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researcher

M. Kohno

51 papers hereh-index 15755 citations58 works total

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

author position
  • first author10
  • middle author36
  • last author3

Across the 49 of 51 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA50
  • astro-ph.IM1
same name
  • M. Kohno — 37 papers, h 15
  • M. Kohno — 26 papers, h 18
  • M. Kohno — 8 papers, h 4
  • M. Kohno — 7 papers, h 5
  • M. Kohno — 3 papers, h 4
  • M. Kohno — 3 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
20162026
most citedFOREST Unbiased Galactic plane Imaging survey with the Nobeyama 45-m telescope (FUGIN) I: Project Overview and Initial Results

205 citations · 1.1k across the 51 of their papers we have counts for

collaborators
Showing 2022Show all

3 papers · 1 filter

astro-ph.GA2022★ 11 cited

Distance determination of molecular clouds in the 1st quadrant of the Galactic plane using deep learning : I. Method and Results

Shinji Fujita, A. M. Ito, Yusuke Miyamoto +15

Machine learning has been successfully applied in varied field but whether it is a viable tool for determining the distance to molecular clouds in the Galaxy is an open question. I…

astro-ph.GA2022★ 9 cited

Ammonia mapping observations toward the Galactic massive star-forming region Sh 2-255 and Sh 2-257

Mikito Kohno, Toshihiro Omodaka, Toshihiro Handa +9

We performed NH3​ (J,K)=(1,1),(2,2), and (3,3) mapping observations toward the Galactic massive star-forming region Sh 2-255 and Sh 2-257 using the Nobeyama 45-m telescope as…

astro-ph.GA2022★ 24 cited

Velocity structure of the 50 pc-long NGC 6334 filamentary cloud: Hints of multiple compressions and their impact on the cloud properties?

Doris Arzoumanian, Delphine Russeil, Annie Zavagno +8

[Abridged] The interstellar medium is observed to be organised in filamentary structures, as well as neutral (HI) and ionized (HII) bubbles. The expanding nature of these bubbles m…

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