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Status of the NectarCAM camera project

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dc.book.titleHigh energy, optical, and infrared detectors for astronomy VI
dc.contributor.authorBarrio Uña, Juan Abel
dc.contributor.authorHerranz, D.
dc.contributor.authorTejedor, L. A.
dc.date.accessioned2023-06-19T15:54:46Z
dc.date.available2023-06-19T15:54:46Z
dc.date.issued2014
dc.description© 2014 SPIE. Artículo firmado por 64 autores and the CTA consortium. We gratefully acknowledge support from the agencies and organizations listed in this page http://www.cta- observatory.org/?q=node/22. We gratefully acknowledge financial support from the following agencies and organizations: Ministerio de Ciencia, Tecnología e Innovación Productiva (MinCyT), Comisión Nacional de Energía Atómica (CNEA), Consejo Nacional de Investigaciones Científicas y Técnicas (CONICET), Argentina; State Committee of Science of Armenia, Armenia; Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq), Fundação de Amparo à Pesquisa do Estado do Rio de Janeiro (FAPERJ), Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP), Brasil; Croatian Science Foundation, Croatia; Ministry of Education, Youth and Sports, MEYS LE13012, 7AMB12AR013, Czech Republic; Ministry of Higher Education and Research, CNRS-INSU and CNRS-IN2P3, CEA-Irfu, ANR, Regional Council Ile de France, Labex ENIGMASS, OSUG2020 and OCEVU, France; Max Planck Society, BMBF, DESY, Helmholtz Association, Germany; Department of Atomic Energy, Department of Science and Technology, India; Istituto Nazionale di Astrofisica (INAF), MIUR, Italy; ICRR, University of Tokyo, JSPS, Japan; Netherlands Research School for Astronomy (NOVA), Netherlands Organization for Scientific Research (NWO), Netherlands; The Bergen Research Foundation, Norway; Ministry of Science and Higher Education, the National Centre for Research and Development and the National Science Centre, Poland; MINECO support through the National R+D+I, CDTI funding plans and the CPAN and MultiDark Consolider-Ingenio 2010 programme, Spain; Swedish Research Council, Royal Swedish Academy of Sciences, Sweden; Swiss National Science Foundation (SNSF), Ernest Boninchi Foundation, Switzerland; Durham University, Leverhulme Trust, Liverpool University, University of Leicester, University of Oxford, Royal Society, Science and Technologies Facilities Council, UK; U.S. National Science Foundation, U.S. Department of Energy, Argonne National Laboratory, Barnard College, University of California, University of Chicago, Columbia University, Georgia Institute of Technology, Institute for Nuclear and Particle Astrophysics (INPAC-MRPI program), Iowa State University, Washington University McDonnell Center for the Space Sciences, USA. We have received funding from the European Union’s Seventh Framework Programme ([FP7/2007-2013] [FP7/2007-2011]) under Grant Agreement 262053. Conference on High Energy, Optical, and Infrared Detectors for Astronomy(6. 2014. Montreal, Canada).
dc.description.abstractNectarCAM is a camera designed for the medium-sized telescopes of the Cherenkov Telescope Array (CTA) covering the central energy range 100 GeV to 30 TeV. It has a modular design based on the NECTAr chip, at the heart of which is a GHz sampling Switched Capacitor Array and 12-bit Analog to Digital converter. The camera will be equipped with 265 7-photomultiplier modules, covering a field of view of 7 to 8 degrees. Each module includes the photomultiplier bases, High Voltage supply, pre-amplifier, trigger, readout and Thernet transceiver. Events recorded last between a few nanoseconds and tens of nanoseconds. A flexible trigger scheme allows to read out very long events. NectarCAM can sustain a data rate of 10 kHz. The camera concept, the design and tests of the various subcomponents and results of thermal and electrical prototypes are presented. The design includes the mechanical structure, the cooling of electronics, read-out, clock distribution, slow control, data-acquisition, trigger, monitoring and services. A 133-pixel prototype with full scale mechanics, cooling, data acquisition and slow control will be built at the end of 2014.
dc.description.departmentDepto. de Estructura de la Materia, Física Térmica y Electrónica
dc.description.facultyFac. de Ciencias Físicas
dc.description.refereedTRUE
dc.description.sponsorshipUnión Europea. FP7
dc.description.sponsorshipCroatian Science Foundation, Croatia
dc.description.sponsorshipMinistry of Education, Youth and Sports, Czech Republic
dc.description.sponsorshipMinistry of Higher Education and Research
dc.description.sponsorshipCNRS-INSU
dc.description.sponsorshipCNRS-IN2P3
dc.description.sponsorshipCEA-Irfu
dc.description.sponsorshipANR
dc.description.sponsorshipRegional Council Ile de France
dc.description.sponsorshipLabex ENIGMASS, France
dc.description.sponsorshipLabex OSUG2020, France
dc.description.sponsorshipLabex OCEVU, France
dc.description.sponsorshipMax Planck Society, Germany
dc.description.sponsorshipBMBF, Germany
dc.description.sponsorshipDESY, Germany
dc.description.sponsorshipHelmholtz Association, Germany
dc.description.sponsorshipIstituto Nazionale di Astrofisica (INAF)
dc.description.sponsorshipMIUR, Italy
dc.description.sponsorshipNetherlands Research School for Astronomy (NOVA)
dc.description.sponsorshipNetherlands Organization for Scientific Research (NWO)
dc.description.sponsorshipMinistry of Science and Higher Education
dc.description.sponsorshipThe National Centre for Research and Development, Poland
dc.description.sponsorshipThe National Science Centre, Poland
dc.description.sponsorshipMINECO, Spain
dc.description.sponsorshipCDTI, Spain
dc.description.sponsorshipCPAN, Spain
dc.description.sponsorshipMultiDark Consolider-Ingenio 2010 programme, Spain
dc.description.sponsorshipSwedish Research Council
dc.description.sponsorshipRoyal Swedish Academy of Sciences
dc.description.sponsorshipDurham University
dc.description.sponsorshipLeverhulme Trust
dc.description.sponsorshipLiverpool University
dc.description.sponsorshipUniversity of Leicester
dc.description.sponsorshipUniversity of Oxford
dc.description.sponsorshipRoyal Society, Science and Technologies Facilities Council
dc.description.statuspub
dc.eprint.idhttps://eprints.ucm.es/id/eprint/31310
dc.identifier.doi10.1117/12.2056277
dc.identifier.isbn978-0-8194-9622-5
dc.identifier.officialurlhttp:/dx.doi.org/10.1117/12.2056277
dc.identifier.relatedurlhttp://proceedings.spiedigitallibrary.org/
dc.identifier.urihttps://hdl.handle.net/20.500.14352/35758
dc.issue.number9154
dc.language.isoeng
dc.publisherSPIE-Int Soc Optical Engineering
dc.relation.ispartofseriesProceedings of SPIE
dc.relation.projectIDCTA-PP (262053)
dc.relation.projectIDMEYS LE13012
dc.relation.projectID7AMB12AR013
dc.relation.projectIDFP7/2007-2013
dc.relation.projectIDFP7/2007-2011
dc.rights.accessRightsopen access
dc.subject.cdu539.1
dc.subject.keywordGamma-ray astronomy
dc.subject.keywordCamera for Cherenkov telescopes
dc.subject.keywordNectarCAM
dc.subject.keywordCTA
dc.subject.ucmFísica nuclear
dc.subject.unesco2207 Física Atómica y Nuclear
dc.titleStatus of the NectarCAM camera project
dc.typebook part
dcterms.references[1] Acharya, B. S., Actis, M., Aghajani, T., Agnetta, G., Aguilar, J., Aharonian, F., Ajello, M., Akhperjanian, A., Alcubierre, M., Aleksić, J., and et al., “Introducing the CTA concept," Astroparticle Physics 43, 3-18 (Mar. 2013). [2] Bolmont, J., Corona, P., Gauron, P., Ghislain, P., Gon, C., Guevara Riveros, L., Huppert, J.-F., Martineau-Huynh, O., Nayman, P., Parraud, J.-M., Tavernet, J.-P., Toussenel, F., Vincent, D., Vincent, P., Bertoli, W., Espigat, P., Punch, M., Besin, D., Delagnes, E., Glicenstein, J.-F., Moudden, Y., Venault, P., Zaghia, H., Brunetti, L., Dubois, J., Fiasson, A., Geroy, N., Gomes Monteiro, I., Journet, L., Krayzel, F., Lamanna, G., Le Flour, T., Lees, S., Lieunard, B., Maurin, G., Mugnier, P., Panazol, J., Prast, J., Chounet, L.-M., Edy, E., Fontaine, G., Giebels, B., Hormigos, S., Khélifi, B., Manigot, P., Maritaz, P., de Naurois, M., Compin, M., Feinstein, F., Fernandez, D., Mehault, J., Rivoire, S., Royer, S., Sanguillon, M., and Vasileiadis, G., “The camera of the fth H.E.S.S. telescope. Part I: System description," ArXiv e-prints (Oct. 2013). [3] Barcelo, M., Barrio, J. A., Blanch Bigas, O., Boix, J., Delgado, C., Herranz, D., Lopez-Coto, R., Martinez, G., and CTA Consortium, L. A. T. f. t., “An Analog Trigger System for Atmospheric Cherenkov Telescopes," ArXiv e-prints (July 2013). [4] Naumann, C. L., Tejedor, L. A., and Martínez, G., “COLIBRI: partial camera readout and sliding trigger for the Cherenkov Telescope Array CTA," Journal of Instrumentation 8, 6011P (June 2013). [5] Sanuy, A., Gascon, D., Paredes, J. M., Garrido, L., Ribó, M., and Sieiro, J., “Wideband (500 MHz) 16 bit dynamic range current mode PreAmplier for the CTA cameras (PACTA)," Journal of Instrumentation 7, C1100 (Jan. 2012). [6] Sanuy, A., Delagnes, E., Gascon, D., Sieiro, X., Bolmont, J., Corona, P., Feinstein, F., Glicenstein, J.-F., Naumann, C. L., Nayman, P., Ribó, M., Tavernet, J.-P., Toussenel, F., Vincent, P., and Vorobiov, S.,”Wideband pulse ampliers for the NECTAr chip," Nuclear Instruments and Methods in Physics Research A 695, 385{389 (Dec. 2012). [7] Delagnes, E., Bolmont, J., Corona, P., Dzahini, D., Feinstein, F., Gascon, D., Glicenstein, J. F., Guilloux, F., Naumann, C. L., Nayman, P., Rarbi, F., Sanuy, A., Tavernet, J., Toussenel, F., Vincent, P., and Vorobiov, S., “Nectar0, a new high speed digitizer asic for the cherenkov telescope array," in [Nuclear Science Symposium and Medical Imaging Conference (NSS/MIC), 2011 IEEE], 1457-1462 (Oct 2011). [8] Naumann, C. L., Delagnes, E., Bolmont, J., Corona, P., Dzahini, D., Feinstein, F., Gascón, D., Glicenstein, J.-F., Guilloux, F., Nayman, P., Rarbi, F., Sanuy, A., Tavernet, J.-P., Toussenel, F., Vincent, P., and Vorobiov, S., “New electronics for the Cherenkov Telescope Array (NECTAr)," Nuclear Instruments and Methods in Physics Research A 695, 44-51 (Dec. 2012). [9] Homann, D. and Houles, J., “Prototyping a 10 Gigabit-Ethernet Event-Builder for the CTA Camera Server,"Journal of Physics Conference Series 396, 012024 (Dec. 2012).
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