H. Shibai

7 papers receiving 73 citations

Peers

H. Shibai
Comparison fields: 5 of 22
  • Astronomy and Astrophysics 64
  • Atomic and Molecular Physics, and Optics 17
  • Atmospheric Science 13
  • Spectroscopy 10
  • Geophysics 6
Replace L. K. Deutsch with:
L. K. Deutsch United States
S. D. Sidher United Kingdom
A. Popovas Denmark
E. Baker United States
Jeehyun Yang United States
G. Chlewicki Netherlands
S. A. Khaibrakhmanov Russia
R. Y. Shuping United States
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H. Shibai relative to L. K. Deutsch United States L. K. Deutsch's profile →
Citations per field
00.5×
L. K. Deutsch · 1×
Citations per year

Countries citing papers authored by H. Shibai

Since Specialization
Citations

This map shows the geographic impact of H. Shibai's research. It shows the number of citations coming from papers published by authors working in each country. You can also color the map by specialization and compare the number of citations received by H. Shibai with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites H. Shibai more than expected).

Fields of papers citing papers by H. Shibai

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by H. Shibai. Nodes represent research fields, and links connect fields that are likely to share authors. Colored nodes show fields that tend to cite the papers produced by H. Shibai. The network helps show where H. Shibai may publish in the future.

Co-authorship network of co-authors of H. Shibai

This figure shows the co-authorship network connecting the top 25 collaborators of H. Shibai. A scholar is included among the top collaborators of H. Shibai based on the total number of citations received by their joint publications. Widths of edges represent the number of papers authors have co-authored together. Node borders signify the number of papers an author published with H. Shibai. H. Shibai is excluded from the visualization to improve readability, since they are connected to all nodes in the network.

All Works

8 of 8 papers shown
#WorkIndexed citations
1
Coming in from the cold: the galactic plane source populations revealed by AKARI
0
2
ASTRO-F/FIS observing simulation including detector effects
1
3 37
4
Absorption spectra of Mg-rich Mg-Fe and Ca pyroxenes in the mid- and far-infrared regions
19
5
Diffuse [CII] 158 Micron Line Emission from the Interstellar Matter at High Galactic Latitude
1
6
Infrared spectroscopic observation of methane in Comet P/Halley
15
7 2
8
Observations of diffuse far infrared emission and distribution of interstellar dust
1

About H. Shibai

H. Shibai is a scholar working on Astronomy and Astrophysics, Spectroscopy and Atmospheric Science, having authored 8 papers that have together received 76 indexed citations. Recurring topics across this work include Astrophysics and Star Formation Studies (4 papers), Astro and Planetary Science (3 papers) and Atmospheric Ozone and Climate (2 papers). The work is most often cited by research in Astronomy and Astrophysics (64 citations), Instrumentation (4 citations) and Atmospheric Science (13 citations). H. Shibai has collaborated with scholars based in Japan and United States. Frequent co-authors include Ko Okumura, Takashi Onaka, Brooke Gregory, Toshihiko Tanabé, H. Okuda, I. Yamamura, Takao Nakagawa, Thomas L. Roellig, Tokihiro Yamamoto and C. Koike. Their work appears in journals such as The Astrophysical Journal, Publications of the Astronomical Society of the Pacific and Journal of The Korean Astronomical Society.

Rankless uses publication and citation data sourced from OpenAlex, an open and comprehensive bibliographic database. While OpenAlex provides broad and valuable coverage of the global research landscape, it—like all bibliographic datasets—has inherent limitations. These include incomplete records, variations in author disambiguation, differences in journal indexing, and delays in data updates. As a result, some metrics and network relationships displayed in Rankless may not fully capture the entirety of a scholar's output or impact.

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2026