• 제목/요약/키워드: Space Program

검색결과 2,840건 처리시간 0.027초

GECKO Optical Follow-up Observation of Three Binary Black Hole Merger Events

  • Kim, Joonho;Im, Myungshin;Paek, Gregory S.H.;Lee, Chung-Uk;Kim, Seung-Lee;Chang, Seo-Won;Choi, Changsu;Hwang, Sungyong;Kang, Wonseok;Kim, Sophia;Kim, Taewoo;Lee, Hyung Mok;Lim, Gu;Seo, Jinguk;Sung, Hyun-Il
    • 천문학회보
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    • 제46권1호
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    • pp.53.3-54
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    • 2021
  • We present optical follow-up observation results of three binary black hole merger (BBH) events, GW190408 181802, GW190412, and GW190503 185404, which were detected by the Advanced Ligo and Virgo gravitational wave (GW) detectors. Electromagnetic (EM) counterparts are generally not expected for BBH merger events, however, some theoretical models suggest that EM counterparts of BBH can possibly arise in special environments. To identify EM counterparts of the three BBH merger events, we observed high-credibility regions of the sky with telescopes of the Gravitational-wave EM Counterpart Korean Observatory (GECKO), including the Korea Microlensing Telescope Network (KMTNet). Our observation started as soon as 100 minutes after the GW event alert and covered roughly 29 - 63 deg2 for each event with a depth of 22.5 mag in R-band within hours of observation. No plausible EM counterparts were found for these events. Our result gives a great promise for the GECKO facilities to find EM counterparts within few hours from GW detection in future GW observation runs.

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고등학교 공용공간의 패러다임 변화 분석 - 우수시설학교로 지정된 고등학교를 중심으로 - (A Study on the Analysis of Paradigm Change in Common Space of High School - Focused on High Schools selected as Excellent School Facilities -)

  • 신지은;황희준
    • 교육시설 논문지
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    • 제24권6호
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    • pp.55-64
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    • 2017
  • This study analyzes the common space of the high schools before and after the decade of 2009 which starts Subject-centered clusters school plan, and proposes the direction of common space planning for the future. Based on the floor plans of high schools awarded as excellent school facilities every year, first, types and numbers of common space, second, area ratio between common space and program space and also moving space and staying space, third, space connections were analyzed for tracking the change of the relationship between common, staying and program spaces. The study results demonstrated that types, numbers and area ratio of the common space were increased as the years go on. Especially, the area ratio of staying space was dramatically increased after 2009 and this result was caused by the home-base, alcove space, and hall that were adopted for subject-centered clusters planning after 2009. Connecting diagram of staying area and program spaces also shows the spaces related to staying area were changed from a classrooms and administrative office etc. to a library, gym, and seminar rooms etc. In case of staying area, it would have a value as a common space for various student activities such as group activities, meetings, and multi-uses. Because student activities would be changed and encouraged depending on the location, sizes and program spaces around staying area, it should be emphasized that the planning for staying area is critical for future school design.

Intensive Monitoring Survey of Nearby Galaxies: Current Status

  • Im, Myungshin;Choi, Changsu;Lim, Gu;Kim, Sophia;Paek, Seunghak Gregory;Kim, Joonho;Hwang, Sungyong;Shin, Suhyung;Baek, Insu;Lee, Sangyun;O, Sung A;Yoon, Sung Chul;Sung, Hyun-Il;Jeon, Yeong-Beaom;Lee, Sang Gak;Kang, Wonseok;Kim, Tae-Woo;Kwon, Sun-gil;Pak, Soojong;Eghamberdiev, Shuhrat
    • 천문학회보
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    • 제43권1호
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    • pp.64.1-64.1
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    • 2018
  • SNe light curves have been used to understand the expansion history of the universe, and a lot of efforts have gone into understanding the overall shape of the radioactively powered light curve. However, we still have little direct observational evidence for the theorized SN progenitor systems. Recent studies suggest that the light curve of a supernova shortly after its explosion (< 1 day) contains valuable information about its progenitor system and can be used to set a limit on the progenitor size, R*. In order to catch the early light curve of SNe explosion and understand SNe progenitors, we are performing a ~8hr interval monitoring survey of nearby galaxies (d < 50 Mpc) with 1-m class telescopes around the world. Through this survey, we expect to catch the very early precursor emission as faint as R=21 mag (~0.1 Rsun for the progenitor). In this poster, we outline this project, and present a few scientific highlights, such as the early light curve of SN 2015F in NGC 2442.

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후기구조주의적 사유체계로서의 관계성에 기초한 현대건축공간의 비결정적 프로그램의 특성에 관한 연구 (A Study on the Characteristics of Indeterminate Program based on the Philosophical Concept of Relationship in Post Structuralism)

  • 김윤정;박관일
    • 한국실내디자인학회논문집
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    • 제14권6호
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    • pp.37-46
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    • 2005
  • This study is focused on the indeterminacy of the contemporary social structure based on the philosophical concept of relationship. The purpose of this study is to present the index of the space planning that the contemporary society demands through analysis of a characteristics of the indeterminate program. As the result, we got a characteristic and a design method of the following indeterminate programs. (1)The characteristic of the interior space programs are in such cases as combined, the continuance, the pile, the juxtaposition, mixing and interference etc. (2) The characteristics of space planning are multiple changes of the space occupation, various sight experiences, folding structure, expansion of flow space, the insertion of a between spates etc. (3) The characteristic of space design expression is addition of various functions tv unification of a structural element and an element of furniture.

Optical/NIR Follow-up Observation of GW Sources

  • Im, Myungshin;Lee, Hyung Mok;Choi, Changsu;Kim, Joonho;Gu, Lim;Sung, Hyun-Il;Jeon, Yeong-Beom;Kim, Seung-Li;Lee, Chung-Uk;Pak, Soojong;Eghamberdiev, Shuhrat
    • 천문학회보
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    • 제42권2호
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    • pp.52.3-53
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    • 2017
  • Identification of gravitational wave (GW) sources in electromagnetic (EM) wave observations is important because it enables us to understand the property of the GW-emitting sources/mechanisms much better than the GW detection. For that reason, a large number of astronomers are working on observations to identify the position and the nature of GW sources. We give a short overview of the expected EM signals from GW sources and the current EM follow-up observations that have been undertaken in Korea and the world.

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All-Sky Distribution of the Zodiacal Thermal Emission

  • Kwon, S.M.;Hong, S.S.;Weinberg, J.L.;Lee, C.
    • 한국우주과학회:학술대회논문집(한국우주과학회보)
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    • 한국우주과학회 2000년도 한국우주과학회보 제9권2호
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    • pp.48-48
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    • 2000
  • No Abstract, See Full Text

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우주발사 시스템 개발을 위한 통합 기술관리 시스템 소개 (Introduction of Program Life-Cycle Management System for Space Launch System Development)

  • 조미옥;조철훈;이준호;오범석;박정주;조광래
    • 시스템엔지니어링워크숍
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    • 통권4호
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    • pp.86-89
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    • 2004
  • A web-based program life-cycle management(PLM) system is introduced to implement the system engineering processes and to provide the development teaceability online. This information system aims for the realization of essential system engineering management techniques currently applied to the space launch system development program including management of configuration and data based on the work breakdown structure(WBS), WBS, bill of materials and properties. The system enhances communication and gives access to the development data with relevant information such as data-to-data relation and approval status/history through the web, and preserve all of the development data throughout the program life-cycle. Further improvement of the system is planned to implement the program managrment pricesses and to provide integrated information useful for the programmatic decision making.

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우주 발사 시스템 개발을 위한 통합 기술관리 시스템 소개 (Introduction of Program Life-Cycle Management System for Space Launch System Development)

  • 조미옥;신명호
    • 시스템엔지니어링학술지
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    • 제2권1호
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    • pp.48-53
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    • 2006
  • A web-based program life-cycle management(PLM) system is introduced to implement the system engineering processes and to provide the development traceability online. This information system aims for the realization of essential system engineering management techniques currently applied to the space launch system development program including management of configuration and data based on the work breakdown structure(WBS), WBS, bill of materials and mass properties. The system enhances communication and gives access to the development data with relevant information such as data-to-data relation and approval status/history through the web, and preserve all of the development data throughout the program life-cycle. Further improvement of the system is planned to implement the program management processes and co provide integrated information useful for the programmatic decision making.

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