Novel Silicon Photomultipliers suitable for Dual-Mirror Small-Sized Telescopes of the Cherenkov Telescope Array
Many of the characteristics of Silicon Photomultipliers (SiPMs), such as high Photon Detection Efficiency (PDE), are well matched to the requirements of the cameras of the Small-Sized Telescopes (SSTs) proposed for the Cherenkov Telescope Array. In fact, compared to a single mirror, the double mirro...
Saved in:
Published in | arXiv.org |
---|---|
Main Authors | , , , |
Format | Paper Journal Article |
Language | English |
Published |
Ithaca
Cornell University Library, arXiv.org
23.08.2018
|
Subjects | |
Online Access | Get full text |
Cover
Loading…
Abstract | Many of the characteristics of Silicon Photomultipliers (SiPMs), such as high Photon Detection Efficiency (PDE), are well matched to the requirements of the cameras of the Small-Sized Telescopes (SSTs) proposed for the Cherenkov Telescope Array. In fact, compared to a single mirror, the double mirror Schwarzschild Couder configuration provides a much better Point Spread Function over a large field of view. It allows better correction of aberrations at large off axis angles and facilitates the construction of compact telescopes. Moreover, the small plate scale of the dual-mirror SSTs allows the use of SiPM detectors despite their small pixel sizes. These sensors have two further advantages compared to the Photo Multipliers Tubes: the low cost and the possibility to observe in very high Night Sky Background (NSB) light level without any damage. However, one area in which SiPM performance has required improvement is Optical CrossTalk (OCT), where multiple avalanches are induced by a single impinging photon. OCT, coupled with the typical NSB rate of 25 MCnts/s per pixel during Cherenkov observations, can place severe constraints on the triggering capability of the cameras. This paper describes the performance of novel Low Voltage Reverse (LVR) 2nd and 3rd generation Multi Pixel Photon Counters manufactured by Hamamatsu Photonics. These are designed to have both enhanced PDE and reduced OCT. Two 7 x 7 mm2 S14520 LVR2 MPPCs with 75 um microcells are tested and compared with detectors of the same pixel size with 50 um microcells. A comparative analysis of a 3 x 3 mm2 S14520 LVR2 device and an S14520 LVR3 device is also carried out, demonstrating that the LVR3 gives better photon detection in the 240 380 nm wavelength range. Finally, the effect of an infrared filter on the OCT is analysed. |
---|---|
AbstractList | Nuclear Instruments and Methods in Physics Research section A - 13
August 2018 Many of the characteristics of Silicon Photomultipliers (SiPMs), such as high
Photon Detection Efficiency (PDE), are well matched to the requirements of the
cameras of the Small-Sized Telescopes (SSTs) proposed for the Cherenkov
Telescope Array. In fact, compared to a single mirror, the double mirror
Schwarzschild Couder configuration provides a much better Point Spread Function
over a large field of view. It allows better correction of aberrations at large
off axis angles and facilitates the construction of compact telescopes.
Moreover, the small plate scale of the dual-mirror SSTs allows the use of SiPM
detectors despite their small pixel sizes. These sensors have two further
advantages compared to the Photo Multipliers Tubes: the low cost and the
possibility to observe in very high Night Sky Background (NSB) light level
without any damage. However, one area in which SiPM performance has required
improvement is Optical CrossTalk (OCT), where multiple avalanches are induced
by a single impinging photon. OCT, coupled with the typical NSB rate of 25
MCnts/s per pixel during Cherenkov observations, can place severe constraints
on the triggering capability of the cameras. This paper describes the
performance of novel Low Voltage Reverse (LVR) 2nd and 3rd generation Multi
Pixel Photon Counters manufactured by Hamamatsu Photonics. These are designed
to have both enhanced PDE and reduced OCT. Two 7 x 7 mm2 S14520 LVR2 MPPCs with
75 um microcells are tested and compared with detectors of the same pixel size
with 50 um microcells. A comparative analysis of a 3 x 3 mm2 S14520 LVR2 device
and an S14520 LVR3 device is also carried out, demonstrating that the LVR3
gives better photon detection in the 240 380 nm wavelength range. Finally, the
effect of an infrared filter on the OCT is analysed. Many of the characteristics of Silicon Photomultipliers (SiPMs), such as high Photon Detection Efficiency (PDE), are well matched to the requirements of the cameras of the Small-Sized Telescopes (SSTs) proposed for the Cherenkov Telescope Array. In fact, compared to a single mirror, the double mirror Schwarzschild Couder configuration provides a much better Point Spread Function over a large field of view. It allows better correction of aberrations at large off axis angles and facilitates the construction of compact telescopes. Moreover, the small plate scale of the dual-mirror SSTs allows the use of SiPM detectors despite their small pixel sizes. These sensors have two further advantages compared to the Photo Multipliers Tubes: the low cost and the possibility to observe in very high Night Sky Background (NSB) light level without any damage. However, one area in which SiPM performance has required improvement is Optical CrossTalk (OCT), where multiple avalanches are induced by a single impinging photon. OCT, coupled with the typical NSB rate of 25 MCnts/s per pixel during Cherenkov observations, can place severe constraints on the triggering capability of the cameras. This paper describes the performance of novel Low Voltage Reverse (LVR) 2nd and 3rd generation Multi Pixel Photon Counters manufactured by Hamamatsu Photonics. These are designed to have both enhanced PDE and reduced OCT. Two 7 x 7 mm2 S14520 LVR2 MPPCs with 75 um microcells are tested and compared with detectors of the same pixel size with 50 um microcells. A comparative analysis of a 3 x 3 mm2 S14520 LVR2 device and an S14520 LVR3 device is also carried out, demonstrating that the LVR3 gives better photon detection in the 240 380 nm wavelength range. Finally, the effect of an infrared filter on the OCT is analysed. |
Author | Romeo, Giuseppe Bonanno, Giovanni Sironi, Giorgia Timpanaro, Maria Cristina |
Author_xml | – sequence: 1 givenname: Giuseppe surname: Romeo fullname: Romeo, Giuseppe – sequence: 2 givenname: Giovanni surname: Bonanno fullname: Bonanno, Giovanni – sequence: 3 givenname: Giorgia surname: Sironi fullname: Sironi, Giorgia – sequence: 4 givenname: Maria surname: Timpanaro middlename: Cristina fullname: Timpanaro, Maria Cristina |
BackLink | https://doi.org/10.1016/j.nima.2018.08.035$$DView published paper (Access to full text may be restricted) https://doi.org/10.48550/arXiv.1806.00703$$DView paper in arXiv |
BookMark | eNpFkFtLAzEUhIMoWGt_gE8GfN6ay2Yvj6VeoV6gfV_ONic0Nd2syW6x_nprK_g0AzMMw3dBThvfICFXnI3TQil2C-HLbse8YNmYsZzJEzIQUvKkSIU4J6MY14wxkeVCKTkg_tVv0dG5dXbpG_q-8p3f9K6zrbMYIo297aB2SI0P9K4Hl7zYEPZ-vgHnkrn9Rk0X6DAufYuRekO7FdLpCgM2H377n9FJCLC7JGcGXMTRnw7J4uF-MX1KZm-Pz9PJLAEl8kQZLbVGXUCpOIgl1JKnUkEpTFHwVGMt6lqVhvNM1wCgjckBuBFZoTRTtRyS6-PsgUbVBruBsKt-qVQHKvvGzbHRBv_ZY-yqte9Ds_9UCZZLqQQrc_kDQ3xpdA |
ContentType | Paper Journal Article |
Copyright | 2018. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. http://arxiv.org/licenses/nonexclusive-distrib/1.0 |
Copyright_xml | – notice: 2018. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. – notice: http://arxiv.org/licenses/nonexclusive-distrib/1.0 |
DBID | 8FE 8FG ABJCF ABUWG AFKRA AZQEC BENPR BGLVJ CCPQU DWQXO HCIFZ L6V M7S PIMPY PQEST PQQKQ PQUKI PRINS PTHSS GOX |
DOI | 10.48550/arxiv.1806.00703 |
DatabaseName | ProQuest SciTech Collection ProQuest Technology Collection Materials Science & Engineering Collection ProQuest Central (Alumni) ProQuest Central UK/Ireland ProQuest Central Essentials AUTh Library subscriptions: ProQuest Central Technology Collection ProQuest One Community College ProQuest Central SciTech Premium Collection (Proquest) (PQ_SDU_P3) ProQuest Engineering Collection ProQuest Engineering Database Publicly Available Content Database ProQuest One Academic Eastern Edition (DO NOT USE) ProQuest One Academic ProQuest One Academic UKI Edition ProQuest Central China Engineering Collection arXiv.org |
DatabaseTitle | Publicly Available Content Database Engineering Database Technology Collection ProQuest Central Essentials ProQuest One Academic Eastern Edition ProQuest Central (Alumni Edition) SciTech Premium Collection ProQuest One Community College ProQuest Technology Collection ProQuest SciTech Collection ProQuest Central China ProQuest Central ProQuest Engineering Collection ProQuest One Academic UKI Edition ProQuest Central Korea Materials Science & Engineering Collection ProQuest One Academic Engineering Collection |
DatabaseTitleList | Publicly Available Content Database |
Database_xml | – sequence: 1 dbid: GOX name: arXiv.org url: http://arxiv.org/find sourceTypes: Open Access Repository – sequence: 2 dbid: 8FG name: ProQuest Technology Collection url: https://search.proquest.com/technologycollection1 sourceTypes: Aggregation Database |
DeliveryMethod | fulltext_linktorsrc |
Discipline | Physics |
EISSN | 2331-8422 |
ExternalDocumentID | 1806_00703 |
Genre | Working Paper/Pre-Print |
GroupedDBID | 8FE 8FG ABJCF ABUWG AFKRA ALMA_UNASSIGNED_HOLDINGS AZQEC BENPR BGLVJ CCPQU DWQXO FRJ HCIFZ L6V M7S M~E PIMPY PQEST PQQKQ PQUKI PRINS PTHSS GOX |
ID | FETCH-LOGICAL-a527-5fd3dded8a951a2cab31435a92f8814deb2bb59f116dbaaadff7aa1f2685d05b3 |
IEDL.DBID | GOX |
IngestDate | Mon Jan 08 05:39:33 EST 2024 Thu Oct 10 18:11:49 EDT 2024 |
IsDoiOpenAccess | true |
IsOpenAccess | true |
IsPeerReviewed | false |
IsScholarly | false |
Language | English |
LinkModel | DirectLink |
MergedId | FETCHMERGED-LOGICAL-a527-5fd3dded8a951a2cab31435a92f8814deb2bb59f116dbaaadff7aa1f2685d05b3 |
OpenAccessLink | https://arxiv.org/abs/1806.00703 |
PQID | 2073352097 |
PQPubID | 2050157 |
ParticipantIDs | arxiv_primary_1806_00703 proquest_journals_2073352097 |
PublicationCentury | 2000 |
PublicationDate | 20180823 |
PublicationDateYYYYMMDD | 2018-08-23 |
PublicationDate_xml | – month: 08 year: 2018 text: 20180823 day: 23 |
PublicationDecade | 2010 |
PublicationPlace | Ithaca |
PublicationPlace_xml | – name: Ithaca |
PublicationTitle | arXiv.org |
PublicationYear | 2018 |
Publisher | Cornell University Library, arXiv.org |
Publisher_xml | – name: Cornell University Library, arXiv.org |
SSID | ssj0002672553 |
Score | 1.7098206 |
SecondaryResourceType | preprint |
Snippet | Many of the characteristics of Silicon Photomultipliers (SiPMs), such as high Photon Detection Efficiency (PDE), are well matched to the requirements of the... Nuclear Instruments and Methods in Physics Research section A - 13 August 2018 Many of the characteristics of Silicon Photomultipliers (SiPMs), such as high... |
SourceID | arxiv proquest |
SourceType | Open Access Repository Aggregation Database |
SubjectTerms | Cameras Crosstalk Detectors Field of view Infrared analysis Infrared filters Low voltage Night sky Photomultiplier tubes Photon avalanches Photon counters Photonics Physics - High Energy Physics - Experiment Physics - Instrumentation and Methods for Astrophysics Pixels Point spread functions Silicon Telescopes |
SummonAdditionalLinks | – databaseName: ProQuest Technology Collection dbid: 8FG link: http://utb.summon.serialssolutions.com/2.0.0/link/0/eLvHCXMwfV1JSwMxFA7aInhzxaVKDl6jncxkkjmJVGsRWgqt0NuQFYtjU2faov56k3S0B8FbSG7fI-99bwfgSmlnRoyhyBhFUaI0QYIohRKRJZLGQjLq-537g7T3nDxNyKQOuFV1WeWPTgyKWlnpY-Q-EuLbg9oZvZ2_I781ymdX6xUa26AZYUq988W6j78xFpxSx5jjdTIzjO664eXHdHUdsZCDoH5VVjNc_VHFwb5090BzyOe63AdbenYAdkJZpqwOgR3YlS7gaFo4gc3g8MUubF0C6FdYw2rpXHtRaOioJ7xf8gL1p2XpzqM3XhRoNP3SCo61n9lk57qC1kBH-GDnxTf5vdrV5g3elSX_PALj7sO400P1igTECaaIGBU7_aQYd0SJY8lF7PkPz7BhLHLICywEyUwUpUpwzpWTCueRwSkjqk1EfAwaMzvTJwBGmdQSy4wRppOMqkzzJDZxWzoPkgqGT8FJACqfr6dg5B7DPGB4Clo_2OX1D6jyjbzO_n8-B7uOhPgx2QjHLdBYlEt94Qz9QlwGaX4DSuWrdA priority: 102 providerName: ProQuest |
Title | Novel Silicon Photomultipliers suitable for Dual-Mirror Small-Sized Telescopes of the Cherenkov Telescope Array |
URI | https://www.proquest.com/docview/2073352097 https://arxiv.org/abs/1806.00703 |
hasFullText | 1 |
inHoldings | 1 |
isFullTextHit | |
isPrint | |
link | http://utb.summon.serialssolutions.com/2.0.0/link/0/eLvHCXMwdV3PS8MwFA5zXryIorLpHDl4Da5ps6RHnfuBsDnchN1K0iRsWJvRbkM9-LebtB07iJdQklcK3yt5X8h73wPgTiobRrSmSGtJUSAVQYJIiQIRBjH1Rcyoq3ceT7qjt-B5QRY1APe1MDz7XO1KfWCR33usuCugTs7zCGOXsjV8WZSXk4UUV2V_sLMcs5j6s7UW8WJwBk4rogcfSs-cg5pKL4CZmJ1K4GyVWAekcLo0G1Ol9LmW1DDf2qO6SBS0VBI-bXmCxqsss8-zD54kaLb6VhLOldNgMmuVQ6OhJXCwt3RFe-9md1izH8741yWYD_rz3ghVLQ8QJ5gioqVv9xvJuCU-HMdc-I7P8BBrxjyLpMBCkFB7XlcKzrm0KHPuadxlRHaI8K9APTWpagDohbGKcRwywlQQUhkqHvja78T2REgFw03QKICK1qWqReQwjAoMm6C1xy6q_ug8wq67o8uZodf_v3kDTiyhcJLXCPstUN9kW3Vrg_ZGtMERGwzb4PixP5m-tgs_2nH80_8FUrSefg |
link.rule.ids | 228,230,783,787,888,12777,21400,27937,33385,33756,43612,43817 |
linkProvider | Cornell University |
linkToHtml | http://utb.summon.serialssolutions.com/2.0.0/link/0/eLvHCXMwfV1JTwIxFG4UYvTmGlDUHrxWmc6Udk5GUYMLhAgm3CZdA3GkOANE_fW246gHE29Ne_te-t73dgBOlHZmxBiKjFEURUoTJIhSKBJxJGkoJKO-37nba3WeorsRGZUBt7wsq_zWiYWiVlb6GLmPhPj2oGZMz2evyG-N8tnVcoXGKqj6UVXO-apeXvf6jz9RFtyijjOHX-nMYnjXGc_eJsvTgBVZCOqXZVWLqz_KuLAwN5ug2ucznW2BFT3dBmtFYabMd4Dt2aVO4WCSOpFNYX9s57YsAvRLrGG-cM69SDV05BNeLXiKupMsc-fBC09TNJh8aAWH2k9tsjOdQ2ugo3ywPfZtfs92-fsGL7KMv--C4c31sN1B5ZIExAmmiBgVOg2lGHdUiWPJRegZEI-xYSxw2AssBIlNELSU4JwrJxfOA4NbjKgmEeEeqEztVNcADGKpJZYxI0xHMVWx5lFowqZ0PiQVDNdBrQAqmX3NwUg8hkmBYR00vrFLyj-QJ78S2___-Risd4bdh-Thtnd_ADYcJfFDsxEOG6Ayzxb60Jn9uTgqZfsJbiCvxQ |
openUrl | ctx_ver=Z39.88-2004&ctx_enc=info%3Aofi%2Fenc%3AUTF-8&rfr_id=info%3Asid%2Fsummon.serialssolutions.com&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.atitle=Novel+Silicon+Photomultipliers+suitable+for+Dual-Mirror+Small-Sized+Telescopes+of+the+Cherenkov+Telescope+Array&rft.jtitle=arXiv.org&rft.au=Romeo%2C+Giuseppe&rft.au=Bonanno%2C+Giovanni&rft.au=Sironi%2C+Giorgia&rft.au=Timpanaro%2C+Maria+Cristina&rft.date=2018-08-23&rft.pub=Cornell+University+Library%2C+arXiv.org&rft.eissn=2331-8422&rft_id=info:doi/10.48550%2Farxiv.1806.00703 |