K. Mase

742 citations
4 papers · 35 · h-index 3

Impact in

    • Astrophysics and Cosmic Phenomena
    • Dark Matter and Cosmic Phenomena
    • Neutrino Physics Research
    • X-ray Spectroscopy and Fluorescence Analysis
    • Advanced X-ray Imaging Techniques

Papers in

    • Nuclear Physics and Applications 2
    • Advanced X-ray Imaging Techniques 1
    • Dark Matter and Cosmic Phenomena 2
    • Astrophysics and Cosmic Phenomena 2
    • Neutrino Physics Research 1

K. Mase

3 papers receiving 34 citations

Peers

K. Mase
Comparison fields: 5 of 17
  • Nuclear and High Energy Physics 20
  • Radiation 9
  • Condensed Matter Physics 4
  • Astronomy and Astrophysics 4
  • Materials Chemistry 7
Replace V.L. Solovyanov with:
V.L. Solovyanov Russia
H.E. Roloff Germany
R. Wedenig Austria
A. I. Mincer United States
T. Sugimoto Japan
I. Dumanoğlu Türkiye
G. N. Kniajeva Finland
J.-P. Mendiburu France
T. Lagouri Germany
U. Dosselli Italy
K. Mase relative to V.L. Solovyanov Russia V.L. Solovyanov's profile →
Citations per field
00.5×1.5×
V.L. Solovyanov · 1×
Citations per year

Countries citing papers authored by K. Mase

Since Specialization
Citations

This map shows the geographic impact of K. Mase'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 K. Mase with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites K. Mase more than expected).

Fields of papers citing papers by K. Mase

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by K. Mase. 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 K. Mase. The network helps show where K. Mase may publish in the future.

Co-authors

The 11 scholars most cited alongside K. Mase, linked wherever they have co-authored with each other. Click a name or a connecting line to browse the papers they share.

Border = papers with K. Mase Line = papers co-authored together K. Mase links everyone, so they are left out of the graph.

All Works

4 of 4 papers shown

About K. Mase

K. Mase is a scholar working on Radiation, Nuclear and High Energy Physics, Condensed Matter Physics, Astronomy and Astrophysics and Materials Chemistry, having authored 4 papers that have together received 35 indexed citations. Recurring topics across this work include Dark Matter and Cosmic Phenomena (2 papers), Nuclear Physics and Applications (2 papers), Astrophysics and Cosmic Phenomena (2 papers), X-ray Diffraction in Crystallography (1 paper), Radio Astronomy Observations and Technology (1 paper), Neutrino Physics Research (1 paper), Crystallography and Radiation Phenomena (1 paper) and Advanced X-ray Imaging Techniques (1 paper). The work is most often cited by research in Nuclear and High Energy Physics (20 citations), Radiation (9 citations), Condensed Matter Physics (4 citations), Astronomy and Astrophysics (4 citations) and Materials Chemistry (7 citations). K. Mase has collaborated with scholars based in Japan, United States and Germany. Frequent co-authors include Tokonatsu Yamamoto, Н. Сакаки, Yoshiyuki Amemiya, M. Takeda, M. Teshima, Hiroo Hashizume, Hidetoshi Hashizume, K. Kohra, Kazutake Köhra and M. Ave. Their work appears in journals such as Astroparticle Physics, Japanese Journal of Applied Physics, Nuclear Instruments and Methods and International Cosmic Ray Conference.

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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