スポンサーリンク
Mizusawa Vlbi Observatory National Astronomical Observatory Of Japan | 論文
- Astrometry of H_2O Masers in Nearby Star-Forming Regions with VERA III : IRAS 22198+6336 in Lynds 1204G
- Dual-Beam Delay Calibration for VERA
- Astrometry of H_2O Masers in Nearby Star-Forming Regions with VERA II SVS 13 in NGC 1333
- Astrometry of H_2O Masers in Nearby Star-Forming Regions with VERA I : IRAS 16293-2422 in ρ Oph East
- Distance to Orion KL Measured with VERA
- Astrometry of Galactic Star-Forming Region Sharpless 269 with VERA : Parallax Measurements and Constraint on Outer Rotation Curve
- Absolute Proper Motions of H_2O Masers Away from the Galactic Plane Measured with VERA in the "Superbubble" Region NGC 281
- VERA Observations of H_2O Maser Sources in Three Massive Star-Forming Regions and Galactic Rotation Measurements
- Four-way Doppler measurements and inverse VLBI observations for the Martian exploration(Satellite Systems,ICSANE 2010 (International Conference on Space, Aeronautical and Navigational Electronics))
- Statistical Properties of Stellar H_2O Masers : Results of Three-Year Single-Dish Observations with the VERA Iriki Telescope
- VLBI Detections of Parsec-Scale Nonthermal Jets in Radio-Loud Broad Absorption Line Quasars
- Astrometric VLBI Observation of PSR 0329+54
- Japanese VLBI Network Mapping of SiO v = 3 J = 1-0 Maser Emission in W Hydrae
- Astrometry of the star-forming region IRAS 05137 + 3919 in the far outer Galaxy (Special feature: Recent results from VERA)
- Astrometry of H2O masers in nearby star-forming regions with VERA (4) L 1448 C (Special feature: Recent results from VERA)
- Determination of the Pattern Speed of Barred Spiral Galaxies
- Nobeyama Millimeter Array Observations of the Nuclear Starburst of M83 : A GMA Scale Correlation between Dense Gas Fraction and Star Formation Efficiency
- Hubble Constant at Intermediate Redshift Using the CO-Line Tully-Fisher Relation
- CO Observations of Luminous IR Galaxies at Intermediate Redshift
- Distance Measurement of Galaxies to a Redshift of-0.1 Using the CO-Line Tully-Fisher Relation