activity
20242026
collaborators

8 papers

astro-ph.HE2026

Resolving Nearby Supermassive Black Holes with the Black Hole Explorer

Yuto Akiyama, Kazunori Akiyama, Dominic W. Pesce +12

Recent Event Horizon Telescope results have demonstrated unique and transformative science in gravitational physics and black hole astrophysics enabled by event-horizon-scale imagi…

astro-ph.HE2026

Radio Constraints on the Circumstellar Environment of the Type IIb Supernova SN 2024iss

Yuhei Iwata, Tomoki Matsuoka, Masanori Akimoto +6

Type~IIb supernovae exhibit diverse progenitor properties, and radio observations offer a unique probe of their mass-loss histories shortly before the explosion. We present Japanes…

astro-ph.IM2026

Black Hole Explorer Mission Development in Japan

Kazunori Akiyama, Mareki Honma, Akihiro Doi +21

The Black Hole Explorer (BHEX) is a next-generation space very-long-baseline interferometry (VLBI) mission concept that will extend existing ground-based millimeter/submillimeter V…

astro-ph.HE2026

VLBI Astrometry of Magnetars

Takuya Akahori, Sujin Eie, Kei Amada +8

The origin of the strongest magnetic fields in the Universe, i.e., the origin of magnetars, is a longstanding question. An enhanced dynamo effect in an irregular supernova explosio…

astro-ph.IM2026

VLBI-Enabled Localization of Continuous GW Sources

Keitaro Takahashi, Takuya Akahori, Kenta Fujisawa +8

Pulsar timing arrays (PTAs) are opening the nanohertz gravitational-wave (GW) band by timing millisecond pulsars (MSPs) to target signals from supermassive black hole binaries (SMB…

astro-ph.SR2026

Fast variability and circular polarization of the 6.7 GHz methanol maser in G33.6410.228

Kenta Fujisawa, Yui Sugiura, Yuta Kojima +5

The 6.7 GHz methanol maser in a high-mass star-forming region G33.6410.228 is known to exhibit burst-like flux variability due to an unknown mechanism. To investigate the burst…