• 천문학회지
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• 제38권4호
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• pp.463-470
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• 2005

In this paper, we have made the component-based development of observational software for KASI solar imaging spectrograph (KSIS) that is able to obtain three-dimensional imaging spectrograms by using a scanning mirror in front of the spectrograph slit. Since 2002, the KASI solar spectrograph has been successfully operated to observe solar spectra for a given slit region as well as to inspect the response functions of narrow band filters. To improve its capability, we have developed the KSIS that can perform sequential observations of solar spectra by simultaneously controlling the scanning mirror and the CCD camera via Visual C++. Main task of this paper is to introduce the development of the component-based software for KSIS. Each component of the software is reusable on the level of executable file instead of source code because the software was developed by using CBD (component-based development) methodology. The main advantage of such a component-based software is that key components such as image processing component and display component can be applied to other similar observational software without any modifications. Using this software, we have successfully obtained solar imaging spectra of an active region (AR 10708) including a small sunspot. Finally, we present solar $H{\alpha}$ spectra ($6562.81{\AA}$) that were obtained at an active region and a quiet region in order to confirm the validity of the developed KSIS and its software.

• 천문학논총
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• 제9권1호
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• pp.101-110
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• 1994

We have investigated intensively an optical telescope with 76cm diameter and CCD camera system in astronomical observatory of Kyung Hee university, in order to maximize instrumental functions of our observational equipments and to construct a more reliable photometric system. And computer softwares AUTO DOME, KH CCD and KH PHO for astronomical image observations and their automatic photometries with high accuracy have been made for observers w use our observational system conveniently and efficiently. Throughout careful examinations of these programs, it has been proved that the observing time by our program is shorter than that by manual operations, so that, fast and accurate observations can be executed with ease. For open cluster NGC 7063 observed with S/N value of 350 or more by KH PHO, we have found the magnitude measurements of 11 object stars would show 0.007 magnitude difference, comparing with magnitude data from IRAF/APPHOT. From automatic photometry of eclipsing binary, AB And observed by our software, total 220 data points with good quality have been acquired during 8 hours and so we could make a better light curve than that obtained from any observational results by domestic photoelectric photometry system.

• 천문학논총
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• 제10권1호
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• pp.135-146
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• 1995

We have developed a graphic software for image processing of astronomical data obtained by observational equipment in Astronomical Observatory of Kyung Hee University. The essential hardware for running our computer program is simply composed of a PC with the graphic card to handle 256 colors and the color graphic monitor, including CCD camera system. Our software has been programmed in WINDOWS to provide good environments for users, by using various techniques of image processing on astronomical image data recorded in FITS format by KHCCD program(Jin and Kim, 1994) with a compressional mode. We are convinced that our results will be a fundamental and useful technique in the construction of data processing system and can be effectively used in any other observatories, as well as in data processing system of Kyung Hee University.

• 대한원격탐사학회:학술대회논문집
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• 대한원격탐사학회 2002년도 Proceedings of International Symposium on Remote Sensing
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• pp.407-407
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• 2002

The most widespread techniques for DEM generation are stereoscopy for optical sensor images and interfereometry for SAR images. These techniques suffer from certain sensor and processing limitations, which can be overcome by the synergetic use of both sensors and DEMs respectively. In this paper, different strategies for fusing SAR and optical data are combined to derive high quality DEM products. The filtering techniques, which take advantage of the complementary properties of SAR and stereo optical DEMs, will be applied for the fusion process. By taking advantage of the fact that errors of the DEMs are of different nature using the filtering technique, affected part are filtered and replaced by those of the counterpart and is tested with two sets of SPOT and ERS DEM, resulting in a remarkable improvement in DEM. for the analysis of results, the reference DEM is generated from digital base map(1:5000).

• 대한공간정보학회지
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• 제10권5호
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• pp.53-65
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• 2002

The most widespread techniques for DEM generation are stereoscopy for optical sensor images and SAR interferometry(InSAR) for SAR images. These techniques suffer from certain sensor and processing limitations, which can be overcome by the synergetic use of both sensors and DEMs respectively. This study is associated with improvements of accuracy with consistency of image's characteristics between two different DEMs coming from stereoscopy for the optical images and interferometry for SAR images. The MWD(Multiresolution Wavelet Decomposition) and HPF(High-Pass Filtering), which take advantage of the complementary properties of SAR and stereo optical DEMs, will be applied for the fusion process. DEM fusion is tested with two sets of SPOT and ERS-l/-2 satellite imagery and for the analysis of results, DEM generated from digital topographic map(1 to 5000) is used. As a result of an integration of DEMs, it can more clearly portray topographic slopes and tilts when applying the strengths of DEM of SAR image to DEM of an optical satellite image and in the case of HPF, the resulting DEM.

• Journal of Preventive Medicine and Public Health
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• 제55권2호
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• pp.116-124
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• 2022

Epidemiological studies typically examine the causal effect of exposure on a health outcome. Standardization is one of the most straightforward methods for estimating causal estimands. However, compared to inverse probability weighting, there is a lack of user-centric explanations for implementing standardization to estimate causal estimands. This paper explains the standardization method using basic R functions only and how it is linked to the R package stdReg, which can be used to implement the same procedure. We provide a step-by-step tutorial for estimating causal risk differences, causal risk ratios, and causal odds ratios based on standardization. We also discuss how to carry out subgroup analysis in detail.

• 한국컴퓨터정보학회논문지
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• 제16권3호
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• pp.175-187
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• 2011

곤충 종은 환경생태학적 종 다양성 보존과 국가적 생물자원 활용전략 관점에서 중요한 역할을 하기 때문에 생태계의 주요 구성요소로 인식되고 있다. 곤충 종 보존과 육성을 위해서는 곤충전문가는 물론 곤충비전문가인 일반인과 학생들도 곤충에 관심을 가질 수 있는 곤충관찰학습 환경이 요구된다. 그러므로, 곤충식별은 관찰학습에 있어서 주요학습의 동기유발 요인이 된다. 현재 서비스하고 있는 온라인 곤충 종 분류검색시스템은 시간 소모적이며, 곤충 종에 대한 지식이 부족한 일반인들이 곤충식별의 도구로 사용하기에는 많은 노력을 요구하기 때문에 비효율적이다. 본 연구에서는 이러한 문제를 해결하기 위하여, 일반인들이 자연 생태계에서 관찰한 내용을 바탕으로 곤충식별을 도와주는 스마트폰 기반의 유러닝시스템인 곤충 종 식별추론 시스템을 제안하였다. 본 시스템은 사용자의 곤충관찰정보와 생물학적 곤충특성과의 유사도에 기반하여 추론검색을 수행한다. 이를 위해, 생물학적 곤충특성을 목, 과, 종 단위의 27개 항목으로 분류하고, 관찰 단계별 유사도 지표를 제안하였다. 또한, 본 연구의 유용성을 보이기 위하여 추론검색 프로토타입시스템을 개발하고, 기존의 분류검색시스템과의 곤충식별 비교테스트를 하였다. 실험결과, 본 연구의 추론검색 방법이 곤충식별의 효과성에 있어 더 우수함을 보였고, 검색시간에 있어서도 보다 효율적인 시스템이 될 수 있음을 보였다.

• 천문학회보
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• 제30권1호
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• pp.28.2-28.2
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• 2005

• 천문학회보
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• 제42권1호
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• pp.34.3-35
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• 2017

Spectral energy distribution camera for QUasars in EArly uNiverse (SQUEAN) is a successor of Camera for Quasars in EArly uNiverse (CQUEAN) which was developed by Center for the Exploration of the Origin of the Universe and operated at the 2.1 m Otto Struve Telescope in the McDonald Observatory, USA, since 2010. The software of SQUEAN controls a science camera, a guiding camera, and a filter wheel, and communicates with the telescope control system (TCS). It has been constantly revised and modularized according to the upgrades of the TCS and the hardware changes. Recently we have implemented the stable network communication and the semi-automatic focusing modules to enhance observational convenience. In this presentation we describe the current status of the SQUEAN control software and introduce a software architecture which is optimized on efficient astronomical observations.

• Journal of Astronomy and Space Sciences
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• 제14권2호
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• pp.320-329
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• 1997

전파연구소 이천 분소에는 각각 세 개의 안테나로 30MHz∼2500MHz 대역의 태양전파를 관측할 수 있는 광대 역 태양전파분광시스템이 1995년에 설치되었다. 그 동안 태양전파 데이터를 수집 분석할 수 있는 소프트웨어가 없어 실질적인 관측이 이루어지지 않았으나 본 연구에 의해 운용 소프트웨어가 개발됨으로써 본격적인 태양전파관측 연구를 수행할 수 있게 되었다. 개발된 운용 소프트웨어를 실험 이용한 결과 1997년 11월 4일 06시경(UT)에 연속하여 발생한 3개의 TYPE III Burst에 대한 양질의 관측자료를 얻을 수 있었다. 본 논문에서는 전파연구소 이천 분소의 광대역 전파분광시스템을 소개하고 태양전파 데이터의 취득, 처리 및 분석을 위해 개발한 소프트웨어와 이를 통해 관측된 결과에 대하여 설명한다.