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000485236 0247_ $$2doi$$a10.1117/1.JATIS.8.1.014005
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000485236 0247_ $$2arXiv$$aarXiv:2201.08103
000485236 0247_ $$2datacite_doi$$a10.3204/PUBDB-2022-06623
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000485236 088__ $$2arXiv$$aarXiv:2201.08103
000485236 1001_ $$0N.L.Palombara.1$$aPalombara, Nicola La$$b0$$eCorresponding author
000485236 1112_ $$aSPIE Optical Engineering + Applications$$cSan Diego$$d2019-08-11 - 2019-08-15$$wUnited States
000485236 245__ $$aMirror production for the Cherenkov telescopes of the ASTRI mini-array and the MST project for the Cherenkov Telescope Array
000485236 260__ $$a[Bellingham, Wash.]$$bSPIE$$c2022
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000485236 500__ $$aAccepted for publication in the SPIE Journal of Astronomical Telescopes, Instruments, and Systems (JATIS); 29 pages, 17 figures, 4 tables, quite a lot of stress, infinite patience. Published online on February 3, 2022 at http://dx.doi.org/10.1117/1.JATIS.8.1.014005
000485236 520__ $$aThe 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 m$^2$ of reflecting surface) of the MST and SST CTA telescopes. 
000485236 536__ $$0G:(DE-HGF)POF4-613$$a613 - Matter and Radiation from the Universe (POF4-613)$$cPOF4-613$$fPOF IV$$x0
000485236 588__ $$aDataset connected to CrossRef, INSPIRE, Journals: bib-pubdb1.desy.de
000485236 650_7 $$2INSPIRE$$aactivity report
000485236 650_7 $$2INSPIRE$$amirror
000485236 650_7 $$2INSPIRE$$aCherenkov Telescope Array
000485236 650_7 $$2INSPIRE$$aquality: monitoring
000485236 650_7 $$2INSPIRE$$aCherenkov counter
000485236 650_7 $$2INSPIRE$$afabrication
000485236 650_7 $$2INSPIRE$$aperformance
000485236 650_7 $$2autogen$$aMirrors
000485236 650_7 $$2autogen$$aAtmospheric Cherenkov telescopes
000485236 650_7 $$2autogen$$aTelescopes
000485236 650_7 $$2autogen$$aReflectivity
000485236 650_7 $$2autogen$$aGlasses
000485236 650_7 $$2autogen$$aPoint spread functions
000485236 650_7 $$2autogen$$aSpherical lenses
000485236 650_7 $$2autogen$$aAluminum
000485236 650_7 $$2autogen$$aCoating
000485236 650_7 $$2autogen$$aSolids
000485236 650_7 $$2autogen$$aCTA
000485236 650_7 $$2autogen$$aASTRI
000485236 650_7 $$2autogen$$adual mirror
000485236 650_7 $$2autogen$$acold-slumping technology
000485236 650_7 $$2autogen$$ahot-slumpìing technology
000485236 650_7 $$2autogen$$acoating
000485236 650_7 $$2autogen$$aquality assurance
000485236 693__ $$0EXP:(DE-H253)CTA-20150101$$5EXP:(DE-H253)CTA-20150101$$eCherenkov Telescope Array$$x0
000485236 7001_ $$0G.Sironi.2$$aSironi, Giorgia$$b1
000485236 7001_ $$0E.Giro.1$$aGiro, Enrico$$b2
000485236 7001_ $$0S.Scuderi.5$$aScuderi, Salvatore$$b3
000485236 7001_ $$0R.Canestrari.1$$aCanestrari, Rodolfo$$b4
000485236 7001_ $$0S.Iovenitti.1$$aIovenitti, Simone$$b5
000485236 7001_ $$0P:(DE-H253)PIP1019066$$aGarczarczyk, Markus$$b6$$udesy
000485236 7001_ $$0P:(DE-H253)PIP1012636$$aKrause, Maria$$b7$$udesy
000485236 7001_ $$0S.Diebold.3$$aDiebold, Sebastian$$b8
000485236 7001_ $$0Rachele.Millul.1$$aMillul, Rachele$$b9
000485236 7001_ $$0O.F.Marioni.1$$aMarioni, Fabio$$b10
000485236 7001_ $$0N.Missaglia.1$$aMissaglia, Nadia$$b11
000485236 7001_ $$0M.Redaelli.1$$aRedaelli, Matteo$$b12
000485236 7001_ $$0G.Valsecchi.1$$aValsecchi, Giuseppe$$b13
000485236 7001_ $$0F.Zocchi.1$$aZocchi, Fabio$$b14
000485236 7001_ $$0A.Zanoni.2$$aZanoni, Adelfio$$b15
000485236 7001_ $$0G.Pareschi.1$$aPareschi, Giovanni$$b16
000485236 773__ $$0PERI:(DE-600)2799363-2$$a10.1117/1.JATIS.8.1.014005$$gVol. 11119, no. 1$$p014005$$tJournal of astronomical telescopes, instruments, and systems$$v8$$x2329-4124$$y2022
000485236 7870_ $$0PUBDB-2022-06822$$aLa Palombara, Nicola et.al.$$d2019$$iIsParent$$rarXiv:2201.08103$$tMirror production for the Cherenkov telescopes of the ASTRI mini-array and the MST project for the Cherenkov Telescope Array
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