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A statistical procedure for the identification of positrons in the PAMELA experiment (Articolo in rivista)
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- A statistical procedure for the identification of positrons in the PAMELA experiment (Articolo in rivista) (literal)
- Anno
- 2010-01-01T00:00:00+01:00 (literal)
- Alternative label
O. Adriani, G. C. Barbarino, G. A. Bazilevskaya, R. Bellotti, M. Boezio, E. A. Bogomolov, L. Bonechi, M. Bongi, V. Bonvicini, S. Borisov, S. Bottai, A. Bruno, F. Cafagna, D. Campana, R. Carbone, P. Carlson, M. Casolino, G. Castellini, et al. (2010)
A statistical procedure for the identification of positrons in the PAMELA experiment
in Astroparticle physics (Print)
(literal)
- Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#autori
- O. Adriani, G. C. Barbarino, G. A. Bazilevskaya, R. Bellotti, M. Boezio, E. A. Bogomolov, L. Bonechi, M. Bongi, V. Bonvicini, S. Borisov, S. Bottai, A. Bruno, F. Cafagna, D. Campana, R. Carbone, P. Carlson, M. Casolino, G. Castellini, et al. (literal)
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- 1. Univ Florence, Dept Phys, I-50019 Florence, Italy
2. INFN, Sez Firenze, I-50019 Florence, Italy
3. Univ Naples Federico 2, Dept Phys, I-80126 Naples, Italy
4. INFN, Sez Napoli, I-80126 Naples, Italy
5. PN Lebedev Phys Inst, RU-119991 Moscow, Russia
6. Univ Bari, Dept Phys, I-70126 Bari, Italy
7. INFN, Sez Bari, I-70126 Bari, Italy
8. INFN, Sez Trieste, I-34149 Trieste, Italy
9. AF Ioffe Phys Tech Inst, RU-194021 St Petersburg, Russia
10. INFN, Sez Roma Tor Vergata, I-00133 Rome, Italy
11. Univ Roma Tor Vergata, Dept Phys, I-00133 Rome, Italy
12. Moscow Engn & Phys Inst, RU-11540 Moscow, Russia
13. AlbaNova Univ Ctr, Oskar Klein Ctr Cosmoparticle Phys, SE-10691 Stockholm, Sweden
14. KTH, Dept Phys, SE-10691 Stockholm, Sweden
15. IFAC, I-50019 Florence, Italy
16. Univ Trieste, Dept Phys, I-34147 Trieste, Italy
17. Univ Siegen, Dept Phys, D-57068 Siegen, Germany
18. Ist Nazl Fis Nucl, Lab Nazl Frascati, I-00044 Frascati, Italy (literal)
- Titolo
- A statistical procedure for the identification of positrons in the PAMELA experiment (literal)
- Abstract
- The PAMELA satellite experiment has measured the cosmic-ray positron fraction between 1.5 GeV and 100 GeV. The need to reliably discriminate between the positron signal and proton background has required the development of an ad hoc analysis procedure. In this paper, a method for positron identification is described and its stability and capability to yield a correct background estimate is shown. The analysis includes new experimental data, the application of three different fitting techniques for the background sample and an estimate of systematic uncertainties due to possible inaccuracies in the background selection. The new experimental results confirm both solar modulation effects on cosmic-rays with low rigidities and an anomalous positron abundance above 10 GeV. (literal)
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