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个人简介
Sho Masui received the B.S. and M.S. degrees in physics from Osaka Prefecture University, Osaka, Japan, in 2018 and 2020, respectively. He is currently working on the development of wideband heterodyne receiver system for next-generation radio telescope toward the Ph.D. degree with Osaka Metropolitan University, Osaka, Japan.
From 2017 to 2021, he developed a wideband heterodyne receiver system for an Osaka 1.85 m millimeter–submillimeter telescope. From 2021 to 2022, he joined the National Astronomical Observatory of Japan as a graduate student and has worked on the development of superconducting devices. His research interests include the design and measurement of wideband waveguide circuits and wideband and compact superconducting circuits.
研究兴趣
论文共 18 篇作者统计合作学者相似作者
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Kazunori Akiyama, Kotaro Niinuma, Kazuhiro Hada, Akihiro Doi, Yoshiaki Hagiwara, Aya E. Higuchi, Mareki Honma,Tomohisa Kawashima, Dimitar Kolev, Shoko Koyama,Sho Masui, Ken Ohsuga,
arxiv(2024)
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arxiv(2024)
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IEEE MICROWAVE AND WIRELESS TECHNOLOGY LETTERSno. 7 (2023): 1051-1054
IEEE Transactions on Applied Superconductivityno. 5 (2023): 1-4
Yasumasa Yamasaki,Yutaka Hasegawa,Sho Yoneyama,Sana Kawashita, Tsubasa Chinen,Sho Masui,Chiaki Nosohara, Heyang Sun, Shuto Dakie, Akira Kameyama, Ikko Fujitomo, Yuma Nishikawa,
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPANno. 3 (2023): 499-513
2022 ASIA-PACIFIC MICROWAVE CONFERENCE (APMC)pp.25-27, (2022)
Publications of the Astronomical Society of Japanno. 4 (2021): 1100-1115
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