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Dive into the research topics where F. Fratnik is active.

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Featured researches published by F. Fratnik.


The Astrophysical Journal | 1996

Measurement of the positron to electron ratio in the cosmic rays above 5-GeV

R. L. Golden; S.J. Stochaj; S. A. Stephens; F. Aversa; G. Barbiellini; M. Boezio; U. Bravar; A. Colavita; F. Fratnik; P. Schiavon; A. Vacchi; N. Zampa; J. W. Mitchell; J.F. Ormes; R. E. Streitmatter; R. Bellotti; F. Cafagna; M. Castellano; M. Circella; G. de Cataldo; C. De Marzo; N. Giglietto; B. Marangelli; A. Rain; P. Spinelli; M. Bocciolini; N. Finetti; P. Papini; A. Perego; S. Piccardi

As part of a series of experiments to search for antimatter in cosmic rays, the New Mexico State University balloon-borne magnet spectrometer was configured for a flight to study positrons. Two completely new instruments, a transition radiation detector and a silicon-tungsten imaging calorimeter, were added to the magnet spectrometer. These two detectors provided a proton rejection factor better than 3 × 104. This instrument was flown from Fort Sumner, New Mexico, at an average depth of 4.5 g cm-2 of residual atmosphere for a period of 25 hr. We report here the measured fraction of positrons e+/(e+ + e-) from ~5 to 60 GeV at the top of the atmosphere. Our measurements do not show any compelling evidence for an increase in this ratio with energy, and our results are consistent with a constant fraction of 0.078 ± 0.016 over the entire energy region.


Nuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment | 1996

The Wizard/CAPRICE silicon-tungsten calorimeter

M. Bocciolini; F. Celletti; N. Finetti; M. Grandi; P. Papini; A. Perego; S. Piccardi; P. Spillantini; V. Bidoli; M. Candusso; M. Casolino; M. P. De Pascale; A. Morselli; Piergiorgio Picozza; Roberta Sparvoli; G. Basini; G. Mazzenga; Mario V. Ricci; F. Bronzini; G. Barbiellini; M. Boezio; Ulisse Bravar; F. Fratnik; Paolo Schiavon; Andrea Vacchi; N. Zampa

A silicon-tungsten calorimeter has been developed to be flown in the Wizard/CAPRICE balloon borne experiment to measure the flux of antiprotons, positrons and light nuclei in the cosmic radiation. The calorimeter is composed of 8 .r. .v silicon sampling planes [active area (48 X 48) cm’] interleaved with 7 tungsten absorbers (7 radiation lengths): it provides the topology of the interacting events together with an independent measurement of the deposited energy. Details of the front-end electronics and of the read-out system are given and the overall performances during pre-flight ground operations are described as well.


Nuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment | 1995

WiZard SiW imaging calorimeter: a preliminary study on its particle identification capability during a balloon flight in 1993

F. Aversa; G. Barbiellini; M. Boezio; U. Bravar; A. Colavita; F. Fratnik; P. Schiavon; A. Vacchi; N. Zampa; V. Bidoli; M. Candusso; M. Casolino; M. P. De Pascale; A. Morselli; P. Picozza; Roberta Sparvoli; M. Bocciolini; F. Celletti; N. Finetti; M. Grandi; P. Papini; A. Perego; S. Piccardi; P. Spillantini; G. Basini; F.M. Brancaccio; G. Mazzenga; M. Ricci; R. Bellotti; F. Cafagna

Abstract The WiZard Collaboration is engaged in a program to study the antimatter components of the cosmic rays. A silicon-tungsten (WiW) imaging calorimeter has been developed as part of this program. We present its performance and preliminary results, obtained during a balloon flight on September 8, 1993. The flight was dedicated to the measurement of the positron spectrum in the energy range 4–50 GeV and took place from Ft. Sumner, New Mexico.


Astroparticle Physics | 1997

Study of the combined particle identification capability of a transition radiation detector and a silicon imaging calorimeter during the TS93 balloon flight

R. Bellotti; F. Cafagna; M. Castellano; M. Circella; G. de Cataldo; C. De Marzo; N. Giglietto; B. Marangelli; A. Rainò; P. Spinelli; M. Brancaccio; M. Grandi; P. Papini; A. Perego; S. Piccardi; P. Spillantini; G. Basini; M. Ricci; A. Codino; N. Finetti; C. Grimani; V. Bidoli; M. Candusso; M. Casolino; M. P. De Pascale; A. Morselli; P. Picozza; R. Sparvoli; F. Aversa; G. Barbiellini

Abstract The WiZard Collaboration is involved in a program studying the antimatter components of the cosmic rays. A transition radiation detector and a silicon-tungsten calorimeter with imaging capabilities have been built as part of this program. We present the combined performance of these two detectors for positron identification during a balloon flight on September 8, 1993. The flight was dedicated to the measurement of the positron spectrum in the energy range 4–50 GeV and was launched from Ft. Summer, New Mexico.


Astroparticle Physics | 1996

Identification of cosmic ray electrons and positrons by neural networks

F. Aversa; G. Barbiellini; G. Basini; R. Bellotti; V. Bidoli; M. Bocciolini; U. Bravar; M. Boezio; F. Cafagna; M. Candusso; M. Casolino; M. Castellano; M. Circella; A. Colavita; G. de Cataldo; C. De Marzo; M. P. De Pascale; N. Finetti; F. Fratnik; N. Giglietto; R. L. Golden; C. Grimani; M. Hof; B. Marangelli; F. Massimo Brancaccio; W. Menn; J. W. Mitchell; A. Morselli; P. Papini; A. Perego

Abstract A data analysis based on artificial neural network classifiers has been done to identify cosmic ray electrons and positrons detected with the balloon-borne NMSU/Wizard-TS93 experiment. The information is provided by two ancillary and independent particle detectors: a transition radiation detector and a silicon-tungsten imaging calorimeter. Electrons and positrons measured during the flight have been identified with background rejection factors of 80 ± 3 and 500 ± 37 at signal efficiencies of 72 ± 3% and 86 ± 2% for the transition radiation detector and silicon-tungsten imaging calorimeter, respectively. The ability of the artificial neural network classifiers to perform a careful multidimensional analysis surpasses the results achieved by conventional methods.


Nuclear Physics B - Proceedings Supplements | 1993

Silicon calorimeter for cosmic antimatter search

M. Bocciolini; F. Celletti; M. Grandi; A. Perego; P. Spillantini; G. Basini; F. Bongiorno; F. Massimo Brancaccio; M. Ricci; M.T. Brunetti; A. Codino; M. Menichelli; M. Miozza; I. Salvatori; V. Bidoli; M. Candusso; M. Casolino; C. De Fabritiis; M. P. De Pascale; A. Morselli; P. Picozza; A. Buccheri; A. Incicchitti; D. Prosperi; G. Barbiellini; M. Boezio; F. Fratnik; P. Schiavon; A. Vacchi; N. Zampa

Abstract The silicon sampling calorimeter presented is conceived as a fine grained imaging device to carry out studies of the anti-matter component in the primary cosmic radiation; it will be used in balloon payload program starting in 1993. The first sampling layer (48×48 cm2) of this silicon calorimeter has been completed and successfully tested. We report the first results form studies performed at the CERN PS t7 beam. The complete calorimeter contains 20 xy sampling layers (strip pitch 3.6 mm) interleaved with 19 showering material planes (tungsten 0.5 X0). This allows to picture the transverse distributions of the shower in both coordinates at each sampling. The outstanding imaging capabilities reflects in high particle identification power. Preliminary results from beam tests performed with antiprotons at 3.5 GeV on a tower prototype of the calorimeter are reported.


Nuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment | 2005

Status and characterisation of COMPASS RICH-1

E. Albrecht; Günter Baum; R. Birsa; F. Bradamante; A. Bressan; A. Chapiro; A. Cicuttin; P. Ciliberti; A. Colavita; S. Costa; M. Crespo; P. Cristaudo; S. Dalla Torre; C. D’Ambrosio; V. Diaz; V. Duic; P. Fauland; M. Finger; F. Fratnik; M. Giorgi; B. Gobbo; A. Martin; G. Menon; A. Mielech; P. Pagano; D. Piedigrossi; P. Schiavon; F. Sozzi; F. Tessarotto


Archive | 1995

Performance of the Transition Radiation Detector Flown on the NMSU/WIZARD TS93 Balloon-Borne Instrument

F. Aversa; G. Barbiellini; G. Basini; R. Bellotti; V. Bidoli; M. Bocciolini; M. Boezio; F. Massimo Brancaccio; U. Bravar; F. Bronzini; Maria Teresa Brunetti; A. F. Cafagna; M. Candusso; M. Casolino; Maria Gabriella Castellano; F. Celletti; M. Circella; A. Codino; Colavita; G. de Cataldo; C. De Marzo; M. P. De Pascale; N. Finetti; F. Fratnik; N. Giglietto; R. L. Golden; Mauro Grandi; C. Grimani; M. Hof; B. Marangelli


Archive | 1995

Observations of Cosmic Ray Positrons during the 1993 Flight of the NMSU/WiZard - TS93 Balloon-Borne Apparatus

F. Aversa; G. Barbiellini; G. Basini; R. Belloti; V. Bidoli; M. Bocciolini; M. Boezio; F. Massimo Brancaccio; U. Bravar; F. Bronzini; Maria Teresa Brunetti; F. Cafagna; M. Candusso; M. Casolino; Maria Gabriella Castellano; F. Celletti; M. Circella; A. Codino; Colavita; G. de Cataldo; C. De Marzo; M. P. De Pascale; N. Finetti; F. Fratnik; N. Giglietto; R. L. Golden; C. Grimani; M. Hof; B. Marangelli; G. Mazzenga


Archive | 1991

Silicon tracking calorimeter for antimatter search in space: First experimental results from a prototype

G. Barbiellini; M. Ricci; C. De Fabritiis; P. Spillantini; N. Zampa; M. Menichelli; F. Fratnik; A. Vacchi; M. Bocciolini; G. Basini; A. Morselli; M. P. De Pascale; F. Bongiorno; V. Bidoli; A. Incicchitti; F. Massimo-Brancaccio; P. Schiavon; L. Salvatori; A. Buccheri; A. Perego; P. Picozza; F. Celletti; M. Candusso; D. Prosperi

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M. P. De Pascale

Istituto Nazionale di Fisica Nucleare

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V. Bidoli

University of Rome Tor Vergata

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A. Perego

University of Florence

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M. Casolino

Sapienza University of Rome

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N. Finetti

University of Florence

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A. Morselli

University of Rome Tor Vergata

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F. Aversa

University of Trieste

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F. Celletti

University of Florence

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