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A. Ueda

28 papers hereh-index 242.1k citations87 works total

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

author position
  • middle author21
  • last author3

Across the 24 of 28 papers where every author was matched, so the position is known.

fields
  • astro-ph.EP13
  • astro-ph.IM10
  • astro-ph.SR3
  • astro-ph1
  • astro-ph.HE1
same name
  • A. Ueda — 8 papers, h 11
  • A. Ueda — 5 papers, h 5
  • A. Ueda — 4 papers
  • A. Ueda — 4 papers, h 11
  • A. Ueda — 4 papers, h 17
  • A. Ueda — 4 papers, h 33

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

activity
20012024
most citedStable Operation of a 300-m Laser Interferometer with Sufficient Sensitivity to Detect Gravitational-Wave Events within our Galaxy

282 citations · 1k across the 28 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

3 papers · 1 filter

astro-ph.SR2023★ 4 cited

Direct Imaging Explorations for Companions around Mid-Late M Stars from the Subaru/IRD Strategic Program

Taichi Uyama, Charles Beichman, Masayuki Kuzuhara +32

The Subaru telescope is currently performing a strategic program (SSP) using the high-precision near-infrared (NIR) spectrometer IRD to search for exoplanets around nearby mid/late…

astro-ph.SR2021

Silicon and Strontium abundances of very metal-poor stars determined from near-infrared spectra

Wako Aoki, Timothy C. Beers, Satoshi Honda +19

Silicon and Strontium are key elements to explore the nucleosynthesis and chemical evolution of the Galaxy by measurements of very metal-poor stars. There are, however, only a few…

astro-ph.SR2021★ 30 cited

Elemental abundances of nearby M dwarfs based on high-resolution near-infrared spectra obtained by the Subaru/IRD survey: Proof of concept

Hiroyuki Tako Ishikawa, Wako Aoki, Teruyuki Hirano +24

Detailed chemical analyses of M dwarfs are scarce but necessary to constrain the formation environment and internal structure of planets being found around them. We present element…

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