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researcher

Y. Okada

41 papers hereh-index 202.1k citations104 works total

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

author position
  • first author8
  • middle author23
  • last author5

Across the 36 of 41 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA22
  • astro-ph11
  • astro-ph.IM5
  • astro-ph.CO2
  • astro-ph.EP1
same name
  • Y. Okada — 86 papers, h 43
  • Y. Okada — 28 papers, h 22
  • Y. Okada — 8 papers, h 13
  • Y. Okada — 8 papers, h 3
  • Y. Okada — 7 papers, h 13
  • Y. Okada — 7 papers, h 5

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
20032026
most citedThe Infrared Astronomical Mission AKARI

842 citations · 2.6k across the 41 of their papers we have counts for

collaborators
Showing 2021Show all

3 papers · 1 filter

astro-ph.GA2021★ 33 cited

Self-absorption in [CII], 12CO, and HI in RCW120. Building up a geometrical and physical model of the region

S. Kabanovic, N. Schneider, V. Ossenkopf-Okada +19

Revealing the 3D dynamics of HII regions and their associated molecular clouds is important for understanding the longstanding problem as to how stellar feedback affects the densit…

astro-ph.CO2021★ 101 cited

CCAT-prime Collaboration: Science Goals and Forecasts with Prime-Cam on the Fred Young Submillimeter Telescope

Prime collaboration, M. Aravena, J. E. Austermann +84

We present a detailed overview of the science goals and predictions for the Prime-Cam direct detection camera/spectrometer being constructed by the CCAT-prime collaboration for ded…

astro-ph.IM2021★ 15 cited

Observation and calibration strategies for large-scale multi-beam velocity-resolved mapping of the [CII] emission in the Orion molecular cloud

R. Higgins, S. Kabanovic, C. Pabst +15

Context. The [CII] 158micron far-infrared fine-structure line is one of the dominant cooling lines of the star-forming interstellar medium (ISM). Hence [CII] emission originates in…

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