Zobrazeno 1 - 10
of 41
pro vyhledávání: '"Argan, A."'
Autor:
M. D’Andrea, K. Ravensberg, A. Argan, D. Brienza, S. Lotti, C. Macculi, G. Minervini, L. Piro, G. Torrioli, F. Chiarello, L. Ferrari Barusso, M. Biasotti, G. Gallucci, F. Gatti, M. Rigano, H. Akamatsu, J. Dercksen, L. Gottardi, F. de Groote, R. den Hartog, J.-W. den Herder, R. Hoogeveen, B. Jackson, A. McCalden, S. Rosman, E. Taralli, D. Vaccaro, M. de Wit, J. Chervenak, S. Smith, N. Wakeham
Publikováno v:
Journal of Low Temperature Physics. 209:433-440
The X-IFU is the cryogenic spectrometer onboard the future ATHENA X-ray observatory. It is based on a large array of TES microcalorimeters, which works in combination with a Cryogenic AntiCoincidence detector (CryoAC). This is necessary to reduce the
Autor:
Andrzej A. Zdziarski, Andrei M. Bykov, Irfan Kuvvetli, G. Kanbach, Dieter H. Hartmann, A. Argan, Silvia Zane, Andrea Bulgarelli, Andreas Zoglauer, Julie McEnery, Kazuhiro Nakazawa, Peter von Ballmoos, Søren Brandt, Alessandro De Angelis, M. N. Mazziotta, Vincent Tatischeff, Marco Tavani, M. Hernanz, Elisa Costantini, Uwe Oberlack, Javier Rico, Lorraine Hanlon, Philippe Laurent, Isabelle Grenier, Rui Curado da Silva, R. Walter, A. Morselli, Mark Pearce, Xin Wu
Publikováno v:
Exper.Astron.
Exper.Astron., 2021, 51 (3), pp.1225-1254. ⟨10.1007/s10686-021-09706-y⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
De Angelis, A, Tatischeff, V, Argan, A, Brandt, S, Bulgarelli, A, Bykov, A, Costantini, E, Silva, R C D, Grenier, I A, Hanlon, L, Hartmann, D, Hernanz, M, Kanbach, G, Kuvvetli, I, Laurent, P, Mazziotta, M N, McEnery, J, Morselli, A, Nakazawa, K, Oberlack, U, Pearce, M, Rico, J, Tavani, M, Ballmoos, P V, Walter, R, Wu, X, Zane, S, Zdziarski, A & Zoglauer, A 2021, ' Gamma-ray astrophysics in the MeV range : The ASTROGAM concept and beyond ', Experimental Astronomy, vol. 51, pp. 1225–1254 . https://doi.org/10.1007/s10686-021-09706-y
Exper.Astron., 2021, 51 (3), pp.1225-1254. ⟨10.1007/s10686-021-09706-y⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
De Angelis, A, Tatischeff, V, Argan, A, Brandt, S, Bulgarelli, A, Bykov, A, Costantini, E, Silva, R C D, Grenier, I A, Hanlon, L, Hartmann, D, Hernanz, M, Kanbach, G, Kuvvetli, I, Laurent, P, Mazziotta, M N, McEnery, J, Morselli, A, Nakazawa, K, Oberlack, U, Pearce, M, Rico, J, Tavani, M, Ballmoos, P V, Walter, R, Wu, X, Zane, S, Zdziarski, A & Zoglauer, A 2021, ' Gamma-ray astrophysics in the MeV range : The ASTROGAM concept and beyond ', Experimental Astronomy, vol. 51, pp. 1225–1254 . https://doi.org/10.1007/s10686-021-09706-y
Angelis, A. de, et al.
The energy range between about 100 keV and 1 GeV is of interest for a vast class of astrophysical topics. In particular, (1) it is the missing ingredient for understanding extreme processes in the multi-messenger era; (2)
The energy range between about 100 keV and 1 GeV is of interest for a vast class of astrophysical topics. In particular, (1) it is the missing ingredient for understanding extreme processes in the multi-messenger era; (2)
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e8f812057d32d59399cf673e5ef95be2
https://hal.archives-ouvertes.fr/hal-03150563
https://hal.archives-ouvertes.fr/hal-03150563
Autor:
A. Argan, Francesco Lucarelli, Lina Quintieri, Andrea Bulgarelli, V. Cocco, M. Trifoglio, P. W. Cattaneo, L. Foggetta, M. Prest, A. Pellizzoni, A. Giuliani, F. Boffelli, N. Parmigiani, Valentina Fioretti, A. Zambra, F. D'Ammando, A. Morselli, M. Pilia, S. Sabatini, P. Valente, A. Rappoldi, C. Pittori, T. Froysland, M. Tavani, A. W. Chen, S. Vercellone, F. Longo, Bruno Buonomo, A. Trois, G. Pucella, M. Galli, F. Verrecchia, M. Cardillo, G. Mazzitelli, E. Vallazza, G. Barbiellini, S. Colafrancesco, Arnaud Ferrari, G. Piano, F. Fuschino, F. Gianotti, F. Paoletti, I. Donnarumma, Martino Marisaldi
AGILE is a mission of the Italian Space Agency (ASI) Scientific Program dedicated to gamma-ray astrophysics, operating in a low Earth orbit since April 23, 2007. It is designed to be a very light and compact instrument, capable of simultaneously dete
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2bf3cc7f264e04f8a0273c1a107ec068
http://hdl.handle.net/11368/2941062
http://hdl.handle.net/11368/2941062
Autor:
Bert-Joost van Leeuwen, M. P. Bruijn, Jan van der Kuur, James A. Chervenak, P. Peille, Jan-Willem den Herder, Brian Jackson, Mikko Kiviranta, Luigi Piro, Johannes Dercksen, Claudio Macculi, Dennis van Loon, Marco Barbera, Hiroki Akamatsu, Didier Barret, Roland H. den Hartog, Caroline A. Kilbourne, Henk van Weers, Flavio Gatti, Luciano Gottardi, Ruud W. M. Hoogeveen, Jean-Michel Mesnager, Francoise Douchin, Stephen J. Smith, Simon R. Bandler, A. Argan, Hervé Geoffray
Publikováno v:
Space Telescopes and Instrumentation 2018: Ultraviolet to Gamma Ray.
The X-ray Integral Field Unit (X-IFU) is an imaging microcalorimeter being developed for ESA's Athena X-ray observatory to providing high spectral resolution imaging between 0.2-12 keV, with moderate count-rate capability and a large field-of-view. T
Autor:
L. Piro, Flavio Gatti, M. P. Bruijn, A. Argan, Luciano Gottardi, B. J. van Leeuwen, Mikko Kiviranta, Jay Chervenak, Claudio Macculi, H. van Weers, Hiroki Akamatsu, Didier Barret, Caroline A. Kilbourne, Samuel Smith, Marco Barbera, Thien Lam-Trong, Simon R. Bandler, R. den Hartog, J. W. den Herder, D. Haas, Johannes Dercksen, J. van der Kuur, Brian Jackson
Publikováno v:
B. D. Jackson, B D, van Weers, H, van der Kuur, J, den Hartog, R, Akamatsu, H, Argan, A, Bandler, S R, Barbera, M, Barret, D, Bruijn, M P, Chervenak, J A, Dercksen, J, Gatti, F, Gottardi, L, Haas, D, den Herder, J-W, Kilbourne, C A, Kiviranta, M, Lam-Trong, T, van Leeuwen, B-J, Macculi, C, Piro, L & Smith, S J 2016, The focal plane assembly for the Athena X-ray Integral Field Unit instrument . in Space Telescopes and Instrumentation 2016 : Ultraviolet to Gamma Ray ., 990521, International Society for Optics and Photonics SPIE, Proceedings of SPIE, vol. 9905, SPIE Astronomical Telescopes and Instrumentation, Edinburgh, United Kingdom, 26/06/16 . https://doi.org/10.1117/12.2232544
This paper summarizes a preliminary design concept for the focal plane assembly of the X-ray Integral Field Unit on the Athena spacecraft, an imaging microcalorimeter that will enable high spectral resolution imaging and point-source spectroscopy. Th
Publikováno v:
Experimental Astronomy
ATHENA is a large X-ray observatory, planned to be launched by ESA in 2028 towards an L2 orbit. One of the two instruments of the payload is the X-IFU: a cryogenic spectrometer based on a large array of TES microcalorimeters, able to perform integral
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::09758e5d25ebc8c2494fdd4737e811d9
http://hdl.handle.net/11567/896238
http://hdl.handle.net/11567/896238
Autor:
Michele Biasotti, M. D'Andrea, Simone Lotti, Guido Torrioli, Claudio Macculi, A. Argan, Flavio Gatti, D. Corsini, Luigi Piro
Publikováno v:
SPIE Astronomical Telescopes + Instrumentation, 2016, Edinburgh, United Kingdom, 26 June-01 July 2016
info:cnr-pdr/source/autori:D'Andrea M.; Argan A.; Lotti S.; Macculi C.; Piro L.; Biasotti M.; Corsini D.; Gatti F.; Torrioli G./congresso_nome:SPIE Astronomical Telescopes + Instrumentation, 2016, Edinburgh, United Kingdom/congresso_luogo:/congresso_data:26 June-01 July 2016/anno:2016/pagina_da:/pagina_a:/intervallo_pagine
info:cnr-pdr/source/autori:D'Andrea M.; Argan A.; Lotti S.; Macculi C.; Piro L.; Biasotti M.; Corsini D.; Gatti F.; Torrioli G./congresso_nome:SPIE Astronomical Telescopes + Instrumentation, 2016, Edinburgh, United Kingdom/congresso_luogo:/congresso_data:26 June-01 July 2016/anno:2016/pagina_da:/pagina_a:/intervallo_pagine
The ATHENA observatory is the second large-class mission in ESA Cosmic Vision 2015-2025, with a launch foreseen in 2028 towards the L2 orbit. The mission addresses the science theme "The Hot and Energetic Universe", by coupling a high-performance X-r
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a377d512ce70accdd1953c70ad8136ff
http://hdl.handle.net/11567/897562
http://hdl.handle.net/11567/897562
Autor:
A. Argan, Andrea Bulgarelli, E. Moretti, Geiland Porrovecchio, Martino Marisaldi, A. W. Chen, P. Picozza, A. Zambra, F. D'Ammando, Bruno Buonomo, P. Santolamazza, G. Barbiellini, S. Vercellone, Alessio Trois, M. Fiorini, I. Donnarumma, M. Galli, Y. Evangelista, E. Vallazza, Marco Feroci, Fulvio Gianotti, Arnaud Ferrari, Luigi Pacciani, F. Longo, G. De Paris, F. Verrecchia, F. Perotti, G. Piano, S. Sabatini, F. Boffelli, Ennio Morelli, Alda Rubini, P. W. Cattaneo, P. Caraveo, V. Cocco, L. Foggetta, Claudio Labanti, Francesco Lazzarotto, Marco Tavani, A. Pellizzoni, E. Costa, M. Prest, D. Zanello, L. Salotti, A. Morselli, M. Pilia, Paolo Soffitta, Paolo Valente, Sandro Mereghetti, G. Di Cocco, A. Rappoldi, A. Giuliani, M. Mastropietro, S. Colafrancesco, V. Vittorini, Massimo Rapisarda, G. Pucella, Lina Quintieri, C. Pittori, T. Froysland, E. Striani, F. Fuschino, I. Lapshov, Paolo Lipari, P. Giommi, E. Del Monte, G. Mazzitelli, M. Trifoglio
Publikováno v:
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment. 674:55-66
At the core of the AGILE scientific instrument, designed to operate on a satellite, there is the Gamma Ray Imaging Detector (GRID) consisting of a Silicon Tracker (ST), a Cesium Iodide Mini-Calorimeter and an Anti-Coincidence system of plastic scinti
Autor:
Martino Marisaldi, A. Argan, Marco Tavani, Marco Feroci, Francesco Lazzarotto, Luigi Pacciani, Andrea Bulgarelli, E. Del Monte, F. Fuschino, I. Donnarumma, M. Trifoglio, M. Galli, Claudio Labanti, Fulvio Gianotti, Alessio Trois
Publikováno v:
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment. 588:17-21
AGILE, the small scientific mission of the Italian Space Agency devoted to Hard-X and Gamma-ray astrophysics, was successfully launched on April 23, 2007. The AGILE payload is composed of a tungsten-silicon tracker (ST), operating in the gamma-ray en
Autor:
Claudio Macculi, L Piro, F Gatti, S Lotti, A Argan, M Laurenza, M D'Andrea, G Torrioli, M Biasotti, D Corsini, A Orlando, T Mineo, A D'Ai, S Molendi, F Gastaldello, A Bulgarelli, V Fioretti, C Jacquey, P Laurent
Publikováno v:
EXPLORING THE HOT AND ENERGETIC UNIVERSE: THE FIRST SCIENTIFIC CONFERENCE DEDICATED TO THE ATHENA X-RAY OBSERVATORY, 8-10 september 2015
info:cnr-pdr/source/autori:Claudio Macculi, L Piro, F Gatti, S Lotti, A Argan, M Laurenza, M D'Andrea, G Torrioli, M Biasotti, D Corsini, A Orlando, T Mineo, A D'Ai, S Molendi, F Gastaldello, A Bulgarelli, V Fioretti, C Jacquey, P Laurent/congresso_nome:EXPLORING THE HOT AND ENERGETIC UNIVERSE: THE FIRST SCIENTIFIC CONFERENCE DEDICATED TO THE ATHENA X-RAY OBSERVATORY/congresso_luogo:/congresso_data:8-10 september 2015/anno:2015/pagina_da:/pagina_a:/intervallo_pagine
info:cnr-pdr/source/autori:Claudio Macculi, L Piro, F Gatti, S Lotti, A Argan, M Laurenza, M D'Andrea, G Torrioli, M Biasotti, D Corsini, A Orlando, T Mineo, A D'Ai, S Molendi, F Gastaldello, A Bulgarelli, V Fioretti, C Jacquey, P Laurent/congresso_nome:EXPLORING THE HOT AND ENERGETIC UNIVERSE: THE FIRST SCIENTIFIC CONFERENCE DEDICATED TO THE ATHENA X-RAY OBSERVATORY/congresso_luogo:/congresso_data:8-10 september 2015/anno:2015/pagina_da:/pagina_a:/intervallo_pagine
We present the particle background reduction techniques aimed to increase the X-IFU sensitivity, which is reduced by primary protons of both solar and Cosmic Rays origin, and secondary electrons. The adopted solutions involve Monte Carlo simulation b
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=cnr_________::c89657bf8c63f7710b221aa485a9c0c4
https://publications.cnr.it/doc/413985
https://publications.cnr.it/doc/413985