• Proceedings of the Korea Information Processing Society Conference
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• 2011.04a
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• pp.451-454
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• 2011

COSMOS (COntentS Making Omnipotent System)는 컴퓨터 게임이나 3차원 애니메이션 제작이 가능하도록 그래픽 랜더링, 특수효과, 물리엔진, 인공지능 엔진 등의 기능을 갖춘 범용성 3차원 콘텐츠 저작 시스템이며, 무엇보다도 직관적인 인터페이스 기능을 통해 사용자의 편리성을 제공해 준다. 본 논문은 COSMOS에서 음향 정보를 자동으로 3D 콘텐츠 구성 요소에 배합될 수 있도록 하는 기술에 대한 내용이다. 본 기술의 도입을 통해 COSMOS에서는 사용자의 의성어 소리를 인식하여, 그 의미에 적합한 디지털 사운드를 검색한 후에 사용자의 의도에 맞추어 변환하여 이와 관련된 콘텐츠 구성 요소와 일치 시켜줌으로써 보다 직관적으로 콘텐츠 저작 기능을 제공할 수 있다.

• The Bulletin of The Korean Astronomical Society
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• v.44 no.2
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• pp.58.1-58.1
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• 2019

We have developed Ground Software (GSW) of BITSE. The ground software includes mission operation software, data visualization software and data processing software. Mission operation software is implemented using COSMOS. COSMOS is a command and control system providing commanding, scripting and data visualization capabilities for embedded systems. Mission operation software send commands to flight software and control coronagraph. It displays every telemetry packets and provides realtime graphing of telemetry data. Data visualization software is used to display and analyze science image data in real time. It is graphical user interface (GUI) and has various functions such as directory listing, image display, and intensity profile. The data visualization software shows also image information which is FITS header, pixel resolution, and histogram. It helps users to confirm alignment and exposure time during the mission. Data processing software creates 4-channel polarization data from raw data.

• The Bulletin of The Korean Astronomical Society
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• v.46 no.2
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• pp.43.1-43.1
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• 2021

Using 74 galaxy clusters in the COSMOS field at 0.1 < z < 1.2, we calculate the environmental quenching timescale, defined as the time required after a galaxy is accreted by a cluster for it to stop star formation. Cluster candidates are selected as the overdensities with the surface number density exceeding the 4-σ. With the "delayed-then-rapid" quenching model, we can successfully reproduce the separation of the galaxies(star-forming, intermediate, and quiescent) on the NUV-R - R-J color plane comparing with the BC03 evolutionary track. With the mass growth rate of halo mass and the ratio of categorized galaxies, we can constratin the environmental quenching timescale ~ 2Gyr at z ~ 1. We will present the result as a function of redshift and compare them with dynamical timescale and gas depletion timescale.

• The Bulletin of The Korean Astronomical Society
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• v.46 no.1
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• pp.52.3-53
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• 2021

It is yet to be understood what controls the star formation activity in high-redshift galaxy clusters. One recently proposed mechanism is that the star formation activity in galaxy clusters are fed by gas and galaxies in large-scale structures surrounding them, which we call as "web feeding model". Using galaxies in the COSMOS2015 catalog, with mass completeness at log(M/M_⦿)≥9.54 and reliable photometric redshift data (σ_Δz/(1+z) ≲ 0.01), we study the star formation activities of galaxy clusters and their surrounding environment to test the web feeding model. We first identify the overdense regions with number density exceeding the 4σ-level from photometric redshift data as galaxy clusters, and we find that they are well matched with clusters identified in the X-ray extended source catalog. Furthermore, we identify galaxy large scale structures, and will present the correlation or anti-correlation between quiescent galaxy fraction, an indicator of star-forming activity, and the prevalence of galaxy large scale structures.

• The Bulletin of The Korean Astronomical Society
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• v.32 no.2
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• pp.76.1-76.1
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• 2007

• Bulletin of the Korean Space Science Society
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• 2006.04a
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• pp.28-28
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• 2006

• Bulletin of the Korean Space Science Society
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• 2006.04a
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• pp.62-62
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• 2006

• 한국ITS학회:학술대회논문집
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• 2002.11a
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• pp.14-17
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• 2002

• Proceedings of the Zoological Society Korea Conference
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• 1997.10b
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• pp.320.1-320
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• 1997

• 한국ITS학회:학술대회논문집
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• 2004.11a
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• pp.186-191
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• 2004