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Performance evaluation of an SOI pixel sensor with in-pixel binary counters

Radiation Detection Technology and Methods 2018年第1期2卷 80-86页

作者： Longlong Song Yunpeng Lu ryo hashimoto Ryutaro Nishimura Shunji Kishimoto Yang Zhou Zhigang Wu Yasuo Arai Qun Ouyang State Key Laboratory of Particle Detection and Electronics(Institute of High Energy Physics CAS)Beijing 100049China University of Chinese Academy of Sciences Beijing 100049China Institute of Materials Structure Science KEK1-1 OhoTsukubaIbaraki 305-0801Japan School of High Energy Accelerator Science SOKENDAI1-1 OhoTsukubaIbaraki 305-0801Japan Institute of Particle and Nuclear Studies KEK1-1 OhoTsukubaIbaraki 305-0801Japan

Introduction Pixel detectors fabricated with the silicon-on-insulator(SOI)technology suffered from the digital pickup,due to the capacitive coupling between the sensing electrode and the in-pixel *** order to tackle this issue,an advanced process called double SOI has been developed.A prototype chip CPIXTEG3b adopting this new process was designed and *** optimization concerning the double-SOI design and testing of the single pixel were already presented in a separate publication,this paper focuses on its noise performance of the full matrix and X-ray detection utilizing a synchrotron photon *** Equivalent noise charge(ENC)of the full pixel matrix was measured with electrical pulse *** threshold dispersion was minimized by the DAC tuning in each individual *** a photon-counting X-ray imager,noise count accumulated up to 1 h was *** efficiency was measured with a micro-focused beam as well as a flat field generated by the X-ray scattering on a glassy carbon at the KEK PF beam line *** The typical ENC is 52 e−and the sigma of threshold dispersion is 10 e−over the full matrix.A merit of“zero”noise count is also demonstrated,which is consistent with the low *** prototype chip has been tested with microbeam and used to measure the beam profile to be with a full width of 50µm at 2.4%of the maximum *** sensor depletion and charge sharing between neighboring pixels have been carefully characterized,providing insights for further *** homogeneity of response to X-ray photons has been demonstrated in the flat field *** work has drawn a final conclusion to the solution of digital pickup issue and opened a promising prospect in low-noise and high-resolution X-ray imaging.

关键词： Double SOI X-ray imaging detectors Photon counting Pixel detector

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Magnetic Resonance Imaging Characteristics of Tumefactive Demyelinating Lesions

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Journal of Biomedical Science and Engineering 2015年第5期8卷 321-326页

作者： Jiro Akimoto Tomohiro Suda ryo hashimoto Hirokazu Fukuhara Michihiro Kohno Department of Neurosurgery Tokyo Medical University Tokyo Japan

Tumefactive demyelinating lesions (TDLs) are often misdiagnosed as brain tumors. To identify imaging characteristics of TDLs for their proper diagnosis, their differences from malignant gliomas, etc., were investigated based on 3-Tesla magnetic resonance imaging (MRI) and MR spectroscopy data that was obtained from 5 patients diagnosed with TDLs in our hospital. MfRI displayed a paraventricular lesion with a maximum diameter of ≥2 cm. Diffusion-weighted imaging (DWI) displayed a region of bright signal intensity at the margin of the lesion, and apparent diffusion coefficient (ADC) imaging displayed high signal intensity at the core of the lesion. The mass effect was mild relative to the size of the lesion, and the edema around the lesion was mild to moderate. Gadolinium-enhanced MRI displayed a characteristic open-ring sign, in which the ring of enhancement was incomplete (open towards the cortex), with the medullary vein running through the lesion, resulting in the enhancement of the surrounding area. MR spectroscopy displayed an increase in the choline peak, a decrease in the N-acetyl aspartate (NAA) peak, the presence of lactate/lipid peaks, and the presence of β, γ-glutamate-glutamine (GLX) peaks that are slightly shifted to a higher resonance frequency (2.1 - 2.4 ppm) from the NAA peak. Taken together, the following main characteristics were identified as imaging features of TDLs: bright rim on DWI, a high signal core on ADC imaging, an open-ring sign, and β, γ-GLX peaks on proton MR spectroscopy. We concluded that the key to the improvement of neurological symptoms of patients is the prompt initiation of steroid treatment following the accurate diagnosis of TDLs.

关键词： Tumefactive Demyelinating Lesions Open-Ring Sign MRI MR Spectroscopy

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The Relationship between Neck and Shoulder Pain and the Sagittal Alignment of the Spine in Standing in Younger Generation

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Open Journal of Orthopedics 2015年第11期5卷 337-344页

作者： Tomonori Kenmoku Takane Suzuki Nobuyasu Ochiai Tatsuki Ebata Genyo Miyajima Naoshige Nagura Mitsufumi Nakawaki ryo Tazawa Sho Hiramatsu Hironori Yamazaki Yu Sasaki Takeshi Yamaguchi Eiko hashimoto Kenji Onuma Naonobu Takahira Kazuhisa Takahashi Masashi Takaso Department of Orthopedic Surgery Kitasato University School of Medicine Sagamihara Japan Sakura Orthopaedic Hospital Sakura Japan Department of Bioenvironmental Medicine Graduate School of Medicine Chiba Japan Department of Orthopaedic Surgery Chiba University Graduate School of Medicine Chiba Japan Department of Orthopedic Surgery Kitasato Medical Center Kitamoto Japan School of Allied Health Science Kitasato University Sagamihara Japan

Background: The relationship between chronic neck and shoulder pain and posture remains controversial. The purpose of this study was to investigate the relationship between chronic neck and shoulder pain and spinal sagittal alignment in standing posture in younger generation. Methods: Subjects included 57 females and 32 males (average age, 29.9 ± 5.7 years). All subjects were 20s or 30s. Spinal curvature was assessed using SpinalMouse. The subjects were also divided into a normal group (VAS zero group) and a pain group by VAS results. Statistical analysis was performed by Student’s t-test. Significance was defined as p < 0.05. Results: The normal group and pain group included 29 and 60 subjects, respectively. In terms of location of pain, thirty-one subjects felt neck pain, 50 felt pain above the scapula, and 17 felt pain between the thoracic spine and scapula. Thoracic kyphosis and lumbar lordosis in the pain group were significantly higher than those in the normal group (p = 0.013 and p = 0.020, respectively). Thoracic kyphosis in subjects with neck pain or pain above scapula was significantly higher than that in subjects without pain (p = 0.0075 and p = 0.025, respectively). Lumbar lordosis in subjects with pain above the scapula or interscapula was significantly higher than that in subjects without pain (p = 0.016).

关键词： Choronic Neck and Shoulder Pain Sagittal Alignment of the Spine Thoracic Kyphosis Lumber Lordosis

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Near-infrared polarimetry of the GG Tauri A binary system

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Research in Astronomy and Astrophysics 2014年第11期14卷 1438-1446页

作者： Yoichi Itoh Yumiko Oasa Tomoyuki Kudo Nobuhiko Kusakabe Jun hashimoto Lyu Abe Wolfgang Brandner Timothy D.Brandt Joseph C.Carson Sebastian Egner Markus Feldt Carol A.Grady Olivier Guyon Yutaka Hayano Masahiko Hayashi Saeko S.Hayashi Thomas Henning Klaus W.Hodapp Miki Ishii Masanori Iye Markus Janson ryo Kandori Gillian R.Knapp Masayuki Kuzuhara Jungmi Kwon Taro Matsuo Michael W.McElwain Shoken Miyama Jun-Ichi Morino Amaya Moro-Martin Tetsuo Nishimura Tae-Soo Pyo Eugene Serabyn Takuya Suenaga Hiroshi Suto Ryuji Suzuki Yasuhiro H.Takahashi Naruhisa Takato Hiroshi Terada Christian Thalmann Daigo Tomono Edwin L.Turner Makoto Watanabe John Wisniewski Toru Yamada Satoshi Mayama Thayne Currie Hideki Takami Tomonori Usuda Motohide Tamura Nishi-Harima Astronomical Observatory Center for AstronomyUniversity of Hyogo407-2NishigaichiSayoHyogo 679-5313Japan Faculty of Education Saitama University255 Shimo-OkuboSakuraSaitamaSaitama338-8570Japan Subaru Telescope National Astronomical Observatory of Japan650 North Ahoku PlaceHiloHI 96720USA National Astronomical Observatory of Japan 2-21-1OsawaMitakaTokyo181-8588Japan H.L.Dodge Department of Physics & Astronomy University of Oklahoma440 W Brooks St.NormanOK 73019USA Laboratoire Lagrange (UMR 7293) Universit de Nice-Sophia AntipolisCNRSObservatoire de la Cote d’Azur28 avenue Valrose06108 Nice Cedex 2France Max Planck Institute for Astronomy Knigstuhl 1769117 HeidelbergGermany Department of Astrophysical Science Princeton UniversityPeyton HallIvy LanePrincetonNJ 08544USA Department of Physics and Astronomy College of Charleston58 Coming St.CharlestonSC29424USA Subaru Telescope National Astronomical Observatory of Japan650 North A’ohoku PlaceHiloHI 96720USA Exoplanets and Stellar Astrophysics Laboratory Code 667Goddard Space Flight CenterGreenbeltMD 20771USA Eureka Scientific 2452 DelmerSuite 100Oakland CA 96002USA Goddard Center for Astrobiology GreenbeltMD 20771USA Institute for Astronomy University of Hawaii640 N.Aohoku PlaceHiloHI 96720USA Department of Earth and Planetary Sciences Tokyo Institute of TechnologyOokayamaMeguro-kuTokyo 152-8551Japan Department of Astronomy Kyoto UniversityKitashirakawa-Oiwake-choSakyo-kuKyotoKyoto 606-8502Japan Hiroshima University 1-3-2KagamiyamaHigashihiroshimaHiroshima 739-8511Japan Department of Astrophysics CAB-CSIC/INTA28850 Torrejón de ArdozMadridSpain Jet Propulsion Laboratory California Institute of TechnologyPasadenaCA91109USA Department of Astronomical Science The Graduate University for Advanced Studies2-21-1OsawaMitakaTokyo181-8588Japan Department of Astronomy The University of Tokyo7-3-1HongoBunkyo-kuTokyo113-0033Japan Astronomical Institute "Anton Pannekoek" University

A high angular resolution near-infrared image that shows the intensity of polarization for the GG Tau A binary system was obtained with the Subaru Telescope. The image shows a circumbinary disk scattering the light from the central binary. The azimuthal profile of the intensity of polarization for the circumbinary disk is roughly reproduced by a simple disk model with the Henyey-Greenstein phase function and the Rayleigh function, indicating there are small dust grains at the surface of the disk. Combined with a previous observation of the circumbinary disk, our image indicates that the gap structure in the circumbinary disk orbits counterclockwise, but material in the disk orbits clockwise. We propose that there is a shadow caused by material located between the central binary and the circumbinary disk. The separations and position angles of the stellar components of the binary in the past 20 yr are consistent with the binary orbit with a = 33.4 AU and e = 0.34.

关键词： stars individual (GG Tauri) -- stars pre-maln sequence - techniques high angular resolution

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