H. Ishino
Okayama University
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Publication
Featured researches published by H. Ishino.
ieee nuclear science symposium | 2000
M. Yokoyama; H. Aihara; M. Hazumi; H. Ishino; J. Kaneko; Y. Li; D. Marlow; S. Mikkelsen; E. Nygard; H. Tajima; J. Talebi; G. Varner; H. Yamamoto
We have studied the radiation hardness of the VA1, a Viking-architecture preamplifier VLSI chip. Large-scale integrated (LSI) samples are fabricated in 0.8 and 0.35 /spl mu/m process technologies to improve the radiation hardness of the LSI for the Belle silicon vertex detector upgrade. We have observed significant improvement of the radiation hardness with 0.8-/spl mu/m technology compared to 1.2-/spl mu/m technology. Little degradation of noise and gain is observed up to a total dose of 20 Mrd for the VA1 fabricated in the 0.35-/spl mu/m technology. We find that the radiation hardness improves with a scaling of better than t/sub ox//sup -6/ (t/sub ox/: oxide thickness). Basic parameters of MOSFETs are also studied to understand the mechanism of radiation damage in the VA1.
Applied Optics | 2016
Tomotake Matsumura; Karl Young; Qi Wen; Shaul Hanany; H. Ishino; Y. Inoue; M. Hazumi; Jürgen Koch; Oliver Suttman; Viktor Schütz
We report on the first use of laser ablation to make submillimeter, broadband, antireflection coatings (ARCs) based on subwavelength structures (SWSs) on alumina and sapphire. We used a 515 nm laser to produce pyramid-shaped structures with a pitch of about 320 μm and a total height of near 800 μm. Transmission measurements between 70 and 140 GHz are in agreement with simulations using electromagnetic propagation software. The simulations indicate that SWS-ARCs with the fabricated shape should have a fractional bandwidth response of Δν/νcenter=0.55 centered on 235 GHz for which reflections are below 3%. Extension of the bandwidth to both lower and higher frequencies, between a few tens of gigahertz and a few terahertz, should be straightforward with appropriate adjustment of laser ablation parameters.
Journal of Cosmology and Astroparticle Physics | 2017
Duc Thuong Hoang; Guillaume Patanchon; M. Bucher; Tomotake Matsumura; Ranajoy Banerji; H. Ishino; M. Hazumi; Jacques Delabrouille
Future Cosmic Microwave Background (CMB) satellite missions aim to use the
ieee nuclear science symposium | 2000
J. Kaneko; H. Aihara; G. Alimonti; H. Hazumi; H. Ishino; Y. Li; K. Sumisawa; H. Tajima; J. Tanaka; G. N. Taylor; H. Yamamoto; M. Yokoyama; G. Varner
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ieee nuclear science symposium | 2000
H. Aihara; M. Hazumi; H. Ishino; J. Kaneko; Y. Li; D. Marlow; S. Mikkelsen; D. Nguyen; E. Nygaard; H. Tajima; J. Talebi; G. Varner; H. Yamamoto; M. Yokoyama
mode polarization to measure the tensor-to-scalar ratio
Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy IX | 2018
Tomotake Matsumura; Yuki Sakurai; Nobuhiko Katayama; Hajime Sugai; Hiroaki Imada; H. Ishino; M. Hazumi; Ryota Takaku; K. Komatsu
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Journal of Low Temperature Physics | 2018
Y. Yamada; H. Ishino; A. Kibayashi; Y. Kida; N. Hidehira; K. Komatsu; M. Hazumi; Nobuaki Sato; K. Sakai; Hirotake Yamamori; F. Hirayama; Satoshi Kohjiro
with a sensitivity of about
instrumentation and measurement technology conference | 2015
A. Kibayashi; H. Ishino; Yosuke Yamada; akinori Okamoto; Y. Kida; Masashi Hazumi; Nobuaki Sato; Hiroki Watanabe
10^{-3}
Proceedings of Technology and Instrumentation in Particle Physics 2014 — PoS(TIPP2014) | 2015
H. Ishino; A. Kibayashi; Y. Kibe; Y. Yamada; akinori Okamoto; Y. Kida; M. Hazumi; Nobuaki Sato; H. Watanabe
. Achieving this goal will not only require sufficient detector array sensitivity but also unprecedented control of all systematic errors inherent to CMB polarization measurements. Since polarization measurements derive from differences between observations at different times and from different sensors, detector response mismatches introduce leakages from intensity to polarization and thus lead to a spurious
Proceedings of the 12th Asia Pacific Physics Conference (APPC12) | 2014
H. Ishino
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