논문 상세보기

OPTICAL-INFRARED AND HIGH-ENERGY ASTRONOMY COLLABORATION AT HIROSHIMA ASTROPHYSICAL SCIENCE CENTER KCI 등재

Makoto Uemura, Michitoshi Yoshida, Koji, S. Kawabata, Tsunefumi Mizuno, Yasuyuki, T. Tanaka, Hiroshi Akitaya, Yousuke Utsumi, Yuki Moritani, Ryosuke Itoh, Yasushi Fukazawa, Hiromitsu Takahashi, Masanori Ohno, Takahiro Ui, Katsutoshi Takaki, Nana Ebisuda, Kenji Kawaguchi, Kensyo Mori, Yuma Ohashi, Yuka Kanda, Miho Kawabata, Koji Takata, Tatsuya Nakaoka
  • 언어ENG
  • URLhttps://db.koreascholar.com/Article/Detail/385725
구독 기관 인증 시 무료 이용이 가능합니다. 3,000원
천문학논총 (Publications of the Korean Astronomical Society)
한국천문학회 (Korean Astronomical Society)
초록

The Hiroshima Astrophysical Science Center (HASC) was founded in 2004 at Hiroshima University, Japan. The main mission of this institute is the observational study of various transient objects includ- ing gamma-ray bursts, supernovae, novae, cataclysmic variables, and active galactic nuclei by means of multi-wavelength observations. HASC consists of three divisions; the optical-infrared astronomy divi- sion, high-energy astronomy division, and theoretical astronomy division. HASC is operating the 1.5m optical-infrared telescope Kanata, which is dedicated to follow-up and monitoring observations of transient objects. The high-energy division is the key operation center for the Fermi gamma-ray space telescope. HASC and the high-energy astronomy group in the department of physical science at Hiroshima University are closely collaborating with each other to promote multi-wavelength time-domain astronomy. We report the recent activities of HASC and some science topics pursued by this multi-wavelength collaboration.

키워드
telescopes
목차
ABSTRACT
1. INTRODUCTION
2. JET SOURCES AND POLARIMETRIC OBSERVA-TIONS
3. SIMULTANEOUS MULTI-BAND OBSERVATIONS
4. SUMMARY
REFERENCES
저자
  • Makoto Uemura(Hiroshima Astrophysical Science Center, Hiroshima University)
  • Michitoshi Yoshida(Hiroshima Astrophysical Science Center, Hiroshima University)
  • Koji, S. Kawabata(Hiroshima Astrophysical Science Center, Hiroshima University)
  • Tsunefumi Mizuno(Hiroshima Astrophysical Science Center, Hiroshima University)
  • Yasuyuki, T. Tanaka(Hiroshima Astrophysical Science Center, Hiroshima University)
  • Hiroshi Akitaya(Hiroshima Astrophysical Science Center, Hiroshima University)
  • Yousuke Utsumi(Hiroshima Astrophysical Science Center, Hiroshima University)
  • Yuki Moritani(Hiroshima Astrophysical Science Center, Hiroshima University)
  • Ryosuke Itoh(Department of Physical Sciences, Hiroshima University)
  • Yasushi Fukazawa(Department of Physical Sciences, Hiroshima University)
  • Hiromitsu Takahashi(Department of Physical Sciences, Hiroshima University)
  • Masanori Ohno(Department of Physical Sciences, Hiroshima University)
  • Takahiro Ui(Department of Physical Sciences, Hiroshima University)
  • Katsutoshi Takaki(Department of Physical Sciences, Hiroshima University)
  • Nana Ebisuda(Department of Physical Sciences, Hiroshima University)
  • Kenji Kawaguchi(Department of Physical Sciences, Hiroshima University)
  • Kensyo Mori(Department of Physical Sciences, Hiroshima University)
  • Yuma Ohashi(Department of Physical Sciences, Hiroshima University)
  • Yuka Kanda(Department of Physical Sciences, Hiroshima University)
  • Miho Kawabata(Department of Physical Sciences, Hiroshima University)
  • Koji Takata(Department of Physical Sciences, Hiroshima University)
  • Tatsuya Nakaoka(Department of Physical Sciences, Hiroshima University)