CREAM flight data processing

H. S. Ahn; P. Allison; M. G. Bagliesi; J. J. Beatty; G. Bigongiari; P. Boyle; J. T. Childers; N. B. Conklin; S. Coutu; M. A. DuVernois; O. Ganel; J. H. Han; H. J. Hyun; J. A. Jeon; K. C. Kim; J. K. Lee; M. H. Lee; L. Lutz; P. Maestro; A. Malinine; P. S. Marrocchesi; S. Minnick; S. I. Mognet; S. W. Nam; S. Nutter; H. Park; I. H. Park; N. H. Park; E. S. Seo; R. Sina; S. Swordy; S. Wakely; J. Wu; J. Yang; Y. S. Yoon; R. Zei; S. Y. Zinn

CREAM flight data processing

H. S. Ahn
, P. Allison
, M. G. Bagliesi
, J. J. Beatty
, G. Bigongiari
, P. Boyle
, J. T. Childers
, N. B. Conklin
, S. Coutu
, M. A. DuVernois
, O. Ganel
, J. H. Han
, H. J. Hyun
, J. A. Jeon
, K. C. Kim
, J. K. Lee
, M. H. Lee
, L. Lutz
, P. Maestro
, A. Malinine

P. S. Marrocchesi, S. Minnick, S. I. Mognet, S. W. Nam, S. Nutter, H. Park, I. H. Park, N. H. Park, E. S. Seo, R. Sina, S. Swordy, S. Wakely, J. Wu, J. Yang, Y. S. Yoon, R. Zei, S. Y. Zinn

Research output: Contribution to conference › Paper › peer-review

Abstract

The Cosmic Ray Energetics And Mass (CREAM) instrument is a balloon-borne experiment designed to measure the composition and energy spectra of cosmic rays up to ̃ 10 ₁₅ eV. The instrument consists of, from top to bottom, an 8-paddle Timing Charge Detector (TCD), a 512-tube Transition Radiation Detector (TRD), a 2912-pixel Silicon Charge Detector (SCD), 2035 scintillating fibers in 3 hodoscopes interleaved with a pair of graphite targets, and a 20-layer tungsten/scintillating-fiber sampling calorimeter with 1000 fiber ribbons. We have developed the CREAM Data Processing System (CDPS), an object-oriented data processing program based on ROOT. In this paper we describe the data processing scheme used to handle flight data.

Original language	English (US)
Pages	389-392
Number of pages	4
State	Published - 2005
Event	29th International Cosmic Ray Conference, ICRC 2005 - Pune, India Duration: Aug 3 2005 → Aug 10 2005

Other

Other	29th International Cosmic Ray Conference, ICRC 2005
Country/Territory	India
City	Pune
Period	8/3/05 → 8/10/05

All Science Journal Classification (ASJC) codes

Nuclear and High Energy Physics

Cite this

Ahn, H. S., Allison, P., Bagliesi, M. G., Beatty, J. J., Bigongiari, G., Boyle, P., Childers, J. T., Conklin, N. B., Coutu, S., DuVernois, M. A., Ganel, O., Han, J. H., Hyun, H. J., Jeon, J. A., Kim, K. C., Lee, J. K., Lee, M. H., Lutz, L., Maestro, P., ... Zinn, S. Y. (2005). CREAM flight data processing. 389-392. Paper presented at 29th International Cosmic Ray Conference, ICRC 2005, Pune, India.

@conference{9279f6ca15b04b67ad0c08d957b37df6,

title = "CREAM flight data processing",

abstract = "The Cosmic Ray Energetics And Mass (CREAM) instrument is a balloon-borne experiment designed to measure the composition and energy spectra of cosmic rays up to{\~ } 10 15 eV. The instrument consists of, from top to bottom, an 8-paddle Timing Charge Detector (TCD), a 512-tube Transition Radiation Detector (TRD), a 2912-pixel Silicon Charge Detector (SCD), 2035 scintillating fibers in 3 hodoscopes interleaved with a pair of graphite targets, and a 20-layer tungsten/scintillating-fiber sampling calorimeter with 1000 fiber ribbons. We have developed the CREAM Data Processing System (CDPS), an object-oriented data processing program based on ROOT. In this paper we describe the data processing scheme used to handle flight data.",

author = "Ahn, \{H. S.\} and P. Allison and Bagliesi, \{M. G.\} and Beatty, \{J. J.\} and G. Bigongiari and P. Boyle and Childers, \{J. T.\} and Conklin, \{N. B.\} and S. Coutu and DuVernois, \{M. A.\} and O. Ganel and Han, \{J. H.\} and Hyun, \{H. J.\} and Jeon, \{J. A.\} and Kim, \{K. C.\} and Lee, \{J. K.\} and Lee, \{M. H.\} and L. Lutz and P. Maestro and A. Malinine and Marrocchesi, \{P. S.\} and S. Minnick and Mognet, \{S. I.\} and Nam, \{S. W.\} and S. Nutter and H. Park and Park, \{I. H.\} and Park, \{N. H.\} and Seo, \{E. S.\} and R. Sina and S. Swordy and S. Wakely and J. Wu and J. Yang and Yoon, \{Y. S.\} and R. Zei and Zinn, \{S. Y.\}",

year = "2005",

language = "English (US)",

pages = "389--392",

note = "29th International Cosmic Ray Conference, ICRC 2005 ; Conference date: 03-08-2005 Through 10-08-2005",

}

Ahn, HS, Allison, P, Bagliesi, MG, Beatty, JJ, Bigongiari, G, Boyle, P, Childers, JT, Conklin, NB, Coutu, S, DuVernois, MA, Ganel, O, Han, JH, Hyun, HJ, Jeon, JA, Kim, KC, Lee, JK, Lee, MH, Lutz, L, Maestro, P, Malinine, A, Marrocchesi, PS, Minnick, S, Mognet, SI, Nam, SW, Nutter, S, Park, H, Park, IH, Park, NH, Seo, ES, Sina, R, Swordy, S, Wakely, S, Wu, J, Yang, J, Yoon, YS, Zei, R & Zinn, SY 2005, 'CREAM flight data processing', Paper presented at 29th International Cosmic Ray Conference, ICRC 2005, Pune, India, 8/3/05 - 8/10/05 pp. 389-392.

TY - CONF

T1 - CREAM flight data processing

AU - Ahn, H. S.

AU - Allison, P.

AU - Bagliesi, M. G.

AU - Beatty, J. J.

AU - Bigongiari, G.

AU - Boyle, P.

AU - Childers, J. T.

AU - Conklin, N. B.

AU - Coutu, S.

AU - DuVernois, M. A.

AU - Ganel, O.

AU - Han, J. H.

AU - Hyun, H. J.

AU - Jeon, J. A.

AU - Kim, K. C.

AU - Lee, J. K.

AU - Lee, M. H.

AU - Lutz, L.

AU - Maestro, P.

AU - Malinine, A.

AU - Marrocchesi, P. S.

AU - Minnick, S.

AU - Mognet, S. I.

AU - Nam, S. W.

AU - Nutter, S.

AU - Park, H.

AU - Park, I. H.

AU - Park, N. H.

AU - Seo, E. S.

AU - Sina, R.

AU - Swordy, S.

AU - Wakely, S.

AU - Wu, J.

AU - Yang, J.

AU - Yoon, Y. S.

AU - Zei, R.

AU - Zinn, S. Y.

PY - 2005

Y1 - 2005

N2 - The Cosmic Ray Energetics And Mass (CREAM) instrument is a balloon-borne experiment designed to measure the composition and energy spectra of cosmic rays up to ̃ 10 15 eV. The instrument consists of, from top to bottom, an 8-paddle Timing Charge Detector (TCD), a 512-tube Transition Radiation Detector (TRD), a 2912-pixel Silicon Charge Detector (SCD), 2035 scintillating fibers in 3 hodoscopes interleaved with a pair of graphite targets, and a 20-layer tungsten/scintillating-fiber sampling calorimeter with 1000 fiber ribbons. We have developed the CREAM Data Processing System (CDPS), an object-oriented data processing program based on ROOT. In this paper we describe the data processing scheme used to handle flight data.

AB - The Cosmic Ray Energetics And Mass (CREAM) instrument is a balloon-borne experiment designed to measure the composition and energy spectra of cosmic rays up to ̃ 10 15 eV. The instrument consists of, from top to bottom, an 8-paddle Timing Charge Detector (TCD), a 512-tube Transition Radiation Detector (TRD), a 2912-pixel Silicon Charge Detector (SCD), 2035 scintillating fibers in 3 hodoscopes interleaved with a pair of graphite targets, and a 20-layer tungsten/scintillating-fiber sampling calorimeter with 1000 fiber ribbons. We have developed the CREAM Data Processing System (CDPS), an object-oriented data processing program based on ROOT. In this paper we describe the data processing scheme used to handle flight data.

UR - https://www.scopus.com/pages/publications/84899008324

UR - https://www.scopus.com/pages/publications/84899008324#tab=citedBy

M3 - Paper

AN - SCOPUS:84899008324

SP - 389

EP - 392

T2 - 29th International Cosmic Ray Conference, ICRC 2005

Y2 - 3 August 2005 through 10 August 2005

ER -

CREAM flight data processing

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All Science Journal Classification (ASJC) codes

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