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Featured researches published by F. Dazzi.


arXiv: Instrumentation and Methods for Astrophysics | 2016

INFN Camera demonstrator for the Cherenkov Telescope Array

G. Ambrosi; M. Ambrosio; C. Aramo; B. Bertucci; E. Bissaldi; M. Bitossi; S. Brasolin; G. Busetto; R. Carosi; S. Catalanotti; M. A. Ciocci; R. Consoletti; P. Da Vela; F. Dazzi; A. De Angelis; B. De Lotto; F. de Palma; R. Desiante; T. Di Girolamo; C. Di Giulio; M. Doro; D. D'Urso; G. Ferraro; F. Ferrarotto; F. Gargano; N. Giglietto; F. Giordano; G. Giraudo; M. Iacovacci; M. Ionica

The Cherenkov Telescope Array is a world-wide project for a new generation of ground-based Cherenkov telescopes of the Imaging class with the aim of exploring the highest energy region of the electromagnetic spectrum. With two planned arrays, one for each hemisphere, it will guarantee a good sky coverage in the energy range from a few tens of GeV to hundreds of TeV, with improved angular resolution and a sensitivity in the TeV energy region better by one order of magnitude than the currently operating arrays. In order to cover this wide energy range, three different telescope types are envisaged, with different mirror sizes and focal plane features. In particular, for the highest energies a possible design is a dual-mirror Schwarzschild-Couder optical scheme, with a compact focal plane. A silicon photomultiplier (SiPM) based camera is being proposed as a solution to match the dimensions of the pixel (angular size of ~ 0.17 degrees). INFN is developing a camera demonstrator made by 9 Photo Sensor Modules (PSMs, 64 pixels each, with total coverage 1/4 of the focal plane) equipped with FBK (Fondazione Bruno Kessler, Italy) Near UltraViolet High Fill factor SiPMs and Front-End Electronics (FEE) based on a Target 7 ASIC, a 16 channels fast sampler (up to 2GS/s) with deep buffer, self-trigger and on-demand digitization capabilities specifically developed for this purpose. The pixel dimensions of


Nuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment | 2008

The reflective surface of the MAGIC telescope

M. Doro; D. Bastieri; A. Biland; F. Dazzi; L. Font; M. Garczarczyk; M. Ghigo; E. Giro; F. Goebel; R. Kosyra; E. Lorenz; M. Mariotti; R. Mirzoyan; L. Peruzzo; Giovanni Pareschi; J. Zapatero

6\times6


arXiv: Astrophysics | 2007

The reflecting surface of the MAGIC-II Telescope

D. Bastieri; J. Arnold; C. Baixeras; O. Citterio; F. Dazzi; B. De Lotto; M. Doro; M. Ghigo; E. Giro; F. Goebel; R. Kosyra; E. Lorenz; M. Mariotti; R. Mirzoyan; R. Paoletti; Giovanni Pareschi; D. Pascoli; A. Pepato; L. Peruzzo; A. Saggion; P. Sartori; A. Sillanpää

mm


arXiv: High Energy Astrophysical Phenomena | 2009

MAGIC Collaboration: Contributions to the 31st International Cosmic Ray Conference (ICRC 2009)

H. Anderhub; L. A. Antonelli; P. Antoranz; M. Backes; C. Baixeras; S. Balestra; J. A. Barrio; D. Bastieri; J. Becerra González; J. Becker; W. Bednarek; K. Berger; E. Bernardini; A. Biland; R. Bock; G. Bonnoli; P. Bordas; D. Borla Tridon; V. Bosch-Ramon; D. Bose; I. Braun; T. Bretz; D. Britzger; M. Camara; E. Carmona; A. Carosi; P. Colin; S. Commichau; J. L. Contreras; J. Cortina

^2


Archive | 2004

Design studies for ECO, the European gamma-ray observatory

C. Baixeras; Denis Bastieri; C. Bigongiari; Mikko Pasanen; Daniel Ferenc; David Paneque; A. Sillanpää; Abelardo Moralejo; W. Wittek; Jose Antonio Coarasa Perez; M. Meucci; Jose Flix Molina; Carles Domingo; D. Dorner; Emma Ona-Wilhelmi; O. Blanch; D. Sobczynska; Ashot Chilingarian; N. Galante; Andreu Torres; K. Mannheim; Barbara De Lotto; Serguei Volkov; T. Hengstebeck; Luis Jose Contreras; Massimo Pin; E. Lorenz; Alessio Piccioli; Nadia Tonello; Paolo Sartori

lead to a very compact design with challenging problems of thermal dissipation. A modular structure, made by copper frames hosting one PSM and the corresponding FEE, has been conceived, with a water cooling system to keep the required working temperature. The actual design, the adopted technical solutions and the achieved results for this demonstrator are presented and discussed.


arXiv: High Energy Astrophysical Phenomena | 2018

The extreme HBL behaviour of Markarian 501 during 2012.

M. L. Ahnen; S. Ansoldi; L. A. Antonelli; C. Arcaro; A. Babic; B. Banerjee; P. Bangale; U. Barres de Almeida; J. A. Barrio; J. Becerra González; W. Bednarek; E. Bernardini; A. Berti; W. Bhattacharyya; O. Blanch; G. Bonnoli; R. Carosi; A. Carosi; Avishek Chatterjee; S. M. Colak; P. Colin; E. Colombo; Julio Contreras; J. Cortina; S. Covino; P. Cumani; P. Da Vela; F. Dazzi; A. De Angelis; B. De Lotto


Archive | 2014

Discovery of very high energy gamma-ray emission from the blazar 1ES 1727+502 with the MAGIC Telescopes (Research Note)

L. A. Antonelli; M. Asensio; M. Backes; U. Barres de Almeida; J. A. Barrio; J. Becerra González; K. Berger; E. Bernardini; A. Biland; A. Boller; S. Bonnefoy; G. Bonnoli; D. Borla Tridon; F. Borracci; D. Carreto Fidalgo; E. Colombo; Julio Contreras; J. Cortina; L. Cossio; F. Dazzi; B. De Lotto; C. Delgado Mendez; A. Domínguez; D. Dominis Prester; D. Dorner; D. Eisenacher; D. Elsaesser; D. Ferenc; M. V. Fonseca; L. Font

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C. Baixeras

Autonomous University of Barcelona

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J. A. Barrio

Complutense University of Madrid

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J. Becerra González

Spanish National Research Council

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E. Bernardini

Humboldt University of Berlin

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