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Control of XIST Expression by MeCP2 and HDAC

  • Park, Jee-Hye;Kang, Yoon-Sung;Son, Jin-Sook;Min, Na-Young;Park, Young-Hoon;Lee, Kwang-Ho
    • 한국동물학회:학술대회논문집
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    • 한국동물학회 2003년도 한국생물과학협회 학술발표대회
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    • pp.204.4-204
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    • 2003

  • No Abstract, See Full Text

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Conceptual Design of the NISS onboard NEXTSat-1

  • Jeong, Woong-Seob;Park, Sung-Joon;Park, Kwijong;Lee, Dae-Hee;Pyo, Jeonghyun;Moon, Bongkon;Park, Youngsik;Kim, Il-Joong;Park, Won-Kee;Lee, Duk-Hang;Park, Chan;Ko, Kyeongyeon;Matsumoto, Toshio;Takeyama, Norihide;Enokuchi, Akito;Shin, Goo-Whan;Chae, Jangsoo;Nam, Uk-Won
    • Journal of Astronomy and Space Sciences
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    • 제31권1호
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    • pp.83-90
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    • 2014

  • The NISS onboard NEXTSat-1 is being developed by Korea astronomy and space science institute (KASI). For the study of the cosmic star formation history, the NISS performs the imaging spectroscopic observation in the near-infrared range for nearby galaxies, low background regions, star-forming regions and so on. It is designed to cover a wide field of view ($2{\times}2$ deg) and a wide wavelength range from 0.95 to $3.8{\mu}m$ by using linear variable filters. In order to reduce the thermal noise, the telescope and the infrared sensor are cooled down to 200 K and 80 K, respectively. Evading a stray light outside the field of view and making the most use of limited space, the NISS adopts the off-axis reflective optical system. The primary and the secondary mirrors, the opto-mechanical part and the mechanical structure are designed to be made of aluminum material. It reduces the degradation of optical performance due to a thermal variation. This paper presents the study on the conceptual design of the NISS.

  • https://doi.org/10.5140/JASS.2014.31.1.83 인용 PDF KSCI