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Institute for Astrophysics, Project Research Institutes Comprehensive Research Organization, Waseda University, 3-4-1 Okubo, Shinjuku-ku, Tokyo 169-8555, Japan
Department of Science, School of Education, Waseda University, Shinjuku-ku, Tokyo, Japan.
Department of Science, School of Education, Waseda University, 1-6-1 Nishi-Waseda, Shinjuku-ku, Tokyo 169-8050, Japan
Department of Science, School of Education, Waseda University, 1-6-1 Nishi-waseda, Shinjuku-ku, Tokyo 169-8050 of Science, School of Education, Waseda University, Tokyo, Japan.
Institute for Astrophysic; and Project Research Institutes, Comprehensive Research Organization, Waseda University, Shinjuku-ku, Tokyo, Japa; Institute for Astrophysic; and Department of Pure and Applied Physics, Graduate School of Science and Engineering, Waseda University, Shinjuku-ku, Tokyo, Japan; Department of Science, School of Education, Waseda University, Shinjuku-ku, Tokyo, Japan.
Institute for Astrophysics, Project Research Institutes, Comprehensive Research Organization, Waseda University, 3-4-1 Okubo, Shinjuku-ku, Tokyo 169-8555, Japan
Institute for Astrophysics, Project Research Institutes, Comprehensive Research Organization, Waseda University, Shinjuku-ku, Tokyo, Japan
Waseda University, Shinjyuku-ku, Tokyo, Japan
Tokyo University
Tokyo, University, Tokyo, Japan
Kuki High School, Kuki City, Saitama, Japan.
Institute for Astrophysics, Comprehensive Research Organization, Waseda University, 1-6-1 Nishi-Waseda, Shinjuku-ku, Tokyo 169-8050, Japan
Department of Science, School of Education, Waseda University, 1-6-1 Nishi-Waseda, Shinjyuku-ku, Tokyo 169-8050, Japan
Department of Science, School of Education, Waseda University, 1-6-1 Nishi-Waseda, Shinjuku-ku, Tokyo 169-8050
Waseda University, Tokyo, Japan
Astrophysics, Department of Science, School of Education, Waseda University, 1-6-1 Nishi-Waseda, Shinjuku-ku, Tokyo 169-8050
Department of Science School of Education, Waseda University, 1-6-1, Nishi-Waseda, S
A 3 Jy Radio Burst at a High Galactic Latitude
A Bursting Transient Was Detected At High Galactic Latitude In Waseda Nasu Pulsar Observatory
A design for digital signal processing in a large field radio patrol camera
A high-speed parallel FFT-processor for a radio astronomy telescope
A Strong Radio Transient at High Galactic Latitude
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