Enrico Virgilli
University of Ferrara
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Featured researches published by Enrico Virgilli.
Proceedings of SPIE | 2013
Enrico Virgilli; Filippo Frontera; V. Valsan; V. Liccardo; V. Carassiti; S. Squerzanti; M. Statera; M. Parise; S. Chiozzi; F. Evangelisti; E. Caroli; J. B. Stephen; N. Auricchio; S. Silvestri; A. Basili; F. Cassese; L. Recanatesi; V. Guidi; V. Bellucci; R. Camattari; Claudio Ferrari; Andrea Zappettini; Elisa Buffagni; Elisa Bonnini; M. Pecora; S. Mottini; B. Negri
We will describe the LAUE project, supported by the Italian Space Agency, whose aim is to demonstrate the capability to build a focusing optics in the hard X-/soft gamma-ray domain (80{600 keV). To show the lens feasibility, the assembling of a Laue lens petal prototype with 20 m focal length is ongoing. Indeed, a feasibility study, within the LAUE project, has demonstrated that a Laue lens made of petals is feasible. Our goal is a lens in the 80-600 keV energy band. In addition to a detailed description of the new LARIX facility, in which the lens is being assembled, we will report the results of the project obtained so far.
Proceedings of SPIE | 2011
Enrico Virgilli; F. Frontera; V. Valsan; V. Liccardo; V. Carassiti; F. Evangelisti; S. Squerzanti
We present the results obtained with the new Laue lens prototype built in the LARIX facility in the Physics Department of University of Ferrara. Following the results of the first prototype presented at the SPIE conference in Marseille, and also thanks to the methods adopted for improving the prototype (SPIE conference in San Diego, Ferrari et al. 2009) here we present the results of the new prototype with improved performances in terms of point spread function (PSF) and spectral response.
Proceedings of SPIE | 2011
Enrico Virgilli; Filippo Frontera; V. Valsan; V. Liccardo; E. Caroli; J. B. Stephen; F. Cassese; L. Recanatesi; M. Pecora; S. Mottini; Primo Attinà; B. Negri
We present the LAUE project devoted to develop an advanced technology for building a high focal length Laue lens for soft gamma-ray astronomy (80-600 keV). The final goal is to develop a focusing optics that can improve the current sensitivity in the above energy band by 2 orders of magnitude.
Proceedings of SPIE | 2012
F. Frontera; Enrico Virgilli; V. Liccardo; V. Valsan; V. Carassiti; S. Chiozzi; F. Evangelisti; S. Squerzanti; M. Statera; V. Guidi; C. Ferrari; R. A. Zappettini; E. Caroli; N. Auricchio; S. Silvestri; R. Camattari; F. Cassese; L. Recanatesi; M. Pecora; S. Mottini; B. Negri
We present the status of LAUE, a project supported by the Italian Space Agency (ASI), and devoted to develop Laue lenses with long focal length (from 10–15 meters up to 100 meters), for hard X–/soft gamma–ray astronomy (80-600 keV). Thanks to their focusing capability, the design goal is to improve the sensitivity of the current instrumention in the above energy band by 2 orders of magnitude, down to a few times 10−8 photons/(cm2 s keV).
Proceedings of SPIE | 2013
Filippo Frontera; Enrico Virgilli; V. Valsan; V. Liccardo; V. Carassiti; E. Caroli; F. Cassese; C. Ferrari; V. Guidi; S. Mottini; M. Pecora; B. Negri; L. Recanatesi; L. Amati; N. Auricchio; L. Bassani; R. Campana; R. Farinelli; C. Guidorzi; Claudio Labanti; R. Landi; A. Malizia; M. Orlandini; P. Rosati; V. Sguera; J. B. Stephen; Lev Titarchuk
This paper summarizes the development of a successful project, LAUE, supported by the Italian Space Agency (ASI) and devoted to the development of long foca length (up to 100—m) Laue lenses for hard X–/soft gamma– ray astronomy (80-600 keV). The apparatus is ready and the assembling of a prototype lens petal is ongoing. The great achievement of this project is the use of bent crystals. From measurements obtained on single crystals and from simulations, we have estimated the expected Point Spread Function and thus the sensitivity of a lens made of petals. The expected sensitivity is a few ×10−8 photons cm−2 s−1 keV−1). We discuss a number of open astrophysical questions that can settled with such an instrument aboard a free-flying satellite.
Proceedings of SPIE | 2012
V. Liccardo; Enrico Virgilli; F. Frontera; V. Valsan
In the context of the LAUE project devoted to build a long focal-length focusing optics for soft γ–ray astronomy (80 – 600 keV), we present the results of reflectivity measurements of bent crystals in different configurations, obtained by bending perfect or mosaic flat crystals. We also compare these results with those obtained using flat crystals. The measurements were performed using the Kα line of the Tungsten anode of the X–ray tube in the LARIX facility at the University of Ferrara. These results are finalized to select the best materials and to optimize the thickness of the crystal tiles that will be used for building a Laue lens petal which is a part of an entire Laue lens, with 20 m focal length and 100–300 keV passband. The final goal of the LAUE project is to overcome, by at least 2 orders of magnitude, the sensitivity limits of the current generation of γ–ray telescopes, and to improve the current γ–ray imaging capability.
Proceedings of SPIE | 2013
V. Liccardo; Enrico Virgilli; Filippo Frontera; V. Valsan; V. Guidi; Elisa Buffagni
For the first time, with the Laue project, bent crystals are being used for focusing photons in the 80-300 keV energy range. The advantage is their high reflectivity and better Point Spread Function with respect to the mosaic at crystals. Simulations have already shown their excellent focusing capability which makes them the best candidates for a Laue lens whose sensitivity is also driven by the size of the focused spot. Selected crystals are Germanium (perfect, (111)) and Gallium Arsenide (mosaic, (220)) with 40 m curvature radius to get a spherical lens with 20 m long focal length. A lens petal is being built. We report the measurement technique by which we are able to estimate the exact curvature of each tile within a few percent of uncertainty and their diffraction efficiency. We also discuss some results.
Proceedings of SPIE | 2012
V. Valsan; Filippo Frontera; Enrico Virgilli; V. Liccardo
In the context of the LAUE project devoted to build a long focal length focusing optics for soft gamma-ray astronomy (70/100 keV to <>600 keV), we present results of simulation of a Laue lens, based on bent crystals in different assembling configurations (quasi-mosaic and reflection-like geometries). The main aim is to significantly overcome the sensitivity limits of the current generation of gamma-ray telescopes and improve the imaging capability.
Proceedings of SPIE | 2009
F. Ferrari; Filippo Frontera; G. Loffredo; Enrico Virgilli; C. Guidorzi; V. Carassiti; F. Evangelisti; L. Landi; S. Chiozzi; S. Squerzanti; E. Caroli; J. B. Stephen; F. Schiavone; A. Basili; K. Andersen; P. Courtois
We report on new results on the development activity of broad band Laue lenses for hard X-/gamma-ray astronomy (70/100-600 keV). After the development of a first prototype, whose performance was presented at the SPIE conference on Astronomical Telescopes held last year in Marseille (Frontera et al. 2008), we have improved the lens assembling technology. We present the the development status of the new lens prototype that is on the way to be assembled.
Journal of Astronomical Telescopes, Instruments, and Systems | 2017
Enrico Virgilli; Valsan; Filippo Frontera; E. Caroli; V. Liccardo; John B. Stephen
Abstract. In the context of the Laue project devoted to build a Laue lens prototype for focusing celestial hard x-/soft gamma-rays, a Laue lens made of bent crystal tiles, with 20-m focal length, is simulated. The focusing energy passband is assumed to be 90 to 600 keV. The distortion of the image produced by the lens on the focal plane, due to effects of crystal tile misalignment and radial distortion of the crystal curvature, is investigated. The corresponding effective area of the lens, its point spread function, and sensitivity are calculated and compared with those exhibited by a nominal Laue lens with no misalignment and/or distortion. Such analysis is crucial to estimate the optical properties of a real lens, in which the investigated shortcomings could be present.