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The Introduction of Adverse Drug Reaction (ADR) Monitoring System

  • Jung, Sun-Hoi;Park, Kyoung-Ho;Soh, Ok-Kyoung;Lee, Byung-Gu;Park, Kaung-Jun;Bae, Guen-Shub;Jang, In-Jin;Kim, Youn-Gun;Kim, Ju-Sung;Chae, In-Ho;Kim, Yeun-Su;Ha, Jong-Won;Song, Yong-Sung;Choung, Jon-Ho;Kyun, Jin-Soo;Kim, Sang-Yeun;Go, Zae-Sung;Park, Jun-Dong;Song, Kyeng-Ja;Park, Byung-Joo
    • Proceedings of the PSK Conference
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    • 2001.10a
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    • pp.323-323
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    • 2001

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Gene Ontology Development and Implementation at the Saccharomyces Genome Database

  • Hong, E.L.;Weng, S.;Dolinski, K.;Balakrishnan, R.;Christie, K.R.;Costanzo, M.C.;Dwight, S.S.;Engel, S.R.;Fisk, D.G.;Hirschman, J.E.;Issel-Tarver, L.;Sethuraman, A.;Theesfeld, C.L.;Binkley, G.;Schroeder, M.;Dong, S.;Andrada, R.;Botstein, D.;Cherry, J.M.
    • Proceedings of the Korean Society for Applied Microbiology Conference
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    • 2003.06a
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    • pp.95-102
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    • 2003

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Neutron Beam Hardening with Heavy Water

  • Onizuka, Y.;Hoshi, M.;Takada, J.;Endo, S.;Uehara, S.;Takatsuji, T.;Utshumi, H.;Kobayashi, T.;Sakurai, Y.;Hayabuchi, N.;Yamaguchi, H.;Takada, M.;Fujikawa, K.;Maeda, N.
    • Proceedings of the Korean Society of Medical Physics Conference
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    • 1999.11a
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    • pp.342-344
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    • 1999

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Design and Construction of Detector Module for UFFO Burst Alert & Trigger Telescope

  • Jung, Aera;Ahmad, Salleh;Barrillon, Pierre;Brandt, Soren;Budtz-Jorgensen, Carl;Castro-Tirado, Alberto J.;Chen, Pisin;Choi, Ji Nyeong;Choi, Yeon Ju;Connell, Paul;Dagoret-Campagne, Sylvie;Eyles, Christopher;Grossan, Bruce;Huang, Ming-Huey A.;Jeong, Soomin;Kim, Ji Eun;Kim, Min Bin;Kim, Sug-Whan;Kim, Ye Won;Krasnov, A.S.;Lee, Jik;Lim, Heuijin;Linder, Eric V.;Liu, T.C.;Lund, Niels;Min, Kyung Wook;Na, Go Woon;Nam, Ji Woo;Panasyuk, Mikhile I.;Park, Il Hung;Ripa, Jakub.;Reglero, Victor;Rodrigo, Juana M.;Smoot, George.F.;Suh, Jung Eun;Svertilov, Sergei.;Vedenkin, Nikolay;Wang, Min-Zu;Yashin, Ivan
    • The Bulletin of The Korean Astronomical Society
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    • v.37 no.2
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    • pp.207.1-207.1
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    • 2012

  • One of the key aspects of the upcoming Ultra-Fast Observatory (UFFO) Pathfinder for Gamma-Ray Bursts(GRBs) identification will be the UFFO Burst Alert & Trigger Telescope(UBAT), based on a novel space telescope technique. The UBAT consists of coded mask, hopper, and detector module(DM). The UBAT DM consists of YSO crystal arrays, multi-anode photo mulipliers, and readout electronics. We will present the design and construction of the UBAT DM, and the response of the UBAT DM to X-ray sources.

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miniTAO/ANIR Paα SURVEY OF LOCAL LIRGs

  • Tateuchi, Ken;Motohara, Kentaro;Konishi, Masahiro;Takahashi, Hidenori;Kato, Natsuko;Uchimoto, Yuka K.;Toshikawa, Koji;Ohsawa, Ryou;Kitagawa, Yutaro;Yoshii, Yuzuru;Doi, Mamoru;Kohno, Kotaro;Kawara, Kimiaki;Tanaka, Masuo;Miyata, Takashi;Tanabe, Toshihiko;Minezaki, Takeo;Sako, Shigeyuki;Morokuma, Tomoki;Tamura, Yoichi;Aoki, Tsutomu;Soyano, Takeo;Tarusawa, Kenfichi;Koshida, Shintaro;Kamizuka, Takafumi;Nakamura, Tomohiko;Asano, Kentaro;Uchiyama, Mizuho;Okada, Kazushi;Ita, Yoshifusa
    • Publications of The Korean Astronomical Society
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    • v.27 no.4
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    • pp.297-298
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    • 2012

  • ANIR (Atacama Near InfraRed camera) is a near infrared camera for the University of Tokyo Atacama 1m telescope, installed at the summit of Co. Chajnantor (5,640 m altitude) in northern Chile. The high altitude and extremely low water vapor (PWV = 0.5 mm) of the site enable us to perform observation of hydrogen $Pa{\alpha}$ emission line at $1.8751{\mu}m$. Since its first light observation in June 2009, we have been carrying out a $Pa{\alpha}$ narrow-band imaging survey of nearby luminous infrared galaxies (LIRGs), and have obtained $Pa{\alpha}$ for 38 nearby LIRGs listed in AKARI/FIS-PSC at the velocity of recession between 2,800 km/s and 8,100 km/s. LIRGs are affected by a large amount of dust extinction ($A_V$~ 3 mag), produced by their active star formation activities. Because $Pa{\alpha}$ is the strongest hydrogen recombination line in the infrared wavelength ranges, it is a good and direct tracer of dust-enshrouded star forming regions, and enables us to probe the star formation activities in LIRGs. We find that LIRGs have two star-forming modes. The origin of the two modes probably come from differences between merging stage and/or star-forming process.

  • https://doi.org/10.5303/PKAS.2012.27.4.297 인용 PDF KSCI