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researcher

Hideyuki Kobayashi

3 papers hereh-index 28 citations9 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author1
  • middle author2

Across the 3 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.IM2
  • astro-ph.GA1
same name
  • Hideyuki Kobayashi — 4 papers
  • Hideyuki Kobayashi — 1 paper
  • Hideyuki Kobayashi — 1 paper, h 1
  • Hideyuki Kobayashi — 1 paper, h 2

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

most citedTrigonometric parallax and proper motion of Sagittarius A* measured by VERA using the new broad-band back-end system OCTAVE-DAS

6 citations · 6 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.IM2026

Low-Frequency VLBI Network Using SKA-LOW

Hideyuki Kobayashi, Tomoaki Oyama, Kazuma Fujita +17

We propose the development of a low-frequency Very Long Baseline Interferometry (VLBI) network operating in the 100-350 MHz range, incorporating the Square Kilometre Array Low (SKA…

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.GA2024★ 6 cited

Trigonometric parallax and proper motion of Sagittarius A* measured by VERA using the new broad-band back-end system OCTAVE-DAS

Tomoaki Oyama, Takumi Nagayama, Aya Yamauchi +12

We successfully measured the trigonometric parallax of Sagittarius A* (Sgr A*) to be 117±17 micro-arcseconds (μas) using the VLBI Exploration of Radio Astrometry (VERA) with…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.