Experimental Astrophysics group in Tokyo Metropolitan University, X-ray Astronomy & Astrophysics

Ishida, (Manabu Ishida)

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Name

Ishida, (Manabu Ishida)

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Professor, Institute of space sciences (And cooperation with Tokyo Metropolitan University)

Outline of research

  • White dwarf、Dwarf novae、Strong magnetic field cataclysmic、X-ray pulsar
  • Development of the President-elect with X x-ray astronomical satellite Astro-h X-ray telescope
  • Development of a next-generation high-definition X-ray telescope
  • Data analysis of X-ray astronomy satellite is currently active in orbit "Suzaku"、And education and research guidance

Contact

Ishida(@)Astro.ISAs.JAXA.jp

Details of the study

Science by Suzaku

  1. Elucidation of the physical state of the boundary layer of dwarf novae and geometry
  2. Kinematics of the accretion column gas of strongly Magnetic Cataclysmic variable stars, x-ray pulsars
  3. Application of x-ray radiation from strongly Magnetic Cataclysmic variable stars accretion column model establishment and observation data

Astro-h satellite development

  1. Development of a next-generation high-definition X-ray telescope
  2. Development of an optical table ( EOB )

Research history

1987Year -1992, Department of physics, Department of graduate school of m.s., University of Tokyo, Ph.d., (Makishima lab)

  • "Ginga" low-mass x-ray binary star system based on satellite data(LMXB)And strongly Magnetic Cataclysmic variable star(mCV)Of the research
  • ASCA satellite equipped with aerial imaging gas scintillation proportional counter(GIS)Of the development

19922001 research associate, education science Department of space science Institute of high energy celestial physics first.

  • Discovery of mCV in ASCA satellite SIS data by the white dwarf's mass method
  • Heavy element compositions of Supernova Remnants with ASCA satellite SIS data
  • "Asuka" clusters of galaxies coalesced using the data of the satellite GIS、And the study of temperature distribution
  • Discovery of X-ray sources in globular clusters with ASCA satellite GIS data
  • GIS ASCA satellite orbit maintenance and calibration test
  • Leading reciprocal in all instruments of the ASCA satellite orbit calibration and construction of response function
  • Day-to-day operations of the "Asuka" satellite、Emergency response、Power Management、Other responsibility in charge of the satellite maintenance General
  • Astro-E satellite equipped with extension type optical bench(EOB)Of the development
  • Astro-E satellite equipped with x-ray telescopes(XRT)The development and calibration test for ground
  • Command creation support software ISACS Plan development and development of the system for Astro-E command create it using

2001In 2005, Tokyo Metropolitan University and capital University of Tokyo associate professor.

  • Study of the accretion flow to the magnetic poles of the x-ray pulsars with ASCA satellite data
  • Discovery of X-ray sources in globular clusters with ASCA satellite data
  • "XMM-Newton" satellite、Cataclysmic by high-resolution spectroscopic data of the "Chandra" satellite(CV)Of the research
  • Studies of Circumstellar matter of the Chandra satellite data x-ray pulsars
  • Chandra satellite、A study of the mass distribution of galaxy clusters by the data of the XMM-Newton satellite
  • Participate in the do Warm-Hot Intergalactic Medium distribution and unidentified baryon exploration DIOS mission
  • Astro-E2 satellite equipped with XRT development and calibration test for ground
  • Development of Astro-E2 satellite equipped with XRT for pre-collimator
  • Development of Astro-E2 satellite equipped with EOB
  • Astro-E2 satellite、Responsibility responsible for the measurement and adjustment of the PI devices mutual alignment on the ground
  • Research and development aimed at the high resolution of the NeXT satellite equipped with x-ray telescopes
  • Development of the NeXT satellite with EOB

2006Year - current Professor, Institute of space sciences (And cooperation with Tokyo Metropolitan University)

  • Elucidation of the physical state of the boundary layer of dwarf novae and geometry
  • Kinematics of the accretion column gas of strongly Magnetic Cataclysmic variable stars, x-ray pulsars
  • Application of x-ray radiation from strongly Magnetic Cataclysmic variable stars accretion column model establishment and observation data
  • Astro-h satellite development
  • Development of a next-generation high-definition X-ray telescope
  • An optical units(EOB)Of the development
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