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Performance of the BACCUS Transition Radiation Detector
/ Picot-Clémente, Nicolas (Maryland U., College Park, IPST) ; Amare, Y (Maryland U., College Park, IPST) ; Anderson, T (Penn State U.) ; Angelaszek, D (Maryland U., College Park, IPST ; Maryland U.) ; Anthony, N (Maryland U.) ; Cheryian, K (Maryland U.) ; Choi, G H (Sungkyunkwan U.) ; Copley, M (Maryland U., College Park, IPST) ; Coutu, S (Penn State U.) ; Derome, Laurent (LPSC, Grenoble) et al.
The Boron And Carbon Cosmic rays in the Upper Stratosphere (BACCUS) balloon-borne exper-iment flew for 30 days over Antarctica in December 2016. It is the successor of the CREAMballoon program in Antarctica which recorded a total cumulative exposure of 161 days. [...]
SISSA, 2017 - 8 p.
- Published in : PoS ICRC2017 (2018) 246
Fulltext: PDF; External link: PoS server
In : 35th International Cosmic Ray Conference, Busan, Republique De Coree, 12 - 20 Jul 2017, pp.246
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Performance of the ISS-CREAM Calorimeter
/ Picot-Clémente, Nicolas (Maryland U., College Park, IPST) ; Amare, Y (Maryland U., College Park, IPST) ; Anderson, T (Penn State U.) ; Angelaszek, D (Maryland U., College Park, IPST ; Maryland U.) ; Anthony, N (Maryland U.) ; Cheryian, K (Maryland U.) ; Choi, G H (Sungkyunkwan U.) ; Copley, M (Maryland U., College Park, IPST) ; Coutu, S (Penn State U.) ; Derome, L (LPSC, Grenoble) et al.
The Cosmic Ray Energetics And Mass experiment for the International Space Station (ISS-CREAM) is scheduled for launch in 2017. It is designed to directly measure and identify theelemental composition of incident Galactic cosmic rays from a few hundred GeV to PeV energies.Such large energy range sensitivity is reached by using an electromagnetic sampling calorimeter(CAL) which measures the energy deposit of particle-induced showers. [...]
SISSA, 2017 - 6 p.
- Published in : PoS ICRC2017 (2018) 247
Fulltext: PDF; External link: PoS server
In : 35th International Cosmic Ray Conference, Busan, Republique De Coree, 12 - 20 Jul 2017, pp.247
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Charge resolution of the ISS-CREAM SCD measured with a heavy-ion beam
/ Hong, Gihan (Sungkyunkwan U.) ; Amare, Y (Maryland U., College Park, IPST) ; Anderson, T (Penn State U.) ; Angelaszek, D (Maryland U., College Park, IPST ; Maryland U.) ; Anthony, N (Maryland U., College Park, IPST) ; Cheryian, K (Maryland U., College Park, IPST) ; Choi, G H (Sungkyunkwan U.) ; Copley, M (Maryland U., College Park, IPST) ; Coutu, S (Penn State U.) ; Derome, L (LPSC, Grenoble) et al.
The Cosmic Ray Energetics And Mass experiment for the International Space Station (ISS-CREAM) is scheduled to be launched and installed on the ISS in August 2017, and will carry out a measurement of the energy and composition of energetic cosmic rays in space. The Silicon Charge Detector (SCD) will identify the charge of through-going cosmic rays. [...]
SISSA, 2017 - 8 p.
- Published in : PoS ICRC2017 (2018) 229
Fulltext: PDF; External link: PoS server
In : 35th International Cosmic Ray Conference, Busan, Republique De Coree, 12 - 20 Jul 2017, pp.229
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4.
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Penn State U. server - Full text
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Measurements of High-Energy Heavy Nuclei with the CREAM-I TRD
/ Wakely, Scott P (Chicago U.) ; Ahn, H S (Maryland U.) ; Allison, P S (Ohio State U.) ; Bagliesi, M G (U. Siena (main) ; INFN, Siena) ; Beatty, J J (Ohio State U.) ; Bigongiari, G (U. Siena (main) ; INFN, Siena) ; Boyle, P J (Chicago U., EFI) ; Brandt, T J (Ohio State U.) ; Childers, J T (Minnesota U.) ; Conklin, N B (Penn State U.) et al.
The balloon-borne cosmic-ray experiment CREAM-I (Cosmic-Ray Energetics And Mass) completed a successful 42-day flight during the 2004-2005 NASA\/NSF\/NSBF Antarctic expedition. CREAM-I combines an imaging calorimeter with charge detectors and a precision transition radiation detector (TRD). [...]
2007 - 4 p.
- Published in : : 2, pp. 187-190
Fulltext: PDF; External link: INDICO
In : 30th International Cosmic Ray Conference, Merida, Mexico, 3 - 11 Jul 2007, pp.187-190
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Precision Measurement of the Proton Flux in Primary Cosmic Rays from Rigidity 1 GV to 1.8 TV with the Alpha Magnetic Spectrometer on the International Space Station
/ Aguilar, M (Madrid, CIEMAT) ; Aisa, D (INFN, Perugia ; Perugia U.) ; Alpat, B (INFN, Perugia) ; Alvino, A (INFN, Perugia) ; Ambrosi, G (INFN, Perugia) ; Andeen, K (KIT, Karlsruhe, IKP) ; Arruda, L (LIP, Lisbon) ; Attig, N (IAS, Julich ; JARA, Aachen) ; Azzarello, P (INFN, Perugia ; Geneva U.) ; Bachlechner, A (RWTH Aachen U. ; JARA, Aachen) et al.
/AMS
A precise measurement of the proton flux in primary cosmic rays with rigidity (momentum/charge) from 1 GV to 1.8 TV is presented based on 300 million events. Knowledge of the rigidity dependence of the proton flux is important in understanding the origin, acceleration, and propagation of cosmic rays. [...]
2015 - 9 p.
- Published in : Phys. Rev. Lett. 114 (2015) 171103
APS Open Access article: PDF; Fulltext: PDF;
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Elemental Spectra from the CREAM-I Flight
/ Ahn, Hoseok ; Allison, P S ; Bagliesi, M G ; Beatty, J J ; Bigongiari, G ; Boyle, P J ; Childers, J T ; Conklin, N B ; Coutu, S ; Duvernois, M A et al.
The Cosmic Ray Energetics And Mass (CREAM) instrument is a balloon-borne experiment designed to measure the composition and energy spectra of cosmic rays of charge Z = 1 to 26 up to an energy of ∼1015 eV. CREAM had two successful flights on long-duration balloons (LDB) launched from McMurdo Station, Antarctica, in December 2004 and December 2005. [...]
2007 - 4 p.
- Published in : : 2, pp. 63-66
Fulltext: PDF; External link: INDICO
In : 30th International Cosmic Ray Conference, Merida, Mexico, 3 - 11 Jul 2007, pp.63-66
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Precision Measurement of the Boron to Carbon Flux Ratio in Cosmic Rays from 1.9 GV to 2.6 TV with the Alpha Magnetic Spectrometer on the International Space Station
/ Aguilar, M (Madrid, CIEMAT) ; Ali Cavasonza, L (JARA, Aachen) ; Alpat, B (INFN, Perugia) ; Ambrosi, G (INFN, Perugia) ; Arruda, L (LIP, Lisbon) ; Attig, N (Julich, NIC ; Unlisted, DE) ; Aupetit, S (LPSC, Grenoble) ; Azzarello, P (Geneva U.) ; Bachlechner, A (JARA, Aachen) ; Barao, F (LIP, Lisbon) et al.
/AMS
Knowledge of the rigidity dependence of the boron to carbon flux ratio (B/C) is important in understanding the propagation of cosmic rays. The precise measurement of the B/C ratio from 1.9 GV to 2.6 TV, based on 2.3 million boron and 8.3 million carbon nuclei collected by AMS during the first 5 years of operation, is presented. [...]
2016 - 8 p.
- Published in : Phys. Rev. Lett. 117 (2016) 231102
Fulltext: PDF;
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Report of the Topical Group on Cosmic Probes of Fundamental Physics for for Snowmass 2021
/ Adhikari, Rana X. (Caltech) ; Anchordoqui, Luis A. (Lehman Coll. ; City Coll., N.Y. ; Amer. Museum Natural Hist.) ; Fang, Ke (Wisconsin U., Madison) ; Sathyaprakash, B.S. (Penn State U., University Park, IGC ; Penn State U., Astron. Astrophys. ; Cardiff U.) ; Tollefson, Kirsten (Michigan State U.) ; Lewis, Tiffany R. (NASA, Goddard) ; Engel, Kristi (Maryland U. ; Los Alamos) ; Aboubrahim, Amin (U. Munster) ; Akarsu, Ozgur (Istanbul, Tech. U.) ; Akrami, Yashar (Case Western Reserve U.) et al.
Cosmic Probes of Fundamental Physics take two primary forms: Very high energy particles (cosmic rays, neutrinos, and gamma rays) and gravitational waves. [...]
arXiv:2209.11726.
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