Kotaro Niinuma
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View article: A Possible Shutting-Down Event of Mass Accretion in An Active Galactic Nucleus at z~1.8
A Possible Shutting-Down Event of Mass Accretion in An Active Galactic Nucleus at z~1.8 Open
We present the discovery of a large gradual apparent fading event in optical and near-infrared wavelengths in a quasar at z=1.767 by a factor of 20-30 (in optical) over a period of ~20 years in the observed frame. This pronounced fading tr…
View article: A possible shutting-down event of mass accretion in an active galactic nucleus at z ∼ 1.8
A possible shutting-down event of mass accretion in an active galactic nucleus at z ∼ 1.8 Open
We present the discovery of a large gradual apparent fading event in optical and near-infrared wavelengths in a quasar at $z=1.767$ by a factor of ${\sim}20\!-\!30$ (in optical) over a period of ∼20 yr in the observed frame. This pronounce…
View article: Radio Follow-up Observations of SN 2023ixf by Japanese and Korean Very Long Baseline Interferometers
Radio Follow-up Observations of SN 2023ixf by Japanese and Korean Very Long Baseline Interferometers Open
We report on radio follow-up observations of the nearby Type II supernova SN 2023ixf, spanning from 1.7 to 269.9 days after the explosion, conducted using three very long baseline interferometers (VLBIs), which are the Japanese VLBI Networ…
View article: Radio Follow-up Observations of SN 2023ixf by Japanese and Korean VLBIs
Radio Follow-up Observations of SN 2023ixf by Japanese and Korean VLBIs Open
We report on radio follow-up observations of the nearby Type II supernova, SN 2023ixf, spanning from 1.7 to 269.9 days after the explosion, conducted using three very long baseline interferometers (VLBIs), which are the Japanese VLBI Netwo…
View article: The Japanese vision for the Black Hole Explorer mission
The Japanese vision for the Black Hole Explorer mission Open
Akiyama, Kazunori et al.-- Full list of authors: Akiyama, Kazunori; Niinuma, Kotaro; Hada, Kazuhiro; Doi, Akihiro; Hagiwara, Yoshiaki; Higuchi, Aya E.; Honma, Mareki; Kawashima, Tomohisa; Kolev, Dimitar; Koyama, Shoko; Masui, Sho; Ohsuga, …
View article: The Black Hole Explorer: motivation and vision
The Black Hole Explorer: motivation and vision Open
Johnson, Michael D. et al.-- Full list of authors: Johnson, Michael D.; Akiyama, Kazunori; Baturin, Rebecca; Bilyeu, Bryan; Blackburn, Lindy; Boroson, Don; Cárdenas-Avendaño, Alejandro; Chael, Andrew; Chan, Chi-kwan; Chang, Dominic; Cheime…
View article: Black Hole Spacetime and Properties of Accretion Flows and Jets Probed by Black Hole Explorer: Science Cases Proposed by BHEX Japan Team
Black Hole Spacetime and Properties of Accretion Flows and Jets Probed by Black Hole Explorer: Science Cases Proposed by BHEX Japan Team Open
Black Hole Explorer (BHEX) is a space VLBI mission concept, which can probe the black hole spacetime and the plasma properties including the magnetic fields of the accretion flows and relativistic jets. We propose science cases anticipated…
View article: The Black Hole Explorer: Motivation and Vision
The Black Hole Explorer: Motivation and Vision Open
We present the Black Hole Explorer (BHEX), a mission that will produce the sharpest images in the history of astronomy by extending submillimeter Very-Long-Baseline Interferometry (VLBI) to space. BHEX will discover and measure the bright …
View article: Precessing jet nozzle connecting to a spinning black hole in M87
Precessing jet nozzle connecting to a spinning black hole in M87 Open
View article: Spectral analysis of a parsec-scale jet in M 87: Observational constraint on the magnetic field strengths in the jet
Spectral analysis of a parsec-scale jet in M 87: Observational constraint on the magnetic field strengths in the jet Open
Context. Because of its proximity and the large size of its black hole, M 87 is one of the best targets for studying the launching mechanism of active galactic nucleus jets. Currently, magnetic fields are considered to be an essential fact…
View article: Very Long Baseline Interferometry imaging of H2O maser emission in the nearby radio galaxy NGC 4261
Very Long Baseline Interferometry imaging of H2O maser emission in the nearby radio galaxy NGC 4261 Open
We report dual-frequency very long baseline interferometry (VLBI) observations at 22 and 43 GHz toward the nucleus of a nearby radio galaxy NGC 4261. In particular, we present a VLBI image of the 22 GHz H2O maser line and its location in t…
View article: The Past and Future of East Asia to Italy: Nearly Global VLBI
The Past and Future of East Asia to Italy: Nearly Global VLBI Open
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 between Korean, Japanese, and Italian researchers to study compact sources with …
View article: Precessing jet nozzle connecting to a spinning black hole in M87
Precessing jet nozzle connecting to a spinning black hole in M87 Open
Powerful relativistic jets in active galactic nuclei (AGN) are believed to be originated from the accretion of material onto the supermassive black hole (SMBH) 1 . The nearby radio galaxy M87 is one of the best examples of this phenomenon,…
View article: Spectral analysis of a parsec-scale jet in M87: Observational constraint on the magnetic field strengths in the jet
Spectral analysis of a parsec-scale jet in M87: Observational constraint on the magnetic field strengths in the jet Open
Because of its proximity and the large size of its black hole, M87 is one of the best targets for studying the launching mechanism of active galactic nucleus jets. Currently, magnetic fields are considered to be an essential factor in the …
View article: HINOTORI and Its Perspectives in the Black-Hole Jet Study
HINOTORI and Its Perspectives in the Black-Hole Jet Study Open
Simultaneous multi-band very long baseline interferometry (VLBI) observations at millimeter wavelengths have huge potential for various science cases. However, there exist difficulties in expanding the scientific targets, as the sensitivit…
View article: Recent updates of the Hitachi and Takahagi 32-m radio telescopes, Ibaraki Station
Recent updates of the Hitachi and Takahagi 32-m radio telescopes, Ibaraki Station Open
ogy (NICT), have decided to use these antennas for JVN and East-Asian VLBI Network (EAVN).We will also use these antennas for single-dish and two-element interferometric observations.Conversion from telecommunication antennas to radio tele…
View article: Development for Japan L-band VLBI Observation
Development for Japan L-band VLBI Observation Open
View article: Activities of ngVLA-Japan Science Working Groups
Activities of ngVLA-Japan Science Working Groups Open
The next generation Very Large Array (ngVLA) is an interferometric array planned by the National Radio Astronomical Observatory (NRAO).It will be operational in the late 2030s and improve the sensitivity and angular resolution of the curre…
View article: Overview of the Observing System and Initial Scientific Accomplishments of the East Asian VLBI Network (EAVN)
Overview of the Observing System and Initial Scientific Accomplishments of the East Asian VLBI Network (EAVN) Open
The East Asian VLBI Network (EAVN) is an international VLBI facility in East Asia and is operated under mutual collaboration between East Asian countries, as well as part of Southeast Asian and European countries. EAVN currently consists o…
View article: Detection of a bright burst from the repeating FRB 20201124A at 2 GHz
Detection of a bright burst from the repeating FRB 20201124A at 2 GHz Open
We present a detection of a bright burst from FRB 20201124A, which is one of the most active repeating FRBs, based on S-band observations with the 64-m radio telescope at the Usuda Deep Space Center/JAXA. This is the first FRB observed by …
View article: The Intrinsic Structure of Sagittarius A* at 1.3 cm and 7 mm
The Intrinsic Structure of Sagittarius A* at 1.3 cm and 7 mm Open
Sagittarius A* (Sgr A*), the Galactic Center supermassive black hole (SMBH), is one of the best targets in which to resolve the innermost region of an SMBH with very long baseline interferometry (VLBI). In this study, we have carried out o…
View article: A VLA Survey of Late-time Radio Emission from Superluminous Supernovae and the Host Galaxies
A VLA Survey of Late-time Radio Emission from Superluminous Supernovae and the Host Galaxies Open
We present the results of 3 GHz radio continuum observations of 23 superluminous supernovae (SLSNe) and their host galaxies by using the Karl G. Jansky Very Large Array conducted 5–21 yr after the explosions. The sample consists of 15 Type…
View article: Morphological transition of the compact radio lobe in 3C84 via the strong jet-cloud collision
Morphological transition of the compact radio lobe in 3C84 via the strong jet-cloud collision Open
We report multi-epoch Very Long Baseline Interferometric (VLBI) observations of the compact radio lobe in the radio galaxy 3C84 (NGC1275) during 2016 - 2020. The image sequence of 3C84 reveals that the hotspot in the radio lobe showed the …
View article: East Asian VLBI Network observations of active galactic nuclei jets: imaging with KaVA+Tianma+Nanshan
East Asian VLBI Network observations of active galactic nuclei jets: imaging with KaVA+Tianma+Nanshan Open
The East Asian very-long-baseline interferometry (VLBI) Network (EAVN) is a rapidly evolving international VLBI array that is currently promoted under joint efforts among China, Japan, and Korea. EAVN aims at forming a joint VLBI Network b…
View article: Morphological Transition of the Compact Radio Lobe in 3C 84 via the Strong Jet–Cloud Collision
Morphological Transition of the Compact Radio Lobe in 3C 84 via the Strong Jet–Cloud Collision Open
We report multiepoch very long baseline interferometric observations of the compact radio lobe in the radio galaxy 3C 84 (NGC 1275) during 2016–2020. The image sequence of 3C 84 reveals that the hotspot in the radio lobe showed the 1 year …
View article: A VLA Survey of Late-time Radio Emission from Superluminous Supernovae and the Host Galaxies
A VLA Survey of Late-time Radio Emission from Superluminous Supernovae and the Host Galaxies Open
We present the results of 3 GHz radio continuum observations of 23 superluminous supernovae (SLSNe) and their host galaxies by using the Karl G. Jansky Very Large Array conducted 5-21 years after the explosions. The sample consists of 15 T…
View article: Variability of Late-time Radio Emission in the Superluminous Supernova PTF10hgi
Variability of Late-time Radio Emission in the Superluminous Supernova PTF10hgi Open
We report the time variability of the late-time radio emission in a Type I superluminous supernova (SLSN), PTF10hgi, at z = 0.0987. The Karl G. Jansky Very Large Array 3 GHz observations at 8.6 and 10 yr after the explosion both detected r…
View article: Millimeter-VLBI Detection and Imaging of the Gravitationally Lensed Gamma-Ray Blazar JVAS B0218+357
Millimeter-VLBI Detection and Imaging of the Gravitationally Lensed Gamma-Ray Blazar JVAS B0218+357 Open
We observed the gravitationally lensed blazar JVAS B0218+357 with the KVN and VERA Array (KaVA) at 22, 43, and 86 GHz. The source has recently been identified as an active gamma-ray source up to GeV/TeV energy bands, rendering a unique tar…
View article: Millimeter-VLBI Detection and Imaging of the Gravitationally Lensed γ-Ray Blazar JVAS B0218+357
Millimeter-VLBI Detection and Imaging of the Gravitationally Lensed γ-Ray Blazar JVAS B0218+357 Open
We observed the gravitationally lensed blazar JVAS B0218+357 with the KVN and VERA Array (KaVA) at 22, 43, and 86 GHz. The source has recently been identified as an active γ -ray source up to GeV/TeV energy bands, rendering a unique target…
View article: Stable Radio Core of the Blazar Mrk 501 during High-energy Active State in 2012
Stable Radio Core of the Blazar Mrk 501 during High-energy Active State in 2012 Open
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 revisiting from the perspective of astrometry the six-epoch observations with the …