Precise measurement of the absolute yield of fluorescence photons in atmospheric gases

被引：6

作者：

Ave, M. ^{[2
]}

Bohacova, M. ^{[1
,3
,5
]}

Daumiller, K. ^{[2
]}

Di Carlo, P. ^{[4
,6
]}

Di Giulio, C. ^{[7
,8
]}

San Luis, Pedro Facal ^{[1
,5
]}

Gonzales, D. ^{[9
]}

Hojvat, C. ^{[10
]}

Horandel, J. R. ^{[11
]}

Hrabovsky, M. ^{[12
]}

Iarlori, M. ^{[4
,6
]}

Keilhauer, B. ^{[2
]}

Klages, H. ^{[2
]}

Kleifges, M. ^{[13
]}

Kuehn, F. ^{[10
]}

Monasor, M. ^{[1
,5
]}

Nozka, L. ^{[3
]}

Palatka, M. ^{[3
]}

Petrera, S. ^{[4
,6
]}

Privitera, P. ^{[1
,5
]}

Ridky, J. ^{[3
]}

Rizi, V. ^{[4
,6
]}

d'Orfeuil, B. Rouille ^{[1
,5
]}

Salamida, F. ^{[2
]}

Schovanek, P. ^{[3
]}

Smida, R. ^{[2
]}

Spinka, H. ^{[14
]}

Ulrich, A. ^{[15
]}

Verzi, V. ^{[7
,8
]}

Williams, C. ^{[1
]}

机构：

[1] Univ Chicago, Enrico Fermi Inst, Chicago, IL 60637 USA

[2] Karlsruhe Inst Technol, IK, D-76021 Karlsruhe, Germany

[3] Acad Sci Czech Republic, Inst Phys, CZ-18221 Prague 8, Czech Republic

[4] Univ Aquila, Dipartimento Fis, I-67010 Coppito, Aquila, Italy

[5] Univ Chicago, Kavli Inst Cosmol Phys, Chicago, IL 60637 USA

[6] Ist Nazl Fis Nucl, I-67010 Coppito, Aquila, Italy

[7] Univ Roma Tor Vergata, Dipartimento Fis, I-00133 Rome, Italy

[8] Sezione Ist Nazl Fis Nucl, I-00133 Rome, Italy

[9] Karlsruhe Inst Technol, IEKP, D-76021 Karlsruhe, Germany

[10] Fermilab Natl Accelerator Lab, Batavia, IL 60510 USA

[11] Radboud Univ Nijmegen, IMAPP, NL-6500 GL Nijmegen, Netherlands

[12] Palacky Univ, RCATM, Olomuc, Czech Republic

[13] Karlsruhe Inst Technol, IPE, D-76021 Karlsruhe, Germany

[14] Argonne Natl Lab, Argonne, IL 60439 USA

[15] Tech Univ Munich, Phys Dept E12, D-85748 Garching, Germany

来源：

NUCLEAR PHYSICS B-PROCEEDINGS SUPPLEMENTS | 2011年 / 212-13卷

关键词：

DEPENDENCE; DETECTOR;

D O I：

10.1016/j.nuclphysbps.2011.03.048

中图分类号：

O412 [相对论、场论]; O572.2 [粒子物理学];

学科分类号：

摘要：

We have performed a measurement of the absolute yield of fluorescence photons at the Fermi lab Test Beam. A systematic uncertainty at 5% level was achieved by the use of Cherenkov radiation as a reference calibration light source. A cross-check was performed by an independent calibration using a laser light source. A significant improvement on the energy scale uncertainty of Ultra-High Energy Cosmic Rays is expected.

引用

页码：356 / 361

页数：6

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