Search Results - "Niinuma, Kotaro"
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Parabolic Jets from the Spinning Black Hole in M87
Published in The Astrophysical journal (01-12-2018)“…The M87 jet is extensively examined by utilizing general relativistic magnetohydrodynamic (GRMHD) simulations, as well as the steady axisymmetric force-free…”
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2
Kinematics of the M87 Jet in the Collimation Zone: Gradual Acceleration and Velocity Stratification
Published in The Astrophysical journal (20-12-2019)“…We study the kinematics of the M87 jet using the first-year data of the KVN and VERA Array (KaVA) large program, which has densely monitored the jet at 22 and…”
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A VLA Survey of Late-time Radio Emission from Superluminous Supernovae and the Host Galaxies
Published in The Astrophysical journal (01-11-2021)“…Abstract We present the results of 3 GHz radio continuum observations of 23 superluminous supernovae (SLSNe) and their host galaxies by using the Karl G…”
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The First VERA Astrometry Catalog
Published in Publications of the Astronomical Society of Japan (01-08-2020)“…Abstract We present the first astrometry catalog from the Japanese VLBI (very long baseline interferometer) project VERA (VLBI Exploration of Radio…”
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Pilot KaVA monitoring on the M 87 jet: Confirming the inner jet structure and superluminal motions at sub-pc scales
Published in Publications of the Astronomical Society of Japan (01-08-2017)“…Abstract We report the initial results of our high-cadence monitoring program on the radio jet in the active galaxy M 87, obtained by the KVN and VERA Array…”
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6
Detection of a bright burst from the repeating fast radio burst 20201124A at 2 GHz
Published in Publications of the Astronomical Society of Japan (06-02-2023)“…Abstract We present a detection of a bright burst from the fast radio burst (FRB) 20201124A, which is one of the most active repeating FRBs, based on S-band…”
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Fundamental Parameters of the Milky Way Galaxy Based on VLBI Astrometry
Published in Publications of the Astronomical Society of Japan (25-12-2012)“…We present analyses to determine the fundamental parameters of the Galaxy based on VLBI astrometry of 52 Galactic maser sources obtained with VERA, VLBA, and…”
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Spatially resolved molecular gas properties of host galaxy of Type I superluminous supernova SN 2017egm
Published in Publications of the Astronomical Society of Japan (01-08-2020)“…Abstract We present the results of CO(1–0) observations of the host galaxy of a Type I superluminous supernova (SLSN-I), SN 2017egm, one of the closest SLSNe-I…”
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9
The Yamaguchi Interferometer
Published in Publications of the Astronomical Society of Japan (01-12-2022)“…Abstract We report on the Yamaguchi Interferometer (YI), a one-baseline radio interferometer consisting of two radio telescopes with diameters of 32 m and 34…”
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Mid-infrared Excess from the West Hot Spot of the Radio Galaxy Pictor A Unveiled by WISE
Published in The Astrophysical journal (01-12-2017)“…Mid-infrared properties are reported of the west hot spot of the radio galaxy Pictor A with the Wide-field Infrared Survey Explorer (WISE). The mid-infrared…”
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Observations of V404 Cygni during the 2015 outburst by the Nasu telescope array at 1.4 GHz
Published in Publications of the Astronomical Society of Japan (01-10-2020)“…Abstract Waseda University Nasu telescope array is a spatial fast Fourier transform interferometer consisting of eight linearly aligned antennas with 20 m…”
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12
Accelerating a water maser face-on jet from a high mass young stellar object
Published in Publications of the Astronomical Society of Japan (01-10-2016)“…Abstract We report on long-term single-dish and VLBI monitoring for intermittent flare activities of a dominant blue-shifted H2O maser associated with a…”
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13
A Face-on Accretion System in High-mass Star Formation: Possible Dusty Infall Streams within 100 AU
Published in The Astrophysical journal (01-11-2017)“…We report on interferometric observations of a face-on accretion system around the high-mass young stellar object, G353.273+0.641. The innermost accretion…”
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14
Stable Radio Core of the Blazar Mrk 501 during High-energy Active State in 2012
Published in The Astrophysical journal (20-10-2019)“…We investigate the precise location of the radio core in the nearby blazar Mrk 501 for the first time during its X-ray and TeV γ-ray active state in 2012 by…”
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A comparative study of amplitude calibrations for the East Asia VLBI Network: A priori and template spectrum methods
Published in Publications of the Astronomical Society of Japan (01-12-2017)“…Abstract We present the results of a comparative study of amplitude calibrations for the East Asia VLBI Network (EAVN) at 22 and 43 GHz using two different…”
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VERA monitoring of the radio jet 3C 84 in the period of 2007–2013: Detection of non-linear motion
Published in Publications of the Astronomical Society of Japan (01-10-2018)“…Abstract We present a kinematic study of the sub-parsec-scale radio jet of the radio galaxy 3C 84/NGC 1275 with the VLBI Exploration of Radio Astrometry (VERA)…”
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17
The Hitachi and Takahagi 32 m radio telescopes: Upgrade of the antennas from satellite communication to radio astronomy
Published in Publications of the Astronomical Society of Japan (01-10-2016)“…Abstract The Hitachi and Takahagi 32 m radio telescopes (former satellite communication antennas) were so upgraded as to work at 6, 8, and 22 GHz. We developed…”
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HINOTORI and Its Perspectives in the Black-Hole Jet Study
Published in Galaxies (01-02-2023)“…Simultaneous multi-band very long baseline interferometry (VLBI) observations at millimeter wavelengths have huge potential for various science cases. However,…”
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The Past and Future of East Asia to Italy: Nearly Global VLBI
Published in Galaxies (01-04-2023)“…We present here the East Asia to Italy Nearly Global VLBI (EATING VLBI) project. How this project started and the evolution of the international collaboration…”
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Observations of the bursting activity of the 6.7 GHz methanol maser in G33.641−0.228
Published in Publications of the Astronomical Society of Japan (01-12-2014)“…Abstract We have observed bursting variability of the 6.7 GHz methanol maser of G33.641−0.228. Five bursts were detected in the observation period of 294 days…”
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