• DocumentCode
    1009643
  • Title

    Newly developed low background hard X-ray/gamma-ray telescope with the well-type phoswich counters

  • Author

    Takahashi, Tatsuro ; Gunji, S. ; Hirayama, Motoko ; Kamae, Tune ; Miyazaki, S. ; Sekimoto, Yutaro ; Tamura, Takuya ; Tanaka, Mitsuru ; Yamasaki, N.Y. ; Yamagami, T. ; Nomachi, M. ; Murakami, H.

  • Author_Institution
    Dept. of Phys., Tokyo Univ., Japan
  • Volume
    40
  • Issue
    4
  • fYear
    1993
  • fDate
    8/1/1993 12:00:00 AM
  • Firstpage
    890
  • Lastpage
    898
  • Abstract
    A low background hard X-ray/gamma-ray telescope (Welcome-1) for balloon-borne experiments in the energy range from 40 keV to 800-1000 keV is discussed. The detector is based on newly developed well-type phoswich counters. In the first well-type phoswich counter, GSO(Ce) (Gd 2SiO5 doped with Ce) is used as the detection part and CsI(Tl) as the shielding part. Welcome-1 consists of 64 GSO/CsI well-type phoswich counters assembled in the compound-eye configuration, and the effective area is 740 cm2 at 122 keV and 222 cm2 at 511 keV line. The well-type phoswich counter and the compound eye configuration reduce background significantly both externally and internally, and allow a high signal-to-noise ratio in balloon-borne experiments. The background levels at an attitude of 4.5 g/cm2 are 1×10-4/cm2/s/keV at 122 keV. Crab nebula is observed with the signal to background ratio better than unity between 100 and 200 keV. The design of the telescope and the flight performance are presented
  • Keywords
    X-ray astronomy; astronomical telescopes; gamma-ray detection and measurement; scintillation counters; 40 to 1000 keV; Crab nebula; CsI(Tl); CsI:Tl; Gd2SiO5:Ce; Welcome-1; balloon-borne experiments; compound-eye configuration; effective area; flight performance; hard X-ray/gamma-ray telescope; high signal-to-noise ratio; low background; shielding part; well-type phoswich counters; Assembly; Counting circuits; Energy resolution; Network address translation; Physics; Satellites; Signal to noise ratio; Telescopes; X-ray detection; X-ray detectors;
  • fLanguage
    English
  • Journal_Title
    Nuclear Science, IEEE Transactions on
  • Publisher
    ieee
  • ISSN
    0018-9499
  • Type

    jour

  • DOI
    10.1109/23.256679
  • Filename
    256679