TSUBAME: toward the Frontier of X-ray/Gamma-ray Polarimetry in Astronomy

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  • TOIZUMI Takahiro
    Department of Physics, Faculty of Science, Tokyo Institute of Technology
  • KATAOKA Jun
    Department of Physics, Faculty of Science, Tokyo Institute of Technology
  • TSUBUKU Yoshihiro
    Department of Physics, Faculty of Science, Tokyo Institute of Technology
  • KOBAYASHI Mitsuyoshi
    Department of Physics, Faculty of Science, Tokyo Institute of Technology
  • YATSU Yoichi
    Department of Physics, Faculty of Science, Tokyo Institute of Technology
  • ARIMOTO Makoto
    Department of Physics, Faculty of Science, Tokyo Institute of Technology
  • SHIMOKAWABE Takashi
    Department of Physics, Faculty of Science, Tokyo Institute of Technology
  • KAWAI Nobuyuki
    Department of Physics, Faculty of Science, Tokyo Institute of Technology
  • OMAGARI Kuniyuki
    Department of Mechanical and Aerospace Engineering,, Tokyo Institute of Technology
  • FUJIWARA Ken
    Department of Mechanical and Aerospace Engineering,, Tokyo Institute of Technology
  • ASHIDA Hiroki
    Department of Mechanical and Aerospace Engineering,, Tokyo Institute of Technology
  • NISHIDA Junichi
    Department of Mechanical and Aerospace Engineering,, Tokyo Institute of Technology
  • FUJIHASHI Kota
    Department of Mechanical and Aerospace Engineering,, Tokyo Institute of Technology
  • INAGAWA Shinich
    Department of Mechanical and Aerospace Engineering,, Tokyo Institute of Technology
  • MIURA Yoshiyuki
    Department of Mechanical and Aerospace Engineering,, Tokyo Institute of Technology
  • MATSUNAGA Saburo
    Department of Mechanical and Aerospace Engineering,, Tokyo Institute of Technology

抄録

“TSUBAME” is a university-built small satellite mission to measure polarization of hard X-ray photons (30-200 keV) from gamma-ray bursts (GRBs) using azimuthal anisotropy of Compton-scattered photons. Polarimetry in the hard X-ray and soft γ-ray bands should provide crucial information for understanding the high-energy emission mechanisms and the distribution of magnetic fields and radiation fields in the astrophysical sources. TSUBAME has two instruments: the Wide-field Burst Monitor (WBM) and the Hard X-ray Compton Polarimeter (HXCP). The WBM determines on board the direction of the burst occurrence with an accuracy of 10 degrees, then using a high speed attitude control device, the HXCP is pointed to the GRB within 15 seconds after the burst occurrence to promptly detect polarized X-ray photons from the GRB. We present an overview of the TSUBAME mission, its estimated scientific capability for detecting GRBs and measuring their X-ray polarization, development of multi-anode photomultiplier tubes that use ultra bi-alkali photocathodes, and the future plans of this mission.

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