Very large SiPM arrays with aggregated output
In this work we will document the design and the performances of a SiPM-based photo-detector with a surface area of 100 cm 2 conceived to operate as a replacement for PMTs. The signals from 94 SiPMs are summed up to produce an aggregated output that exhibits in liquid nitrogen a dark count rate (DCR...
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| Veröffentlicht in: | Journal of instrumentation 2022-05, Vol.17 (5), p.P05038 |
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| creator | Razeto, A. Acerbi, F. Camillo, V. Carlini, M. Consiglio, L. Flammini, A. Galbiati, C. Ghiano, C. Gola, A. Horikawa, S. Kachru, P. Kochanek, I. Kondo, K. Korga, G. Mazzi, A. Moharana, A. Paternoster, G. Sablone, D. Basco, A. Bocci, V. Bonivento, W. Bottino, B. Caminata, A. Copello, S. Di Capua, F. Giovanetti, G.K. La Commara, M. Musico, P. Paoloni, E. Rignanese, L.P. Sanfilippo, S. Savarese, C. Suvorov, Y. Testera, G. |
| description | In this work we will document the design and the performances of a SiPM-based photo-detector with a surface area of 100 cm
2
conceived to operate as a replacement for PMTs. The signals from 94 SiPMs are summed up to produce an aggregated output that exhibits in liquid nitrogen a dark count rate (DCR) lower than 100 cps over the entire surface, a signal to noise ratio better than 13, and a timing resolution better than 5.5 ns. The module feeds about 360 mW at 5 V with a dynamic range in excess of 500 photo-electrons on a 100 Ω differential line. The unit can also operate at room temperature, at the cost of an increase of DCR to 10
8
cps. |
| doi_str_mv | 10.1088/1748-0221/17/05/P05038 |
| format | Article |
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2
conceived to operate as a replacement for PMTs. The signals from 94 SiPMs are summed up to produce an aggregated output that exhibits in liquid nitrogen a dark count rate (DCR) lower than 100 cps over the entire surface, a signal to noise ratio better than 13, and a timing resolution better than 5.5 ns. The module feeds about 360 mW at 5 V with a dynamic range in excess of 500 photo-electrons on a 100 Ω differential line. The unit can also operate at room temperature, at the cost of an increase of DCR to 10
8
cps.</description><identifier>ISSN: 1748-0221</identifier><identifier>EISSN: 1748-0221</identifier><identifier>DOI: 10.1088/1748-0221/17/05/P05038</identifier><language>eng</language><publisher>Bristol: IOP Publishing</publisher><subject>Front-end electronics for detector readout ; Large detector systems for particle and astroparticle physics ; Liquid nitrogen ; Photon detectors for UV, visible and IR photons (solid-state) ; Photon detectors for UV, visible and IR photons (solid-state) (PIN diodes, APDs, Si-PMTs, G-APDs, CCDs, EBCCDs, EMCCDs, CMOS imagers, etc) ; Room temperature ; Signal to noise ratio</subject><ispartof>Journal of instrumentation, 2022-05, Vol.17 (5), p.P05038</ispartof><rights>2022 IOP Publishing Ltd and Sissa Medialab</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c414t-98f959f2232f4a8cd271dae468640d315289597a285074e63a36c9ab7c1e0c73</citedby><cites>FETCH-LOGICAL-c414t-98f959f2232f4a8cd271dae468640d315289597a285074e63a36c9ab7c1e0c73</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://iopscience.iop.org/article/10.1088/1748-0221/17/05/P05038/pdf$$EPDF$$P50$$Giop$$H</linktopdf><link.rule.ids>314,776,780,27903,27904,53825,53872</link.rule.ids></links><search><creatorcontrib>Razeto, A.</creatorcontrib><creatorcontrib>Acerbi, F.</creatorcontrib><creatorcontrib>Camillo, V.</creatorcontrib><creatorcontrib>Carlini, M.</creatorcontrib><creatorcontrib>Consiglio, L.</creatorcontrib><creatorcontrib>Flammini, A.</creatorcontrib><creatorcontrib>Galbiati, C.</creatorcontrib><creatorcontrib>Ghiano, C.</creatorcontrib><creatorcontrib>Gola, A.</creatorcontrib><creatorcontrib>Horikawa, S.</creatorcontrib><creatorcontrib>Kachru, P.</creatorcontrib><creatorcontrib>Kochanek, I.</creatorcontrib><creatorcontrib>Kondo, K.</creatorcontrib><creatorcontrib>Korga, G.</creatorcontrib><creatorcontrib>Mazzi, A.</creatorcontrib><creatorcontrib>Moharana, A.</creatorcontrib><creatorcontrib>Paternoster, G.</creatorcontrib><creatorcontrib>Sablone, D.</creatorcontrib><creatorcontrib>Basco, A.</creatorcontrib><creatorcontrib>Bocci, V.</creatorcontrib><creatorcontrib>Bonivento, W.</creatorcontrib><creatorcontrib>Bottino, B.</creatorcontrib><creatorcontrib>Caminata, A.</creatorcontrib><creatorcontrib>Copello, S.</creatorcontrib><creatorcontrib>Di Capua, F.</creatorcontrib><creatorcontrib>Giovanetti, G.K.</creatorcontrib><creatorcontrib>La Commara, M.</creatorcontrib><creatorcontrib>Musico, P.</creatorcontrib><creatorcontrib>Paoloni, E.</creatorcontrib><creatorcontrib>Rignanese, L.P.</creatorcontrib><creatorcontrib>Sanfilippo, S.</creatorcontrib><creatorcontrib>Savarese, C.</creatorcontrib><creatorcontrib>Suvorov, Y.</creatorcontrib><creatorcontrib>Testera, G.</creatorcontrib><title>Very large SiPM arrays with aggregated output</title><title>Journal of instrumentation</title><addtitle>J. Instrum</addtitle><description>In this work we will document the design and the performances of a SiPM-based photo-detector with a surface area of 100 cm
2
conceived to operate as a replacement for PMTs. The signals from 94 SiPMs are summed up to produce an aggregated output that exhibits in liquid nitrogen a dark count rate (DCR) lower than 100 cps over the entire surface, a signal to noise ratio better than 13, and a timing resolution better than 5.5 ns. The module feeds about 360 mW at 5 V with a dynamic range in excess of 500 photo-electrons on a 100 Ω differential line. The unit can also operate at room temperature, at the cost of an increase of DCR to 10
8
cps.</description><subject>Front-end electronics for detector readout</subject><subject>Large detector systems for particle and astroparticle physics</subject><subject>Liquid nitrogen</subject><subject>Photon detectors for UV, visible and IR photons (solid-state)</subject><subject>Photon detectors for UV, visible and IR photons (solid-state) (PIN diodes, APDs, Si-PMTs, G-APDs, CCDs, EBCCDs, EMCCDs, CMOS imagers, etc)</subject><subject>Room temperature</subject><subject>Signal to noise ratio</subject><issn>1748-0221</issn><issn>1748-0221</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2022</creationdate><recordtype>article</recordtype><recordid>eNqFUE1LxDAUDKLguvoXJOBNqH35bHqUxS9YccHFa4hpWrus25q0SP-9KRXdg-DpDbyZeW8GoXMCVwSUSknGVQKUkohSEOkKBDB1gGY_i8M9fIxOQtgAiFxwmKHkxfkBb42vHH6uV4_YeG-GgD_r7g2bqvKuMp0rcNN3bd-doqPSbIM7-55ztL69WS_uk-XT3cPieplYTniX5KrMRV5SymjJjbIFzUhhHJdKcigYEVTFfWaoEpBxJ5lh0ubmNbPEgc3YHF1Mtq1vPnoXOr1per-LFzWVMheKMcEjS04s65sQvCt16-t34wdNQI_N6DG0HkNHpEHoqZkopJOwbtpf539Fl3-INvUufrdP1G1Rsi_VonFP</recordid><startdate>20220501</startdate><enddate>20220501</enddate><creator>Razeto, A.</creator><creator>Acerbi, F.</creator><creator>Camillo, V.</creator><creator>Carlini, M.</creator><creator>Consiglio, L.</creator><creator>Flammini, A.</creator><creator>Galbiati, C.</creator><creator>Ghiano, C.</creator><creator>Gola, A.</creator><creator>Horikawa, S.</creator><creator>Kachru, P.</creator><creator>Kochanek, I.</creator><creator>Kondo, K.</creator><creator>Korga, G.</creator><creator>Mazzi, A.</creator><creator>Moharana, A.</creator><creator>Paternoster, G.</creator><creator>Sablone, D.</creator><creator>Basco, A.</creator><creator>Bocci, V.</creator><creator>Bonivento, W.</creator><creator>Bottino, B.</creator><creator>Caminata, A.</creator><creator>Copello, S.</creator><creator>Di Capua, F.</creator><creator>Giovanetti, G.K.</creator><creator>La Commara, M.</creator><creator>Musico, P.</creator><creator>Paoloni, E.</creator><creator>Rignanese, L.P.</creator><creator>Sanfilippo, S.</creator><creator>Savarese, C.</creator><creator>Suvorov, Y.</creator><creator>Testera, G.</creator><general>IOP Publishing</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7U5</scope><scope>8FD</scope><scope>L7M</scope></search><sort><creationdate>20220501</creationdate><title>Very large SiPM arrays with aggregated output</title><author>Razeto, A. ; 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Instrum</addtitle><date>2022-05-01</date><risdate>2022</risdate><volume>17</volume><issue>5</issue><spage>P05038</spage><pages>P05038-</pages><issn>1748-0221</issn><eissn>1748-0221</eissn><abstract>In this work we will document the design and the performances of a SiPM-based photo-detector with a surface area of 100 cm
2
conceived to operate as a replacement for PMTs. The signals from 94 SiPMs are summed up to produce an aggregated output that exhibits in liquid nitrogen a dark count rate (DCR) lower than 100 cps over the entire surface, a signal to noise ratio better than 13, and a timing resolution better than 5.5 ns. The module feeds about 360 mW at 5 V with a dynamic range in excess of 500 photo-electrons on a 100 Ω differential line. The unit can also operate at room temperature, at the cost of an increase of DCR to 10
8
cps.</abstract><cop>Bristol</cop><pub>IOP Publishing</pub><doi>10.1088/1748-0221/17/05/P05038</doi><tpages>13</tpages></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 1748-0221 |
| ispartof | Journal of instrumentation, 2022-05, Vol.17 (5), p.P05038 |
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| language | eng |
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| source | Institute of Physics Journals |
| subjects | Front-end electronics for detector readout Large detector systems for particle and astroparticle physics Liquid nitrogen Photon detectors for UV, visible and IR photons (solid-state) Photon detectors for UV, visible and IR photons (solid-state) (PIN diodes, APDs, Si-PMTs, G-APDs, CCDs, EBCCDs, EMCCDs, CMOS imagers, etc) Room temperature Signal to noise ratio |
| title | Very large SiPM arrays with aggregated output |
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