Abstract
We are conducting tests of optical and electronics components of JEMEUSO at the Telescope Array site in Utah with a ground-based “EUSO-TA” detector. The tests will include an engineering validation of the detector, cross-calibration of EUSO-TA with the TA fluorescence detector and observations of air shower events. Also, the proximity of the TA’s Electron Light Source will allow for convenient use of this calibration device. In this paper, we report initial results obtained with the EUSO-TA telescope.
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Pre-flight qualification tests of the Mini-EUSO telescope engineering model
Calibration aspects of the JEM-EUSO mission
Integration, qualification, and launch of the Mini-EUSO telescope on board the ISS
Notes
The actual number of frames requested for each threshold level has yet to be determined, but initial measurements show that the single photoelectron signal should be lower then 1 % of the maximal signal, requiring more then 10000 GTUs
To trigger on a rising slope, the initial signal must be below the threshold value. Therefore, for thresholds below the pedestal value the detection is performed when the signal fluctuates below the threshold value and then comes back to the baseline. Therefore lowering the threshold value in this range cuts the negative fluctuations causing a drop in number of detections
The total gain of a pixel corresponds to the distance between the pedestal peak and the single photoelectron peak.
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Acknowledgements
This work was partially supported by Basic Science Interdisciplinary Research Projects of RIKEN and JSPS KAKENHI Grant (22340063, 23340081, and 24244042), by the Inter-University Research Program of the Institute for Cosmic Ray Research, by the Italian Ministry of Foreign Affairs, General Direction for the Cultural Promotion and Cooperation and by the ’Helmholtz Alliance for Astroparticle Physics HAP’ funded by the Initiative and Networking Fund of the Helmholtz Association, Germany. LWP acknowledges support by JSPS.
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St. Kliment Ohridski University of Sofia, Sofia, Bulgaria
M. Bogomilov, M. Dupieux, Y. Karadzhov, D. Kolev, R. Matev, I. Rusinov, R. Tsenov & G. Vankova
LAL, Univ Paris-Sud, CNRS/IN2P3, Orsay, France
J. -N. Albert, P. Barrillon, S. Dagoret-Campagne, H. Miyamoto, D. Monnier-Ragaigne & C. Moretto
Omega, Ecole Polytechnique, CNRS/IN2P3, Palaiseau, France
S. Ahmad, S. Blin-Bondil, C. de la Taille & F. Dulucq
APC, Univ Paris Diderot, CNRS/IN2P3, CEA/Irfu, Obs. de Paris, Sorbonne Paris Cité, Paris, France
D. Allard, C. Blaksley, J. -N. Capdevielle, P. Gorodetzky, C. Lachaud, E. Parizot, T. Patzak, P. Prat, G. Prévôt, S. Selmane & D. Semikoz
IRAP, Université de Toulouse, CNRS, Toulouse, France
C. Catalano, M. Lacombe, B. Mot, G. Roudil & P. von Ballmoos
ECAP, University of Erlangen-Nuremberg, Erlangen, Germany
I. Kreykenbohm, M. Wille & J. Wilms
Karlsruhe Institute of Technology (KIT), Karlsruhe, Germany
P. L. Biermann, J. Blümer, A. Ebersoldt, R. Engel, S. Falk, A. Haungs, M. Karus, B. Keilhauer, M. Kleifges, T. Pierog, M. Roth, N. Sakaki, H. Schieler, M. Unger & M. Weber
Ludwig Maximilian University, Munich, Germany
T. Tajima
Institute for Astronomy and Astrophysics, Kepler Center, University of Tübingen, Tübingen, Germany
J. Bayer, G. Distratis, F. Fenu, A. Guzmán, T. Mernik, S. Piraino, A. Santangelo, T. Schanz, K. Shinozaki & C. Tenzer
Institut für Theoretische Physik und Astrophysik, University of Würzburg, Würzburg, Germany
K. Mannheim & O. Tibolla
Istituto Nazionale di Fisica Nucleare, Sezione di Bari, Bari, Italy
R. Bellotti, A. Bruno & F. Cafagna
Universita’ degli Studi di Bari Aldo Moro and INFN, Sezione di Bari, Bari, Italy
R. Bellotti & A. Monaco
Dipartimento di Fisica e Astronomia, Universita’ di Catania, Catania, Italy
R. Caruso & A. Insolia
Consiglio Nazionale delle Ricerche (CNR), Ist. di Fisica Applicata Nello Carrara, Firenze, Italy
G. Castellinic
Istituto Nazionale di Fisica Nucleare - Laboratori Nazionali di Frascati, Frascati, Italy
A. Franceschi, A. Marini, G. Modestino, T. Napolitano, M. Ricci & F. Ronga
Istituto Nazionale di Fisica Nucleare - Sezione di Napoli, Naples, Italy
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Dipartimento di Scienze Fisiche, Universita’ di Napoli Federico II, Naples, Italy
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INAF - Istituto di Astrofisica Spaziale e Fisica Cosmica di Palermo, Palermo, Italy
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Istituto Nazionale di Fisica Nucleare - Sezione di Roma Tor Vergata, Roma, Italy
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Dipartimento di Fisica, Universita’ di Roma Tor Vergata, Roma, Italy
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Istituto Nazionale di Fisica Nucleare - Sezione di Torino, Torino, Italy
M. Bertaina, C. Cassardo, A. Cellino, A. Dell’Oro, M. Di Martino, S. Ferrarese, P. Galeotti, G. Giraudo, P. Vallania & C. Vigorito
Dipartimento di Fisica, Università di Torino, INFN Torino, Torino, Italy
R. Bechini, M. Bertaina, C. Cassardo, R. Cremonini, S. Ferrarese, P. Galeotti & C. Vigorito
Istituto Nazionale di Astrofisica, Osservatorio Astrofisico di Torino, Torino, Italy
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Istituto Nazionale di Fisica Nucleare - Sezione di Catania, Catania, Italy
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Dipartimento di Ingegneria, UTIU, Rome, Italy
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DIETI, Universita’ degli Studi di Napoli Federico II, Napoli, Italy
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Chiba University, Chiba, Japan
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National Institute of Radiological Sciences, Chiba, Japan
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Fukui University of Technology, Fukui, Japan
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Kinki University, Higashi-Osaka, Japan
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Hiroshima University, Hiroshima, Japan
F. Tajima
Kanazawa University, Kanazawa, Japan
D. Yonetoku
Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Japan
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Kobe University, Kobe, Japan
M. Nagata
Konan University, Kobe, Japan
F. Kajino, M. Sakata, H. Sato, T. Yamamoto, Y. Yamamoto & K. Yoshida
Kyoto University, Kyoto, Japan
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Yukawa Institute, Kyoto University, Kyoto, Japan
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National Astronomical Observatory, Mitaka, Japan
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Nagoya University, Nagoya, Japan
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Solar-Terrestrial Environment Laboratory, Nagoya University, Nagoya, Japan
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Graduate School of Science, Osaka City University, Osaka, Japan
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Institute of Space and Astronautical Science/JAXA, Sagamihara, Japan
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Aoyama Gakuin University, Sagamihara, Japan
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Saitama University, Saitama, Japan
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Hokkaido University, Sapporo, Japan
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Interactive Research Center of Science, Tokyo Institute of Technology, Tokyo, Japan
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High Energy Accelerator Research Organization (KEK), Tsukuba, Japan
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Korea Astronomy and Space Science Institute (KASI), Daejeon, Republic of Korea
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Ewha Womans University, Seoul, Republic of Korea
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Sungkyunkwan University, Seoul, Republic of Korea
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Center for Galaxy Evolution Research, Yonsei University, Seoul, Republic of Korea
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Universidad Nacional Autónoma de México (UNAM), Mexico City, Mexico
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Benemérita Universidad Autónoma de Puebla (BUAP), Puebla, Mexico
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Institute of Physics, Jan Kochanowski University, Kielce, Poland
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Astronomical Observatory, Jagiellonian University, Krakow, Poland
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National Centre for Nuclear Research, Lodz, Poland
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Central Research Institute of Machine Building, TsNIIMash, Korolev, Russia
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Skobeltsyn Institute of Nuclear Physics, Lomonosov Moscow State University, Moscow, Russia
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Department of Space Physics, Institute of Experimental Physics, Kosice, Slovakia
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Consejo Superior de Investigaciones Científicas (CSIC), Madrid, Spain
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Instituto Nacional de Técnica Aeroespacial (INTA), Madrid, Spain
T. Belenguer, C. González Alvarado, M. D. Sabau & M. Sanz Palomino
Universidad de Alcalá (UAH), Madrid, Spain
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Universidad Carlos III de Madrid, Madrid, Spain
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ISDC Data Centre for Astrophysics, Versoix, Switzerland
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Institute for Atmospheric and Climate Science, ETH Zürich, Zürich, Switzerland
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Space Science Laboratory, University of California, Berkeley, USA
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Colorado School of Mines, Golden, USA
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Vanderbilt University, Nashville, USA
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RIKEN, 2-1 Hirosawa, Wako-shi, Japan
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Consortia
The JEM-EUSO Collaboration
Corresponding author
Correspondence to L. W. Piotrowski.
Additional information
Contribution to the special issue ‘JEM-EUSO’ of Experimental Astronomy
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The JEM-EUSO Collaboration., Adams, J.H., Ahmad, S. et al. Ground-based tests of JEM-EUSO components at the Telescope Array site, “EUSO-TA”. Exp Astron 40, 301–314 (2015). https://doi.org/10.1007/s10686-015-9441-6
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DOI: https://doi.org/10.1007/s10686-015-9441-6
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