Assembly and performance of SiPM arrays for the prototype SCT proposed for CTA
The Near Ultraviolet High Density (NUV-HD) SiPMs produced by Fondazione Bruno Kessler have been employed to develop 16-pixel optical units to equip the focal plane of the prototype Schwarzschild–Couder Telescope (pSCT) proposed as a possible design for the Medium-Sized Telescope of the Cherenkov Tel...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Ambrosi, G. [verfasserIn] Ambrosio, M. [verfasserIn] Aramo, C. [verfasserIn] Benbow, W. [verfasserIn] Bertucci, B. [verfasserIn] Bissaldi, E. [verfasserIn] Bitossi, M. [verfasserIn] Boiano, A. [verfasserIn] Bonavolontà, C. [verfasserIn] Cameron, R.A. [verfasserIn] Capasso, M. [verfasserIn] Consiglio, L. [verfasserIn] Depaoli, D. [verfasserIn] Di Pierro, F. [verfasserIn] Di Venere, L. [verfasserIn] Fiandrini, E. [verfasserIn] Furniss, A. [verfasserIn] Gent, A. [verfasserIn] Giglietto, N. [verfasserIn] Giordano, F. [verfasserIn] Hanlon, W. [verfasserIn] Hervet, O. [verfasserIn] Incardona, S. [verfasserIn] Ionica, M. [verfasserIn] Jin, W. [verfasserIn] Kieda, D. [verfasserIn] Licciulli, F. [verfasserIn] Loporchio, S. [verfasserIn] Marsella, G. [verfasserIn] Masone, V. [verfasserIn] Mode, B.A.W. [verfasserIn] Mukherjee, R. [verfasserIn] Pantaleo, F.R. [verfasserIn] Paoletti, R. [verfasserIn] Ribeiro, D. [verfasserIn] Rugliancich, A. [verfasserIn] Saha, L. [verfasserIn] Stiaccini, L. [verfasserIn] Taylor, L.P. [verfasserIn] Tosti, L. [verfasserIn] Tripodo, G. [verfasserIn] Vagelli, V. [verfasserIn] Valentino, M. [verfasserIn] Vandenbroucke, J. [verfasserIn] Vassiliev, V.V. [verfasserIn] Williams, D.A. [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2022 |
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| Schlagwörter: |
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| Übergeordnetes Werk: |
Enthalten in: Nuclear instruments & methods in physics research / A - Amsterdam : North-Holland Publ. Co., 1984, 1041 |
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| Übergeordnetes Werk: |
volume:1041 |
| DOI / URN: |
10.1016/j.nima.2022.167359 |
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| 100 | 1 | |a Ambrosi, G. |e verfasserin |0 (orcid)0000-0001-6977-9559 |4 aut | |
| 245 | 1 | 0 | |a Assembly and performance of SiPM arrays for the prototype SCT proposed for CTA |
| 264 | 1 | |c 2022 | |
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| 520 | |a The Near Ultraviolet High Density (NUV-HD) SiPMs produced by Fondazione Bruno Kessler have been employed to develop 16-pixel optical units to equip the focal plane of the prototype Schwarzschild–Couder Telescope (pSCT) proposed as a possible design for the Medium-Sized Telescope of the Cherenkov Telescope Array Observatory. After the assembly procedure, the optical units were tested and characterized to study their performance and homogeneity in terms of gain and dark count rate. In this work, we report on the assembly procedure and on the laboratory tests performed on different production of NUV-HD and the selection we made for the best quality sensors to be used in the installation on the telescope camera. Currently 36 NUV-HD3 optical units have been successfully integrated on the pSCT camera, together with 64 HAMAMATSU MPPCs. An upgrade of the pSCT camera is foreseen over the next years when the full focal plane is expected to be equipped entirely with FBK NUV-HD3 SiPMs, for a total of 11328 pixels. | ||
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| 650 | 4 | |a Cherenkov telescopes array | |
| 650 | 4 | |a Very-high-energy astrophysics | |
| 700 | 1 | |a Ambrosio, M. |e verfasserin |4 aut | |
| 700 | 1 | |a Aramo, C. |e verfasserin |4 aut | |
| 700 | 1 | |a Benbow, W. |e verfasserin |4 aut | |
| 700 | 1 | |a Bertucci, B. |e verfasserin |4 aut | |
| 700 | 1 | |a Bissaldi, E. |e verfasserin |4 aut | |
| 700 | 1 | |a Bitossi, M. |e verfasserin |4 aut | |
| 700 | 1 | |a Boiano, A. |e verfasserin |4 aut | |
| 700 | 1 | |a Bonavolontà, C. |e verfasserin |4 aut | |
| 700 | 1 | |a Cameron, R.A. |e verfasserin |4 aut | |
| 700 | 1 | |a Capasso, M. |e verfasserin |4 aut | |
| 700 | 1 | |a Consiglio, L. |e verfasserin |4 aut | |
| 700 | 1 | |a Depaoli, D. |e verfasserin |4 aut | |
| 700 | 1 | |a Di Pierro, F. |e verfasserin |4 aut | |
| 700 | 1 | |a Di Venere, L. |e verfasserin |4 aut | |
| 700 | 1 | |a Fiandrini, E. |e verfasserin |4 aut | |
| 700 | 1 | |a Furniss, A. |e verfasserin |4 aut | |
| 700 | 1 | |a Gent, A. |e verfasserin |4 aut | |
| 700 | 1 | |a Giglietto, N. |e verfasserin |4 aut | |
| 700 | 1 | |a Giordano, F. |e verfasserin |4 aut | |
| 700 | 1 | |a Hanlon, W. |e verfasserin |4 aut | |
| 700 | 1 | |a Hervet, O. |e verfasserin |4 aut | |
| 700 | 1 | |a Incardona, S. |e verfasserin |4 aut | |
| 700 | 1 | |a Ionica, M. |e verfasserin |4 aut | |
| 700 | 1 | |a Jin, W. |e verfasserin |4 aut | |
| 700 | 1 | |a Kieda, D. |e verfasserin |4 aut | |
| 700 | 1 | |a Licciulli, F. |e verfasserin |4 aut | |
| 700 | 1 | |a Loporchio, S. |e verfasserin |0 (orcid)0000-0003-4457-5431 |4 aut | |
| 700 | 1 | |a Marsella, G. |e verfasserin |4 aut | |
| 700 | 1 | |a Masone, V. |e verfasserin |4 aut | |
| 700 | 1 | |a Mode, B.A.W. |e verfasserin |4 aut | |
| 700 | 1 | |a Mukherjee, R. |e verfasserin |4 aut | |
| 700 | 1 | |a Pantaleo, F.R. |e verfasserin |4 aut | |
| 700 | 1 | |a Paoletti, R. |e verfasserin |4 aut | |
| 700 | 1 | |a Ribeiro, D. |e verfasserin |4 aut | |
| 700 | 1 | |a Rugliancich, A. |e verfasserin |4 aut | |
| 700 | 1 | |a Saha, L. |e verfasserin |4 aut | |
| 700 | 1 | |a Stiaccini, L. |e verfasserin |4 aut | |
| 700 | 1 | |a Taylor, L.P. |e verfasserin |4 aut | |
| 700 | 1 | |a Tosti, L. |e verfasserin |4 aut | |
| 700 | 1 | |a Tripodo, G. |e verfasserin |4 aut | |
| 700 | 1 | |a Vagelli, V. |e verfasserin |4 aut | |
| 700 | 1 | |a Valentino, M. |e verfasserin |4 aut | |
| 700 | 1 | |a Vandenbroucke, J. |e verfasserin |4 aut | |
| 700 | 1 | |a Vassiliev, V.V. |e verfasserin |4 aut | |
| 700 | 1 | |a Williams, D.A. |e verfasserin |4 aut | |
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10.1016/j.nima.2022.167359 doi (DE-627)ELV008480508 (ELSEVIER)S0168-9002(22)00669-6 DE-627 ger DE-627 rda eng 530 DE-600 33.05 bkl 33.07 bkl 33.40 bkl Ambrosi, G. verfasserin (orcid)0000-0001-6977-9559 aut Assembly and performance of SiPM arrays for the prototype SCT proposed for CTA 2022 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The Near Ultraviolet High Density (NUV-HD) SiPMs produced by Fondazione Bruno Kessler have been employed to develop 16-pixel optical units to equip the focal plane of the prototype Schwarzschild–Couder Telescope (pSCT) proposed as a possible design for the Medium-Sized Telescope of the Cherenkov Telescope Array Observatory. After the assembly procedure, the optical units were tested and characterized to study their performance and homogeneity in terms of gain and dark count rate. In this work, we report on the assembly procedure and on the laboratory tests performed on different production of NUV-HD and the selection we made for the best quality sensors to be used in the installation on the telescope camera. Currently 36 NUV-HD3 optical units have been successfully integrated on the pSCT camera, together with 64 HAMAMATSU MPPCs. An upgrade of the pSCT camera is foreseen over the next years when the full focal plane is expected to be equipped entirely with FBK NUV-HD3 SiPMs, for a total of 11328 pixels. Silicon photomultipliers Cherenkov telescopes array Very-high-energy astrophysics Ambrosio, M. verfasserin aut Aramo, C. verfasserin aut Benbow, W. verfasserin aut Bertucci, B. verfasserin aut Bissaldi, E. verfasserin aut Bitossi, M. verfasserin aut Boiano, A. verfasserin aut Bonavolontà, C. verfasserin aut Cameron, R.A. verfasserin aut Capasso, M. verfasserin aut Consiglio, L. verfasserin aut Depaoli, D. verfasserin aut Di Pierro, F. verfasserin aut Di Venere, L. verfasserin aut Fiandrini, E. verfasserin aut Furniss, A. verfasserin aut Gent, A. verfasserin aut Giglietto, N. verfasserin aut Giordano, F. verfasserin aut Hanlon, W. verfasserin aut Hervet, O. verfasserin aut Incardona, S. verfasserin aut Ionica, M. verfasserin aut Jin, W. verfasserin aut Kieda, D. verfasserin aut Licciulli, F. verfasserin aut Loporchio, S. verfasserin (orcid)0000-0003-4457-5431 aut Marsella, G. verfasserin aut Masone, V. verfasserin aut Mode, B.A.W. verfasserin aut Mukherjee, R. verfasserin aut Pantaleo, F.R. verfasserin aut Paoletti, R. verfasserin aut Ribeiro, D. verfasserin aut Rugliancich, A. verfasserin aut Saha, L. verfasserin aut Stiaccini, L. verfasserin aut Taylor, L.P. verfasserin aut Tosti, L. verfasserin aut Tripodo, G. verfasserin aut Vagelli, V. verfasserin aut Valentino, M. verfasserin aut Vandenbroucke, J. verfasserin aut Vassiliev, V.V. verfasserin aut Williams, D.A. verfasserin aut Enthalten in Nuclear instruments & methods in physics research / A Amsterdam : North-Holland Publ. Co., 1984 1041 Online-Ressource (DE-627)266014666 (DE-600)1466532-3 (DE-576)074959743 0168-9002 nnns volume:1041 GBV_USEFLAG_U SYSFLAG_U GBV_ELV GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_224 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2027 GBV_ILN_2034 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2056 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2336 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4313 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4393 33.05 Experimentalphysik 33.07 Spektroskopie 33.40 Kernphysik AR 1041 |
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10.1016/j.nima.2022.167359 doi (DE-627)ELV008480508 (ELSEVIER)S0168-9002(22)00669-6 DE-627 ger DE-627 rda eng 530 DE-600 33.05 bkl 33.07 bkl 33.40 bkl Ambrosi, G. verfasserin (orcid)0000-0001-6977-9559 aut Assembly and performance of SiPM arrays for the prototype SCT proposed for CTA 2022 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The Near Ultraviolet High Density (NUV-HD) SiPMs produced by Fondazione Bruno Kessler have been employed to develop 16-pixel optical units to equip the focal plane of the prototype Schwarzschild–Couder Telescope (pSCT) proposed as a possible design for the Medium-Sized Telescope of the Cherenkov Telescope Array Observatory. After the assembly procedure, the optical units were tested and characterized to study their performance and homogeneity in terms of gain and dark count rate. In this work, we report on the assembly procedure and on the laboratory tests performed on different production of NUV-HD and the selection we made for the best quality sensors to be used in the installation on the telescope camera. Currently 36 NUV-HD3 optical units have been successfully integrated on the pSCT camera, together with 64 HAMAMATSU MPPCs. An upgrade of the pSCT camera is foreseen over the next years when the full focal plane is expected to be equipped entirely with FBK NUV-HD3 SiPMs, for a total of 11328 pixels. Silicon photomultipliers Cherenkov telescopes array Very-high-energy astrophysics Ambrosio, M. verfasserin aut Aramo, C. verfasserin aut Benbow, W. verfasserin aut Bertucci, B. verfasserin aut Bissaldi, E. verfasserin aut Bitossi, M. verfasserin aut Boiano, A. verfasserin aut Bonavolontà, C. verfasserin aut Cameron, R.A. verfasserin aut Capasso, M. verfasserin aut Consiglio, L. verfasserin aut Depaoli, D. verfasserin aut Di Pierro, F. verfasserin aut Di Venere, L. verfasserin aut Fiandrini, E. verfasserin aut Furniss, A. verfasserin aut Gent, A. verfasserin aut Giglietto, N. verfasserin aut Giordano, F. verfasserin aut Hanlon, W. verfasserin aut Hervet, O. verfasserin aut Incardona, S. verfasserin aut Ionica, M. verfasserin aut Jin, W. verfasserin aut Kieda, D. verfasserin aut Licciulli, F. verfasserin aut Loporchio, S. verfasserin (orcid)0000-0003-4457-5431 aut Marsella, G. verfasserin aut Masone, V. verfasserin aut Mode, B.A.W. verfasserin aut Mukherjee, R. verfasserin aut Pantaleo, F.R. verfasserin aut Paoletti, R. verfasserin aut Ribeiro, D. verfasserin aut Rugliancich, A. verfasserin aut Saha, L. verfasserin aut Stiaccini, L. verfasserin aut Taylor, L.P. verfasserin aut Tosti, L. verfasserin aut Tripodo, G. verfasserin aut Vagelli, V. verfasserin aut Valentino, M. verfasserin aut Vandenbroucke, J. verfasserin aut Vassiliev, V.V. verfasserin aut Williams, D.A. verfasserin aut Enthalten in Nuclear instruments & methods in physics research / A Amsterdam : North-Holland Publ. Co., 1984 1041 Online-Ressource (DE-627)266014666 (DE-600)1466532-3 (DE-576)074959743 0168-9002 nnns volume:1041 GBV_USEFLAG_U SYSFLAG_U GBV_ELV GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_224 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2027 GBV_ILN_2034 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2056 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2336 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4313 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4393 33.05 Experimentalphysik 33.07 Spektroskopie 33.40 Kernphysik AR 1041 |
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10.1016/j.nima.2022.167359 doi (DE-627)ELV008480508 (ELSEVIER)S0168-9002(22)00669-6 DE-627 ger DE-627 rda eng 530 DE-600 33.05 bkl 33.07 bkl 33.40 bkl Ambrosi, G. verfasserin (orcid)0000-0001-6977-9559 aut Assembly and performance of SiPM arrays for the prototype SCT proposed for CTA 2022 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The Near Ultraviolet High Density (NUV-HD) SiPMs produced by Fondazione Bruno Kessler have been employed to develop 16-pixel optical units to equip the focal plane of the prototype Schwarzschild–Couder Telescope (pSCT) proposed as a possible design for the Medium-Sized Telescope of the Cherenkov Telescope Array Observatory. After the assembly procedure, the optical units were tested and characterized to study their performance and homogeneity in terms of gain and dark count rate. In this work, we report on the assembly procedure and on the laboratory tests performed on different production of NUV-HD and the selection we made for the best quality sensors to be used in the installation on the telescope camera. Currently 36 NUV-HD3 optical units have been successfully integrated on the pSCT camera, together with 64 HAMAMATSU MPPCs. An upgrade of the pSCT camera is foreseen over the next years when the full focal plane is expected to be equipped entirely with FBK NUV-HD3 SiPMs, for a total of 11328 pixels. Silicon photomultipliers Cherenkov telescopes array Very-high-energy astrophysics Ambrosio, M. verfasserin aut Aramo, C. verfasserin aut Benbow, W. verfasserin aut Bertucci, B. verfasserin aut Bissaldi, E. verfasserin aut Bitossi, M. verfasserin aut Boiano, A. verfasserin aut Bonavolontà, C. verfasserin aut Cameron, R.A. verfasserin aut Capasso, M. verfasserin aut Consiglio, L. verfasserin aut Depaoli, D. verfasserin aut Di Pierro, F. verfasserin aut Di Venere, L. verfasserin aut Fiandrini, E. verfasserin aut Furniss, A. verfasserin aut Gent, A. verfasserin aut Giglietto, N. verfasserin aut Giordano, F. verfasserin aut Hanlon, W. verfasserin aut Hervet, O. verfasserin aut Incardona, S. verfasserin aut Ionica, M. verfasserin aut Jin, W. verfasserin aut Kieda, D. verfasserin aut Licciulli, F. verfasserin aut Loporchio, S. verfasserin (orcid)0000-0003-4457-5431 aut Marsella, G. verfasserin aut Masone, V. verfasserin aut Mode, B.A.W. verfasserin aut Mukherjee, R. verfasserin aut Pantaleo, F.R. verfasserin aut Paoletti, R. verfasserin aut Ribeiro, D. verfasserin aut Rugliancich, A. verfasserin aut Saha, L. verfasserin aut Stiaccini, L. verfasserin aut Taylor, L.P. verfasserin aut Tosti, L. verfasserin aut Tripodo, G. verfasserin aut Vagelli, V. verfasserin aut Valentino, M. verfasserin aut Vandenbroucke, J. verfasserin aut Vassiliev, V.V. verfasserin aut Williams, D.A. verfasserin aut Enthalten in Nuclear instruments & methods in physics research / A Amsterdam : North-Holland Publ. Co., 1984 1041 Online-Ressource (DE-627)266014666 (DE-600)1466532-3 (DE-576)074959743 0168-9002 nnns volume:1041 GBV_USEFLAG_U SYSFLAG_U GBV_ELV GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_224 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2027 GBV_ILN_2034 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2056 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2336 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4313 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4393 33.05 Experimentalphysik 33.07 Spektroskopie 33.40 Kernphysik AR 1041 |
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10.1016/j.nima.2022.167359 doi (DE-627)ELV008480508 (ELSEVIER)S0168-9002(22)00669-6 DE-627 ger DE-627 rda eng 530 DE-600 33.05 bkl 33.07 bkl 33.40 bkl Ambrosi, G. verfasserin (orcid)0000-0001-6977-9559 aut Assembly and performance of SiPM arrays for the prototype SCT proposed for CTA 2022 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The Near Ultraviolet High Density (NUV-HD) SiPMs produced by Fondazione Bruno Kessler have been employed to develop 16-pixel optical units to equip the focal plane of the prototype Schwarzschild–Couder Telescope (pSCT) proposed as a possible design for the Medium-Sized Telescope of the Cherenkov Telescope Array Observatory. After the assembly procedure, the optical units were tested and characterized to study their performance and homogeneity in terms of gain and dark count rate. In this work, we report on the assembly procedure and on the laboratory tests performed on different production of NUV-HD and the selection we made for the best quality sensors to be used in the installation on the telescope camera. Currently 36 NUV-HD3 optical units have been successfully integrated on the pSCT camera, together with 64 HAMAMATSU MPPCs. An upgrade of the pSCT camera is foreseen over the next years when the full focal plane is expected to be equipped entirely with FBK NUV-HD3 SiPMs, for a total of 11328 pixels. Silicon photomultipliers Cherenkov telescopes array Very-high-energy astrophysics Ambrosio, M. verfasserin aut Aramo, C. verfasserin aut Benbow, W. verfasserin aut Bertucci, B. verfasserin aut Bissaldi, E. verfasserin aut Bitossi, M. verfasserin aut Boiano, A. verfasserin aut Bonavolontà, C. verfasserin aut Cameron, R.A. verfasserin aut Capasso, M. verfasserin aut Consiglio, L. verfasserin aut Depaoli, D. verfasserin aut Di Pierro, F. verfasserin aut Di Venere, L. verfasserin aut Fiandrini, E. verfasserin aut Furniss, A. verfasserin aut Gent, A. verfasserin aut Giglietto, N. verfasserin aut Giordano, F. verfasserin aut Hanlon, W. verfasserin aut Hervet, O. verfasserin aut Incardona, S. verfasserin aut Ionica, M. verfasserin aut Jin, W. verfasserin aut Kieda, D. verfasserin aut Licciulli, F. verfasserin aut Loporchio, S. verfasserin (orcid)0000-0003-4457-5431 aut Marsella, G. verfasserin aut Masone, V. verfasserin aut Mode, B.A.W. verfasserin aut Mukherjee, R. verfasserin aut Pantaleo, F.R. verfasserin aut Paoletti, R. verfasserin aut Ribeiro, D. verfasserin aut Rugliancich, A. verfasserin aut Saha, L. verfasserin aut Stiaccini, L. verfasserin aut Taylor, L.P. verfasserin aut Tosti, L. verfasserin aut Tripodo, G. verfasserin aut Vagelli, V. verfasserin aut Valentino, M. verfasserin aut Vandenbroucke, J. verfasserin aut Vassiliev, V.V. verfasserin aut Williams, D.A. verfasserin aut Enthalten in Nuclear instruments & methods in physics research / A Amsterdam : North-Holland Publ. Co., 1984 1041 Online-Ressource (DE-627)266014666 (DE-600)1466532-3 (DE-576)074959743 0168-9002 nnns volume:1041 GBV_USEFLAG_U SYSFLAG_U GBV_ELV GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_224 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2027 GBV_ILN_2034 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2056 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2336 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4313 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4393 33.05 Experimentalphysik 33.07 Spektroskopie 33.40 Kernphysik AR 1041 |
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10.1016/j.nima.2022.167359 doi (DE-627)ELV008480508 (ELSEVIER)S0168-9002(22)00669-6 DE-627 ger DE-627 rda eng 530 DE-600 33.05 bkl 33.07 bkl 33.40 bkl Ambrosi, G. verfasserin (orcid)0000-0001-6977-9559 aut Assembly and performance of SiPM arrays for the prototype SCT proposed for CTA 2022 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The Near Ultraviolet High Density (NUV-HD) SiPMs produced by Fondazione Bruno Kessler have been employed to develop 16-pixel optical units to equip the focal plane of the prototype Schwarzschild–Couder Telescope (pSCT) proposed as a possible design for the Medium-Sized Telescope of the Cherenkov Telescope Array Observatory. After the assembly procedure, the optical units were tested and characterized to study their performance and homogeneity in terms of gain and dark count rate. In this work, we report on the assembly procedure and on the laboratory tests performed on different production of NUV-HD and the selection we made for the best quality sensors to be used in the installation on the telescope camera. Currently 36 NUV-HD3 optical units have been successfully integrated on the pSCT camera, together with 64 HAMAMATSU MPPCs. An upgrade of the pSCT camera is foreseen over the next years when the full focal plane is expected to be equipped entirely with FBK NUV-HD3 SiPMs, for a total of 11328 pixels. Silicon photomultipliers Cherenkov telescopes array Very-high-energy astrophysics Ambrosio, M. verfasserin aut Aramo, C. verfasserin aut Benbow, W. verfasserin aut Bertucci, B. verfasserin aut Bissaldi, E. verfasserin aut Bitossi, M. verfasserin aut Boiano, A. verfasserin aut Bonavolontà, C. verfasserin aut Cameron, R.A. verfasserin aut Capasso, M. verfasserin aut Consiglio, L. verfasserin aut Depaoli, D. verfasserin aut Di Pierro, F. verfasserin aut Di Venere, L. verfasserin aut Fiandrini, E. verfasserin aut Furniss, A. verfasserin aut Gent, A. verfasserin aut Giglietto, N. verfasserin aut Giordano, F. verfasserin aut Hanlon, W. verfasserin aut Hervet, O. verfasserin aut Incardona, S. verfasserin aut Ionica, M. verfasserin aut Jin, W. verfasserin aut Kieda, D. verfasserin aut Licciulli, F. verfasserin aut Loporchio, S. verfasserin (orcid)0000-0003-4457-5431 aut Marsella, G. verfasserin aut Masone, V. verfasserin aut Mode, B.A.W. verfasserin aut Mukherjee, R. verfasserin aut Pantaleo, F.R. verfasserin aut Paoletti, R. verfasserin aut Ribeiro, D. verfasserin aut Rugliancich, A. verfasserin aut Saha, L. verfasserin aut Stiaccini, L. verfasserin aut Taylor, L.P. verfasserin aut Tosti, L. verfasserin aut Tripodo, G. verfasserin aut Vagelli, V. verfasserin aut Valentino, M. verfasserin aut Vandenbroucke, J. verfasserin aut Vassiliev, V.V. verfasserin aut Williams, D.A. verfasserin aut Enthalten in Nuclear instruments & methods in physics research / A Amsterdam : North-Holland Publ. Co., 1984 1041 Online-Ressource (DE-627)266014666 (DE-600)1466532-3 (DE-576)074959743 0168-9002 nnns volume:1041 GBV_USEFLAG_U SYSFLAG_U GBV_ELV GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_224 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2027 GBV_ILN_2034 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2056 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2336 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4313 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4393 33.05 Experimentalphysik 33.07 Spektroskopie 33.40 Kernphysik AR 1041 |
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Ambrosi, G. @@aut@@ Ambrosio, M. @@aut@@ Aramo, C. @@aut@@ Benbow, W. @@aut@@ Bertucci, B. @@aut@@ Bissaldi, E. @@aut@@ Bitossi, M. @@aut@@ Boiano, A. @@aut@@ Bonavolontà, C. @@aut@@ Cameron, R.A. @@aut@@ Capasso, M. @@aut@@ Consiglio, L. @@aut@@ Depaoli, D. @@aut@@ Di Pierro, F. @@aut@@ Di Venere, L. @@aut@@ Fiandrini, E. @@aut@@ Furniss, A. @@aut@@ Gent, A. @@aut@@ Giglietto, N. @@aut@@ Giordano, F. @@aut@@ Hanlon, W. @@aut@@ Hervet, O. @@aut@@ Incardona, S. @@aut@@ Ionica, M. @@aut@@ Jin, W. @@aut@@ Kieda, D. @@aut@@ Licciulli, F. @@aut@@ Loporchio, S. @@aut@@ Marsella, G. @@aut@@ Masone, V. @@aut@@ Mode, B.A.W. @@aut@@ Mukherjee, R. @@aut@@ Pantaleo, F.R. @@aut@@ Paoletti, R. @@aut@@ Ribeiro, D. @@aut@@ Rugliancich, A. @@aut@@ Saha, L. @@aut@@ Stiaccini, L. @@aut@@ Taylor, L.P. @@aut@@ Tosti, L. @@aut@@ Tripodo, G. @@aut@@ Vagelli, V. @@aut@@ Valentino, M. @@aut@@ Vandenbroucke, J. @@aut@@ Vassiliev, V.V. @@aut@@ Williams, D.A. @@aut@@ |
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Ambrosi, G. |
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Ambrosi, G. ddc 530 bkl 33.05 bkl 33.07 bkl 33.40 misc Silicon photomultipliers misc Cherenkov telescopes array misc Very-high-energy astrophysics Assembly and performance of SiPM arrays for the prototype SCT proposed for CTA |
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530 DE-600 33.05 bkl 33.07 bkl 33.40 bkl Assembly and performance of SiPM arrays for the prototype SCT proposed for CTA Silicon photomultipliers Cherenkov telescopes array Very-high-energy astrophysics |
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ddc 530 bkl 33.05 bkl 33.07 bkl 33.40 misc Silicon photomultipliers misc Cherenkov telescopes array misc Very-high-energy astrophysics |
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Assembly and performance of SiPM arrays for the prototype SCT proposed for CTA |
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Assembly and performance of SiPM arrays for the prototype SCT proposed for CTA |
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Ambrosi, G. Ambrosio, M. Aramo, C. Benbow, W. Bertucci, B. Bissaldi, E. Bitossi, M. Boiano, A. Bonavolontà, C. Cameron, R.A. Capasso, M. Consiglio, L. Depaoli, D. Di Pierro, F. Di Venere, L. Fiandrini, E. Furniss, A. Gent, A. Giglietto, N. Giordano, F. Hanlon, W. Hervet, O. Incardona, S. Ionica, M. Jin, W. Kieda, D. Licciulli, F. Loporchio, S. Marsella, G. Masone, V. Mode, B.A.W. Mukherjee, R. Pantaleo, F.R. Paoletti, R. Ribeiro, D. Rugliancich, A. Saha, L. Stiaccini, L. Taylor, L.P. Tosti, L. Tripodo, G. Vagelli, V. Valentino, M. Vandenbroucke, J. Vassiliev, V.V. Williams, D.A. |
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Ambrosi, G. |
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assembly and performance of sipm arrays for the prototype sct proposed for cta |
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Assembly and performance of SiPM arrays for the prototype SCT proposed for CTA |
| abstract |
The Near Ultraviolet High Density (NUV-HD) SiPMs produced by Fondazione Bruno Kessler have been employed to develop 16-pixel optical units to equip the focal plane of the prototype Schwarzschild–Couder Telescope (pSCT) proposed as a possible design for the Medium-Sized Telescope of the Cherenkov Telescope Array Observatory. After the assembly procedure, the optical units were tested and characterized to study their performance and homogeneity in terms of gain and dark count rate. In this work, we report on the assembly procedure and on the laboratory tests performed on different production of NUV-HD and the selection we made for the best quality sensors to be used in the installation on the telescope camera. Currently 36 NUV-HD3 optical units have been successfully integrated on the pSCT camera, together with 64 HAMAMATSU MPPCs. An upgrade of the pSCT camera is foreseen over the next years when the full focal plane is expected to be equipped entirely with FBK NUV-HD3 SiPMs, for a total of 11328 pixels. |
| abstractGer |
The Near Ultraviolet High Density (NUV-HD) SiPMs produced by Fondazione Bruno Kessler have been employed to develop 16-pixel optical units to equip the focal plane of the prototype Schwarzschild–Couder Telescope (pSCT) proposed as a possible design for the Medium-Sized Telescope of the Cherenkov Telescope Array Observatory. After the assembly procedure, the optical units were tested and characterized to study their performance and homogeneity in terms of gain and dark count rate. In this work, we report on the assembly procedure and on the laboratory tests performed on different production of NUV-HD and the selection we made for the best quality sensors to be used in the installation on the telescope camera. Currently 36 NUV-HD3 optical units have been successfully integrated on the pSCT camera, together with 64 HAMAMATSU MPPCs. An upgrade of the pSCT camera is foreseen over the next years when the full focal plane is expected to be equipped entirely with FBK NUV-HD3 SiPMs, for a total of 11328 pixels. |
| abstract_unstemmed |
The Near Ultraviolet High Density (NUV-HD) SiPMs produced by Fondazione Bruno Kessler have been employed to develop 16-pixel optical units to equip the focal plane of the prototype Schwarzschild–Couder Telescope (pSCT) proposed as a possible design for the Medium-Sized Telescope of the Cherenkov Telescope Array Observatory. After the assembly procedure, the optical units were tested and characterized to study their performance and homogeneity in terms of gain and dark count rate. In this work, we report on the assembly procedure and on the laboratory tests performed on different production of NUV-HD and the selection we made for the best quality sensors to be used in the installation on the telescope camera. Currently 36 NUV-HD3 optical units have been successfully integrated on the pSCT camera, together with 64 HAMAMATSU MPPCs. An upgrade of the pSCT camera is foreseen over the next years when the full focal plane is expected to be equipped entirely with FBK NUV-HD3 SiPMs, for a total of 11328 pixels. |
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Assembly and performance of SiPM arrays for the prototype SCT proposed for CTA |
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Ambrosio, M. Aramo, C. Benbow, W. Bertucci, B. Bissaldi, E. Bitossi, M. Boiano, A. Bonavolontà, C. Cameron, R.A. Capasso, M. Consiglio, L. Depaoli, D. Di Pierro, F. Di Venere, L. Fiandrini, E. Furniss, A. Gent, A. Giglietto, N. Giordano, F. Hanlon, W. Hervet, O. Incardona, S. Ionica, M. Jin, W. Kieda, D. Licciulli, F. Loporchio, S. Marsella, G. Masone, V. Mode, B.A.W. Mukherjee, R. Pantaleo, F.R. Paoletti, R. Ribeiro, D. Rugliancich, A. Saha, L. Stiaccini, L. Taylor, L.P. Tosti, L. Tripodo, G. Vagelli, V. Valentino, M. Vandenbroucke, J. Vassiliev, V.V. Williams, D.A. |
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| score |
7.3995867 |