The structure of the zebra telescope, the integration tests and the first calibration results

G. Villa; A. Bussini; F. Perotti; R. Santambrogio; A. Rampini; G. Di Cocco; R. C. Butler; E. Caroli; J. B. Stephen; A. Traci; A. Donati; P. Ubertini; C. La Padula; M. Mastropietro; R. Patriarca; A. J. Dean; A. J. Court; F. A. Younis; P. Maggioli; M. Yearworth; G. Graham

doi:10.1109/TNS.1987.4337295

The structure of the zebra telescope, the integration tests and the first calibration results

G. Villa, A. Bussini, F. Perotti, R. Santambrogio, A. Rampini, G. Di Cocco, R. C. Butler, E. Caroli, J. B. Stephen, A. Traci, A. Donati, P. Ubertini, C. La Padula, M. Mastropietro, R. Patriarca, A. J. Dean, A. J. Court, F. A. Younis, P. Maggioli, M. YearworthG. Graham

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Abstract

The ZEBRA telescope is a balloon borne low energy gamma ray instrument, sensitive in the photon energy range 0.2-10MeV. The main characteristics and components of the telescope are described, and its performance during laboratory calibration is discussed, after its integration with the flight electronics.

Original language	English
Pages (from-to)	25-30
Number of pages	6
Journal	IEEE Transactions on Nuclear Science
Volume	34
Issue number	1
DOIs	https://doi.org/10.1109/TNS.1987.4337295
Publication status	Published - Feb 1987

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Villa, G., Bussini, A., Perotti, F., Santambrogio, R., Rampini, A., Di Cocco, G., Butler, R. C., Caroli, E., Stephen, J. B., Traci, A., Donati, A., Ubertini, P., La Padula, C., Mastropietro, M., Patriarca, R., Dean, A. J., Court, A. J., Younis, F. A., Maggioli, P., ... Graham, G. (1987). The structure of the zebra telescope, the integration tests and the first calibration results. IEEE Transactions on Nuclear Science, 34(1), 25-30. https://doi.org/10.1109/TNS.1987.4337295

@article{b7515e99029642b19e06c2c11cf2f67d,

title = "The structure of the zebra telescope, the integration tests and the first calibration results",

abstract = "The ZEBRA telescope is a balloon borne low energy gamma ray instrument, sensitive in the photon energy range 0.2-10MeV. The main characteristics and components of the telescope are described, and its performance during laboratory calibration is discussed, after its integration with the flight electronics.",

author = "G. Villa and A. Bussini and F. Perotti and R. Santambrogio and A. Rampini and {Di Cocco}, G. and Butler, {R. C.} and E. Caroli and Stephen, {J. B.} and A. Traci and A. Donati and P. Ubertini and {La Padula}, C. and M. Mastropietro and R. Patriarca and Dean, {A. J.} and Court, {A. J.} and Younis, {F. A.} and P. Maggioli and M. Yearworth and G. Graham",

year = "1987",

month = feb,

doi = "10.1109/TNS.1987.4337295",

language = "English",

volume = "34",

pages = "25--30",

journal = "IEEE Transactions on Nuclear Science",

issn = "0018-9499",

publisher = "Institute of Electrical and Electronics Engineers (IEEE)",

number = "1",

}

Villa, G, Bussini, A, Perotti, F, Santambrogio, R, Rampini, A, Di Cocco, G, Butler, RC, Caroli, E, Stephen, JB, Traci, A, Donati, A, Ubertini, P, La Padula, C, Mastropietro, M, Patriarca, R, Dean, AJ, Court, AJ, Younis, FA, Maggioli, P, Yearworth, M & Graham, G 1987, 'The structure of the zebra telescope, the integration tests and the first calibration results', IEEE Transactions on Nuclear Science, vol. 34, no. 1, pp. 25-30. https://doi.org/10.1109/TNS.1987.4337295

TY - JOUR

T1 - The structure of the zebra telescope, the integration tests and the first calibration results

AU - Villa, G.

AU - Bussini, A.

AU - Perotti, F.

AU - Santambrogio, R.

AU - Rampini, A.

AU - Di Cocco, G.

AU - Butler, R. C.

AU - Caroli, E.

AU - Stephen, J. B.

AU - Traci, A.

AU - Donati, A.

AU - Ubertini, P.

AU - La Padula, C.

AU - Mastropietro, M.

AU - Patriarca, R.

AU - Dean, A. J.

AU - Court, A. J.

AU - Younis, F. A.

AU - Maggioli, P.

AU - Yearworth, M.

AU - Graham, G.

PY - 1987/2

Y1 - 1987/2

N2 - The ZEBRA telescope is a balloon borne low energy gamma ray instrument, sensitive in the photon energy range 0.2-10MeV. The main characteristics and components of the telescope are described, and its performance during laboratory calibration is discussed, after its integration with the flight electronics.

AB - The ZEBRA telescope is a balloon borne low energy gamma ray instrument, sensitive in the photon energy range 0.2-10MeV. The main characteristics and components of the telescope are described, and its performance during laboratory calibration is discussed, after its integration with the flight electronics.

UR - http://www.scopus.com/inward/record.url?scp=84939044163&partnerID=8YFLogxK

U2 - 10.1109/TNS.1987.4337295

DO - 10.1109/TNS.1987.4337295

M3 - Article (Academic Journal)

AN - SCOPUS:84939044163

SN - 0018-9499

VL - 34

SP - 25

EP - 30

JO - IEEE Transactions on Nuclear Science

JF - IEEE Transactions on Nuclear Science

IS - 1

ER -

The structure of the zebra telescope, the integration tests and the first calibration results

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