M. Conte
Alenia Aeronautica
3 Papers
2.1K Citations
M. Conte is an academic researcher from Alenia Aeronautica. The author has contributed to research in topics: Photon & Context (language use). The author has an hindex of 3, co-authored 3 publications.
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Papers
The European Photon Imaging Camera on XMM-Newton: The MOS cameras
Martin J. L. Turner,A. F. Abbey,M. Arnaud,M. Balasini,Marco Barbera,Elena Belsole,P. J. Bennie,J. P. Bernard,Giovanni F. Bignami,M. Boer,Ulrich G. Briel,I. Butler,C. Cara,C. Chabaud,Richard E. Cole,Alfonso Collura,M. Conte,A. Cros,M. Denby,P. Dhez,G. Di Coco,J. Dowson,P. Ferrando,Simona Ghizzardi,Fulvio Gianotti,C. V. Goodall,L. Gretton,R. G. Griffiths,O. Hainaut,Jean-François Hochedez,Andrew D. Holland,E. Jourdain,E. Kendziorra,A. Lagostina,R. Lainé,N. La Palombara,M. Lortholary,David H. Lumb,P. Marty,S. Molendi,C. Pigot,E. Poindron,Ken Pounds,James Reeves,Claus Reppin,R. Rothenflug,P. Salvetat,J. L. Sauvageot,D. Schmitt,Steve Sembay,A.D. Short,J. Spragg,J. Stephen,Lothar Strüder,Andrea Tiengo,M. Trifoglio,Joachim Trümper,S. Vercellone,L. Vigroux,Gabriele E. Villa,Martin Ward,S. Whitehead,E. Zonca +62 more
TL;DR: The EPIC focal plane imaging spectrometers on XMM-Newton use CCDs to record the images and spectra of celestial X-ray sources focused by the three Xray mirrors as discussed by the authors.
The AGILE Mission
Marco Tavani,Guido Barbiellini,A. Argan,F. Boffelli,Andrea Bulgarelli,P. A. Caraveo,P. W. Cattaneo,A. W. Chen,V. Cocco,Enrico Costa,Filippo D'Ammando,E. Del Monte,G. De Paris,G. Di Cocco,G. Di Persio,I. Donnarumma,Y. Evangelista,Marco Feroci,Arnaud Ferrari,M. Fiorini,F. Fornari,F. Fuschino,T. Froysland,Massimo Frutti,M. Galli,Fulvio Gianotti,A. Giuliani,Claudio Labanti,I. Lapshov,Francesco Lazzarotto,F. Liello,Paolo Lipari,Francesco Longo,E. Mattaini,Martino Marisaldi,M. Mastropietro,A. Mauri,F. Mauri,Sandro Mereghetti,Ennio Morelli,A. Morselli,Luigi Pacciani,A. Pellizzoni,F. Perotti,G. Piano,P. Picozza,C. Pontoni,Geiland Porrovecchio,M. Prest,G. Pucella,Massimo Rapisarda,A. Rappoldi,E. Rossi,Alda Rubini,Paolo Soffitta,Alessandro Traci,M. Trifoglio,Alessio Trois,E. Vallazza,S. Vercellone,V. Vittorini,A. Zambra,D. Zanello,C. Pittori,B. Preger,P. Santolamazza,F. Verrecchia,P. Giommi,S. Colafrancesco,Angelo Antonelli,S. Cutini,Dario Gasparrini,S. Stellato,G. Fanari,R. Primavera,F. Tamburelli,F. Viola,G. Guarrera,L. Salotti,F. D'Amico,E. Marchetti,M. Crisconio,Paolo Sabatini,G. Annoni,S. Alia,Antonio Francesco Longoni,R. Sanquerin,M. Battilana,P. Concari,E. Dessimone,R. Grossi,A. Parise,F. Monzani,E. Artina,R. Pavesi,G. Marseguerra,L. Nicolini,L. Scandelli,L. Soli,V. Vettorello,E. Zardetto,A. Bonati,L. Maltecca,E. D'Alba,M. Patané,G. Babini,F. Onorati,L. Acquaroli,M. Angelucci,B. Morelli,C. Agostara,M. Cerone,A. Michetti,P. Tempesta,S. D'Eramo,F. Rocca,Franco Giannini,G. Borghi,B. Garavelli,M. Conte,M. Balasini,Ivan Ferrario,M. Vanotti,E. Collavo,M. Giacomazzo +124 more
TL;DR: AGILE as mentioned in this paper is an Italian Space Agency mission dedicated to observing the gamma-ray universe, which was successfully launched on 2007 April 23 from the Indian base of Sriharikota and was inserted in an equatorial orbit with very low particle background.
The EPIC system onboard the ESA XMM mission
G. Villa,A. F. Abbey,Monique Arnaud,M. Balasini,Giovanni F. Bignami,M. Boer,Heinrich Bräuninger,I. Butler,G. Cafagna,C. Cara,C. Chabaud,L. Chiappetti,Richard E. Cole,M. Conte,J. Dowson,P. Dhez,R. Duc,G. Di Cocco,Philippe Ferrando,C. V. Goodall,H. Hippmann,Andrew D. Holland,Eckhard Kendziorra,Alain Labeque,Norbert Meidinger,C. Moriggio,N. La Palombara,C. Musso,E. Poindron,Giovanni Peres,Elmar Pfeffermann,C. Pigot,John P. Pye,Claus Reppin,D. Schmitt,S. Sciortino,Salvatore Serio,J. E. Spragg,J. B. Stephen,Lothar Strüder,M. Trifoglio,P. Tua,Martin J. L. Turner,S. Whitehead +43 more
- 01 Jan 1996
TL;DR: The European Photon Imaging Camera (EPIC) is one of the two main instruments onboard the ESA X-Ray Cornerstone mission XMM as discussed by the authors, which is devoted to performing imaging and spectroscopy of the X-ray sky in the domain 0.1-10 keV with a peak sensitivity in i0 seconds of 2x10'5 erg/cm2.
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