Profile
Name
Ishida, (Manabu Ishida)
Profile
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
- 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
- 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