This map shows the geographic impact of M. Ohno'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 M. Ohno with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites M. Ohno more than expected).
This network shows the impact of papers produced by M. Ohno. 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 M. Ohno. The network helps show where M. Ohno may publish in the future.
Co-authorship network of co-authors of M. Ohno
This figure shows the co-authorship network connecting the top 25 collaborators of M. Ohno.
A scholar is included among the top collaborators of M. Ohno 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 M. Ohno. M. Ohno is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
All Works
20 of 20 papers shown
1.
Katsuda, Satoru, et al.. (2020). Inverse First Ionization Potential Effects in Giant Solar Flares Found from Earth X-Ray Albedo with Suzaku/XIS. Repository of the Academy's Library (Library of the Hungarian Academy of Sciences).17 indexed citations
2.
Ohno, M., M. Arimoto, Niccolò Di Lalla, N. Omodei, & F. Longo. (2020). GRB 200716C: Fermi-LAT detection. GRB Coordinates Network. 28130. 1.
3.
Uchida, Nagomi, H. Takahashi, M. Ohno, et al.. (2020). Attenuation characteristics of a Ce:Gd3Al2Ga3O12 scintillator. Nuclear Instruments and Methods in Physics Research Section A Accelerators Spectrometers Detectors and Associated Equipment. 986. 164725–164725.5 indexed citations
Longo, F., E. Bissaldi, G. Vianello, et al.. (2016). GRB 160509A: Fermi-LAT refined analysis.. GRB Coordinates Network. 19413. 1.1 indexed citations
6.
Longo, F., et al.. (2016). GRB 160509A: Fermi-LAT prompt detection of a very bright burst.. GRB Coordinates Network. 19403. 1.1 indexed citations
7.
Racusin, J. L., S. Zhu, D. Kocevski, et al.. (2013). GRB 131108A: Fermi-LAT onboard detection of a burst.. GCN. 15464. 1.2 indexed citations
8.
Ohno, M., G. Vianello, J. L. Racusin, & Э. Сонбас. (2012). GRB 121011A: Fermi-LAT detection of a burst.. GCN. 13859. 1.1 indexed citations
9.
Ohno, M., H. Takahashi, Yasuyuki Tanaka, et al.. (2011). Fermi LAT and GBM detection of the X2.1 Solar Flare of September 6 2011. ATel. 3635. 1.
10.
Ishikawa, Shin-nosuke, S. Krucker, M. Ohno, et al.. (2011). Suzaku/WAM and RHESSI observation of non-thermal electrons in solar microflares. AGUFM. 2011.1 indexed citations
Cutini, S., et al.. (2009). Fermi LAT and GBM detections of GRB090328.. GCN. 9044. 1.1 indexed citations
15.
Ohno, M., et al.. (2009). Fermi GBM and LAT detections of GRB 090323.. GRB Coordinates Network. 9021. 1.2 indexed citations
16.
Ohno, M. & V. Pelassa. (2009). Fermi LAT detection of GRB 090510.. GCN. 9334. 1.2 indexed citations
17.
Ohno, M., et al.. (2009). GRB090217: Fermi-LAT detection.. GCN. 8903. 1.
18.
Fukazawa, Yasushi, Hirohisa Shirai, M. Ohno, et al.. (2007). Suzaku Observations of the Seyfert 2 Galaxy NGC 4388. ASPC. 373. 165.
19.
Sato, G., Kazuhiro Nakazawa, T. Takahashi, et al.. (2006). GRB 060111B: suzaku WAM observation of the prompt emission.. GRB Coordinates Network. 4571. 1.
20.
Onda, K., M. Tashiro, M. Suzuki, et al.. (2006). GRB 061202: suzaku WAM observation of the prompt emission.. GRB Coordinates Network. 5907. 1.1 indexed citations
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.