Frontemare di Trieste
Istituto Nazionale di Fisica Nucleare
Sezione di Trieste



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  • W. Dabrowski et al., "Low noise monolithic bipolar front-end for Silicon Drift Detectors", to be published in NIM A.
  • S. Beolè et al., "Experimental study of a prototype silicon drift detector", submitted to NIM A.


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  • F. Arfelli et al., "Silicon detectors for synchrotron radiation digital mammography", NIM A360, 283 (1995).
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  • F. Arfelli et al., "Silicon detectors for digital radiography", NIM A367, 48 (1995).
  • C. Colledani et al., "CASTOR1.0: a VLSI analog-digital circuit for pixel imaging applications", Presented at the 3rd Workshop on "Semiconductor pixel detectors for Particle physics and X-ray detection", Bari, March 24-27,1996. LEPSI Note 96-04; submitted to NIM A.
  • F. Arfelli et al., "New developments in the field of silicon detectors for digital radiology", NIM A377, 508 (1996).
  • F. Arfelli et al., "A pixel-like matrix for digital mammography", Presented to the "9th International Workshop on Room
  • Temperature Semiconductor X and g ray Detectors Associated Electronics and Applications", Grenoble, France, September (1995). Accepted for pubblication in NIM.
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  • F. Arfelli et al., "The Digital Mammography Program at the SR Light Source in Trieste", Abstract presented at IEEE MIC 1996, Anaheim, California, 2-9 Nov 1996.


  • M. Bocciolini et al., "A silicon calorimeter for cosmic antimatter search", NIM A333 (1993) 560 and INFN AE 92-17.
  • M. Bocciolini et al., "A silicon imaging calorimeter prototype for antimatter search in space: experimental results", Nucl. Phys. B, Proc. Suppl. 32 (1993) 77 and INFN AE 92-24.
  • G. Barbiellini et al., "The GILDA mission: a new technique for a gamma-ray telescope in the energy range 20 MeV - 100 GeV", NIM A354 (1995) 547 and INFN AE 94-18.
  • F. Aversa et al., "Wizard si-w imaging calorimeter: a preliminary study on its particle identification capability during a balloon flight in 1993", NIM A360 (1995) 17.
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  • G. Barbiellini et al, "The cosmic-ray positron-to-electron ratio in the energy range 0.85 to 14 GeV", A&A 309, (1996) L15-L18 and INFN AE-96/02.
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  • Bocciolini et al., "The WiZard/CAPRICE Silicon-Tungsten Calorimeter", NIM A370 (1996) 403 and LNF-95/052.
  • G. Barbiellini et al., "Performance of the CAPRICE RICH detector during the 1994 balloon flight", NIM A371 (1996) 169.
  • F. Aversa et al., "Identification of cosmic ray electrons and positrons by neural networks", Astropart. Phys. 5 (1996) 111.
  • G. Barbiellini et al., "The cosmic-ray positron-to-electron ratio in the energy range 0.85 to 14 GeV", Astron. Astrophys. 309 (1996) L15 and INFN-AE-96-02.
  • R. Bellotti et al., "Cosmic ray antiproton/electron discrimination capability of the CAPRICE silicon-tungsten calorimeter using neural networks", accepted for publication by NIM A.
  • A. Morselli et al., "A fine grained silicon detector for high energy gamma-ray astrophysics", ROM2f/94/61, to be published in Il Nuovo Cimento B.



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