Schmidt, S, Schubert, A, Sinclair, D, Skarpaas, K, Soma, AK, St-Hilaire, G, Stekhanov, V, Stiegler, T, Sun, XL, Tarka, M, Todd, J, Tolba, T, Totev, TI, Tsang, R, Tsang, T, Vachon, F, Veenstra, B, Veeraraghavan, V, Visser, G, Vuilleumier, JL, Wang, Q, Watkins, J, Weber, M, Wei, W, Wen, LJ, Wichoski, U, Wrede, G, Wu, SX, Wu, WH, Xia, Q, Yang, L, Yen, YR, Zeldovich, O, Zhang, X, Zhao, J & Zhou, Y 2018, 'VUV-Sensitive Silicon Photomultipliers for Xenon Scintillation Light Detection in nEXO', IEEE Transactions on Nuclear Science, vol. 65, no. 11, 8490731, pp. 2823-2833. https://doi.org/10.1109/TNS.2018.2875668

TY - JOUR

T1 - VUV-Sensitive Silicon Photomultipliers for Xenon Scintillation Light Detection in nEXO

AU - Jamil, A.

AU - Ziegler, T.

AU - Hufschmidt, P.

AU - Li, G.

AU - Lupin-Jimenez, L.

AU - Michel, T.

AU - Ostrovskiy, I.

AU - Retière, F.

AU - Schneider, J.

AU - Wagenpfeil, M.

AU - Alamre, A.

AU - Albert, J. B.

AU - Anton, G.

AU - Arnquist, I. J.

AU - Badhrees, I.

AU - Barbeau, P. S.

AU - Beck, D.

AU - Belov, V.

AU - Bhatta, T.

AU - Bourque, F.

AU - Brodsky, J. P.

AU - Brown, E.

AU - Brunner, T.

AU - Burenkov, A.

AU - Cao, G. F.

AU - Cao, L.

AU - Cen, W. R.

AU - Chambers, C.

AU - Charlebois, S. A.

AU - Chiu, M.

AU - Cleveland, B.

AU - Coon, M.

AU - Côté, M.

AU - Craycraft, A.

AU - Cree, W.

AU - Dalmasson, J.

AU - Daniels, T.

AU - Darroch, L.

AU - Daugherty, S. J.

AU - Daughhetee, J.

AU - Delaquis, S.

AU - Mesrobian-Kabakian, A. Der

AU - DeVoe, R.

AU - Dilling, J.

AU - Ding, Y. Y.

AU - Dolinski, M. J.

AU - Dragone, A.

AU - Echevers, J.

AU - Fabris, L.

AU - Fairbank, D.

AU - Fairbank, W.

AU - Farine, J.

AU - Feyzbakhsh, S.

AU - Fontaine, R.

AU - Fudenberg, D.

AU - Gallina, G.

AU - Giacomini, G.

AU - Gornea, R.

AU - Gratta, G.

AU - Hansen, E. V.

AU - Harris, D.

AU - Hasan, M.

AU - Heffner, M.

AU - Hößl, J.

AU - Hoppe, E. W.

AU - House, A.

AU - Hughes, M.

AU - Ito, Y.

AU - Iverson, A.

AU - Jessiman, C.

AU - Jewell, M. J.

AU - Jiang, X. S.

AU - Karelin, A.

AU - Kaufman, L. J.

AU - Koffas, T.

AU - Kravitz, S.

AU - Krücken, R.

AU - Kuchenkov, A.

AU - Kumar, K. S.

AU - Lan, Y.

AU - Larson, A.

AU - Leonard, D. S.

AU - Li, S.

AU - Li, Z.

AU - Licciardi, C.

AU - Lin, Y. H.

AU - Lv, P.

AU - MacLellan, R.

AU - Mong, B.

AU - Moore, D. C.

AU - Murray, K.

AU - Newby, R. J.

AU - Ning, Z.

AU - Njoya, O.

AU - Nolet, F.

AU - Nusair, O.

AU - Odgers, K.

AU - Odian, A.

AU - Oriunno, M.

AU - Orrell, J. L.

AU - Ortega, G. S.

AU - Overman, C. T.

AU - Parent, S.

AU - Piepke, A.

AU - Pocar, A.

AU - Pratte, J. F.

AU - Qiu, D.

AU - Radeka, V.

AU - Raguzin, E.

AU - Rao, T.

AU - Rescia, S.

AU - Robinson, A.

AU - Rossignol, T.

AU - Rowson, P. C.

AU - Roy, N.

AU - Saldanha, R.

AU - Sangiorgio, S.

AU - Schmidt, S.

AU - Schubert, A.

AU - Sinclair, D.

AU - Skarpaas, K.

AU - Soma, A. K.

AU - St-Hilaire, G.

AU - Stekhanov, V.

AU - Stiegler, T.

AU - Sun, X. L.

AU - Tarka, M.

AU - Todd, J.

AU - Tolba, T.

AU - Totev, T. I.

AU - Tsang, R.

AU - Tsang, T.

AU - Vachon, F.

AU - Veenstra, B.

AU - Veeraraghavan, V.

AU - Visser, G.

AU - Vuilleumier, J. L.

AU - Wang, Q.

AU - Watkins, J.

AU - Weber, M.

AU - Wei, W.

AU - Wen, L. J.

AU - Wichoski, U.

AU - Wrede, G.

AU - Wu, S. X.

AU - Wu, W. H.

AU - Xia, Q.

AU - Yang, L.

AU - Yen, Y. R.

AU - Zeldovich, O.

AU - Zhang, X.

AU - Zhao, J.

AU - Zhou, Y.

PY - 2018/11

Y1 - 2018/11

N2 - Future ton-scale liquefied noble gas detectors depend on efficient light detection in the vacuum ultraviolet (VUV) range. In the past years, silicon photomultipliers (SiPMs) have emerged as a valid alternative to standard photomultiplier tubes or large-area avalanche photodiodes. The next-generation double-beta decay experiment, nEXO, with a 5-ton liquid xenon time projection chamber will use SiPMs for detecting the 175-nm xenon scintillation light, in order to achieve an energy resolution of σ/Qββ = 1%. This paper presents recent measurements of the VUV-HD generation SiPMs from Fondazione Bruno Kessler, Trento, Italy, in two complementary setups. It includes measurements of the photon-detection efficiency (PDE) with gaseous xenon scintillation light in a vacuum setup and dark measurements in a dry nitrogen gas setup. We report improved PDE at 175 nm compared to previous generation devices that would meet the criteria of nEXO. Furthermore, we present the projected nEXO detector light collection and energy resolution that could be achieved by using these SiPMs.

AB - Future ton-scale liquefied noble gas detectors depend on efficient light detection in the vacuum ultraviolet (VUV) range. In the past years, silicon photomultipliers (SiPMs) have emerged as a valid alternative to standard photomultiplier tubes or large-area avalanche photodiodes. The next-generation double-beta decay experiment, nEXO, with a 5-ton liquid xenon time projection chamber will use SiPMs for detecting the 175-nm xenon scintillation light, in order to achieve an energy resolution of σ/Qββ = 1%. This paper presents recent measurements of the VUV-HD generation SiPMs from Fondazione Bruno Kessler, Trento, Italy, in two complementary setups. It includes measurements of the photon-detection efficiency (PDE) with gaseous xenon scintillation light in a vacuum setup and dark measurements in a dry nitrogen gas setup. We report improved PDE at 175 nm compared to previous generation devices that would meet the criteria of nEXO. Furthermore, we present the projected nEXO detector light collection and energy resolution that could be achieved by using these SiPMs.

KW - nEXO

KW - photodetectors

KW - silicon photomultiplier

KW - vacuum ultraviolet (VUV) light

KW - xenon detectors

UR - http://www.scopus.com/inward/record.url?scp=85055026366&partnerID=8YFLogxK

U2 - 10.1109/TNS.2018.2875668

DO - 10.1109/TNS.2018.2875668

M3 - Article

AN - SCOPUS:85055026366

SN - 0018-9499

VL - 65

SP - 2823

EP - 2833

JO - IEEE Transactions on Nuclear Science

JF - IEEE Transactions on Nuclear Science

IS - 11

M1 - 8490731

ER -

VUV-Sensitive Silicon Photomultipliers for Xenon Scintillation Light Detection in nEXO

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