Home > Publications database > Mirror production for the Cherenkov telescopes of the ASTRI mini-array and the MST project for the Cherenkov Telescope Array > print

001     485756
005     20230214113316.0
024 7 _ |a Palombara:2019gpp
|2 INSPIRETeX
024 7 _ |a inspire:1769170
|2 inspire
024 7 _ |a arXiv:2201.08103
|2 arXiv
024 7 _ |a altmetric:121325066
|2 altmetric
037 _ _ |a PUBDB-2022-06822
041 _ _ |a English
082 _ _ |a 530
088 _ _ |a arXiv:2201.08103
|2 arXiv
100 1 _ |a La Palombara, Nicola
|0 P:(DE-HGF)0
|b 0
|e Corresponding author
245 _ _ |a Mirror production for the Cherenkov telescopes of the ASTRI mini-array and the MST project for the Cherenkov Telescope Array
260 _ _ |c 2022
336 7 _ |a Preprint
|b preprint
|m preprint
|0 PUB:(DE-HGF)25
|s 1668763255_22386
|2 PUB:(DE-HGF)
336 7 _ |a WORKING_PAPER
|2 ORCID
336 7 _ |a Electronic Article
|0 28
|2 EndNote
336 7 _ |a preprint
|2 DRIVER
336 7 _ |a ARTICLE
|2 BibTeX
336 7 _ |a Output Types/Working Paper
|2 DataCite
500 _ _ |a Accepted for publication in the SPIE Journal of Astronomical Telescopes, Instruments, and Systems (JATIS); 29 pages, 17 figures, 4 tables, quite a lot of stress, infinite patience. Published online on February 3, 2022 at http://dx.doi.org/10.1117/1.JATIS.8.1.014005
520 _ _ |a The Cherenkov Telescope Array (CTA) is the next ground-based γ-ray observatory in the TeV γ-ray spectral region operating with the Imaging Atmospheric Cherenkov Technique. It is based on almost 70 telescopes of different class diameters - LST, MST and SST of 23, 12, and 4 m, respectively - to be installed in two sites in the two hemispheres (at La Palma, Canary Islands, and near Paranal, Chile). Several thousands of reflecting mirror tiles larger than 1 m$^2$ will be produced for realizing the segmented primary mirrors of a so large number of telescopes. Almost in parallel, the ASTRI Mini-Array (MA) is being implemented in Tenerife (Canary Islands), composed of nine 4 m diameter dual-mirror Cherenkov telescopes (very similar to the SSTs). We completed the mirror production for all nine telescopes of the ASTRI MA and two MST telescopes (400 segments in total) using the cold glass slumping replication technology. The results related to the quality achieved with a so large-scale production are presented, also discussing the adopted testing methods and approaches. They will be very useful for the adoption and optimization of the quality assurance process for the huge production (almost 3000 m2 of reflecting surface) of the MST and SST CTA telescopes.
536 _ _ |a 613 - Matter and Radiation from the Universe (POF4-613)
|0 G:(DE-HGF)POF4-613
|c POF4-613
|f POF IV
|x 0
588 _ _ |a Dataset connected to CrossRef, INSPIRE, Journals: bib-pubdb1.desy.de
650 _ 7 |a activity report
|2 INSPIRE
650 _ 7 |a mirror
|2 INSPIRE
650 _ 7 |a Cherenkov Telescope Array
|2 INSPIRE
650 _ 7 |a quality: monitoring
|2 INSPIRE
650 _ 7 |a Cherenkov counter
|2 INSPIRE
650 _ 7 |a fabrication
|2 INSPIRE
650 _ 7 |a performance
|2 INSPIRE
650 _ 7 |a Mirrors
|2 autogen
650 _ 7 |a Atmospheric Cherenkov telescopes
|2 autogen
650 _ 7 |a Telescopes
|2 autogen
650 _ 7 |a Reflectivity
|2 autogen
650 _ 7 |a Glasses
|2 autogen
650 _ 7 |a Point spread functions
|2 autogen
650 _ 7 |a Spherical lenses
|2 autogen
650 _ 7 |a Aluminum
|2 autogen
650 _ 7 |a Coating
|2 autogen
650 _ 7 |a Solids
|2 autogen
650 _ 7 |a CTA
|2 autogen
650 _ 7 |a ASTRI
|2 autogen
650 _ 7 |a dual mirror
|2 autogen
650 _ 7 |a cold-slumping technology
|2 autogen
650 _ 7 |a hot-slumpìing technology
|2 autogen
650 _ 7 |a coating
|2 autogen
650 _ 7 |a quality assurance
|2 autogen
693 _ _ |0 EXP:(DE-H253)CTA-20150101
|5 EXP:(DE-H253)CTA-20150101
|e Cherenkov Telescope Array
|x 0
700 1 _ |a Sironi, Giorgia
|0 G.Sironi.2
|b 1
700 1 _ |a Giro, Enrico
|0 E.Giro.1
|b 2
700 1 _ |a Scuderi, Salvatore
|0 S.Scuderi.5
|b 3
700 1 _ |a Canestrari, Rodolfo
|0 R.Canestrari.1
|b 4
700 1 _ |a Iovenitti, Simone
|0 S.Iovenitti.1
|b 5
700 1 _ |a Garczarczyk, Markus
|0 P:(DE-H253)PIP1019066
|b 6
|u desy
700 1 _ |a Krause, Maria
|0 P:(DE-H253)PIP1012636
|b 7
|u desy
700 1 _ |a Diebold, Sebastian
|0 S.Diebold.3
|b 8
700 1 _ |a Millul, Rachele
|0 Rachele.Millul.1
|b 9
700 1 _ |a Marioni, Fabio
|0 O.F.Marioni.1
|b 10
700 1 _ |a Missaglia, Nadia
|0 N.Missaglia.1
|b 11
700 1 _ |a Redaelli, Matteo
|0 M.Redaelli.1
|b 12
700 1 _ |a Valsecchi, Giuseppe
|0 G.Valsecchi.1
|b 13
700 1 _ |a Zocchi, Fabio
|0 F.Zocchi.1
|b 14
700 1 _ |a Zanoni, Adelfio
|0 A.Zanoni.2
|b 15
700 1 _ |a Pareschi, Giovanni
|0 G.Pareschi.1
|b 16
856 4 _ |u https://bib-pubdb1.desy.de/record/485756/files/2201.08103.pdf
|y Restricted
856 4 _ |u https://bib-pubdb1.desy.de/record/485756/files/2201.08103.pdf?subformat=pdfa
|x pdfa
|y Restricted
909 C O |o oai:bib-pubdb1.desy.de:485756
|p VDB
910 1 _ |a Deutsches Elektronen-Synchrotron
|0 I:(DE-588b)2008985-5
|k DESY
|b 6
|6 P:(DE-H253)PIP1019066
910 1 _ |a Deutsches Elektronen-Synchrotron
|0 I:(DE-588b)2008985-5
|k DESY
|b 7
|6 P:(DE-H253)PIP1012636
913 1 _ |a DE-HGF
|b Forschungsbereich Materie
|l Matter and the Universe
|1 G:(DE-HGF)POF4-610
|0 G:(DE-HGF)POF4-613
|3 G:(DE-HGF)POF4
|2 G:(DE-HGF)POF4-600
|4 G:(DE-HGF)POF
|v Matter and Radiation from the Universe
|x 0
914 1 _ |y 2022
915 _ _ |a Published
|0 StatID:(DE-HGF)0580
|2 StatID
920 1 _ |0 I:(DE-H253)CTAI-20201126
|k CTAI
|l CTAI
|x 0
980 _ _ |a preprint
980 _ _ |a VDB
980 _ _ |a I:(DE-H253)CTAI-20201126
980 _ _ |a UNRESTRICTED

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