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researcher

H. Terada

90 papers hereh-index 405.1k citations282 works total

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

author position
  • first author3
  • middle author70
  • last author4

Across the 77 of 90 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR29
  • astro-ph27
  • astro-ph.EP24
  • astro-ph.GA3
  • astro-ph.IM3
  • astro-ph.CO1
same name
  • H. Terada — 21 papers, h 10
  • H. Terada — 2 papers, 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

activity
19992023
most citedDiscovery of Small-Scale Spiral Structures in the Disk of SAO 206462 (HD 135344B): Implications for the Physical State of the Disk from Spiral Density Wave Theory

399 citations · 3.8k across the 90 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

3 papers · 1 filter

astro-ph.GA2021

Study of the Inner Structure of the Molecular Torus in IRAS 08572+3915 NW with Velocity Decomposition of CO Rovibrational Absorption Lines

Shusuke Onishi, Takao Nakagawa, Shunsuke Baba +6

Understanding the inner structure of the clumpy molecular torus surrounding the active galactic nucleus is essential in revealing the forming mechanism. However, spatially resolvin…

astro-ph.GA2015★ 48 cited

Subaru Telescope adaptive optics observations of gravitationally lensed quasars in the Sloan Digital Sky Survey

Cristian E. Rusu, Masamune Oguri, Yosuke Minowa +12

We present the results of an imaging observation campaign conducted with the Subaru Telescope adaptive optics system (IRCS+AO188) on 28 gravitationally lensed quasars (23 doubles,…

astro-ph.GA2014★ 8 cited

Indications of M-dwarf Deficits in the Halo and Thick Disk of the Galaxy

Mihoko Konishi, Hiroshi Shibai, Takahiro Sumi +55

We compared the number of faint stars detected in deep survey fields with the current stellar distribution model of the Galaxy and found that the detected number in the H band is s…

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