• 대한융합한의학회지
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• 제3권1호
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• pp.15-27
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• 2022

Objectives: This study was conducted to review the overall concept of nutritional evaluation of infants and young children. Methods: Literature search was done to study definition, method and importance of nutritional evaluation of infants and young children. Pubmed and Google scholarship were used in the research. Search words were 'Nutritional evaluation', 'infants' and 'young children'. Results: Nutrition evaluation is mainly used by physical measurement, clinical evaluation, dietary intake survey, and biochemical test depending on the age and disease. The treatment method for 治未病, which is a concept of korean medicine, and 健兒法 for treating the concept of weak children are considered to have very high applicability in solving various problems found through nutrition evaluation in korean medical approach. Conclusion: Infants and children are the fastest growing period of their lives, showing rapid growth in physical, and emotional development along with rapid brain growth. Therefore, inadequate nutrition during this period affects mental and physical growth and development not only during that period but also throughout life. Nutrition evaluation is divided into regular evaluation that includes children in all growing seasons and screening evaluation for problem solving, and follow-up nutritional evaluation that evaluates nutritional status in the long run. For each nutritional evaluation, evaluation is conducted by physical measurement, clinical evaluation, dietary intake survey, and biochemical test. By comprehensively interpreting them, nutritional status is determined. This study provides basic data on the proper nutrition evaluation method to identify and correct nutritional problems such as growth level, nutritional deficiency, and nutritional excess early.

• 대한교통학회지
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• 제33권1호
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• pp.14-28
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• 2015

2000년대 중반부터 인터넷 검색 트래픽을 활용한 다양한 연구가 진행되었다. 대표적으로 구글은 미국의 독감 발병 상황을 인터넷 유저의 검색 패턴을 통해 예측하는 서비스를 만들기도 하였다. 교통지표 역시 인터넷 검색 패턴과 유사할 수 있다는 가설을 확인하기 위하여, 검색 트래픽 데이터를 활용하여 고속도로의 진입 교통량과 구간 속도를 추정하는 모형을 구축하고 적합도 등을 확인하는 것이 본 연구의 목적이다. 그 결과, 첫째, 출퇴근의 상시적 통행이 이루어지는 지점의 TCS 진입 교통량 모형은 구글 검색 트래픽이 입력변수로 우수하였고, 검색 트래픽과는 음의 상관관계를 보였다. 둘째, 여가 통행이 집중적으로 나타났던 지점의 TCS 진입 교통량 모형은 네이버의 검색 트래픽이 입력변수로 선정되었으며, 검색 트래픽과는 양의 상관관계가 나타났다. 셋째, VDS 속도의 경우 시계열 도표상 검색 트래픽과 음의 상관관계를 보였다. 넷째, 검색 트래픽을 입력변수로 활용한 전이함수 잡음 시계열 모형은 그렇지 않은 시계열 모형에 비해 비교적 적합도가 우수하다는 결과를 도출하였다. 다만, VDS 속도 모형의 경우 다수의 입력변수가 포함되고 모형 계수의 부호가 상이함에 따른 한계가 존재하였다. 향후 검색 트래픽의 출처나 검색어, 혹은 시차 및 집계 단위에 대한 추가적 연구가 진행된다면, 교통 분야의 빅 데이터 연구시 활용 폭이 넓어질 것으로 판단된다.

• 천문학회보
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• 제40권1호
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• pp.75.3-75.3
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• 2015

Large area infrared surveys are often accompanied with follow-up optical spectroscopic surveys that has a significant legacy value even for other areas of research. Using these spectral database, we have performed a search for MgII absorption lines in the optical spectrum of background quasar. Over the ~4deg2 of AKARI North Ecliptic Pole survey field and Spitzer First Look Survey field, 18 and 16 MgII absorber systems are identified respectively. The redshift range for the background quasars was 1.0<$z_{qso}$<3.4, while the redshift range for the absorber was 0.6<$z_{abs}$<1.6. Galaxies responsible for MgII absorptions are identified in the deep optical images (CFHT r-band), yet the identification still remains ambiguous for 60% of the systems due to the limited image depth and the source crowdedness. The impact parameter ranges 20-60kpc, and the rest-frame equivalent width of MgII absorption ranges $0.7-4{\AA}$. The most critical part in the identification of MgII absorber galaxies is the existence of deep optical images in addition to the high S/N quasar spectrum with R>3000.

• 대한간호학회지
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• 제26권2호
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• pp.497-506
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• 1996

Gradually, there has been increase in the use of qualitative research methods in nursing research. Nursing scholars are using qualitative research methods to explore the essence of nursing and discover its meaning. However, there has been lack of standards for evaluating qualitative nursing research. Often nursing researchers are applying quantitative research evaluation standards to qualitative nursing research. Thus, there has not been any notable qualitative research done to date. In order to improve the quality of nursing research done to discover new knowledge for the nursing, ＆ for development of nursing theory, criteria for critiquing qualitative research should be established. Therefore, this researcher introduced standards as criteria for critiquing qualitative research which are based on literature reviews and re search experiences. The suggested criteria are developed several question's as follows : 1) description of the research phenomena, 2) significance, 3) research purpose, 4) research question, 5) assumptions, 6) researcher's abilities, 7) selection of research samples, 8) data collection, 9) human subjects, 10) data analysis, 11) description of researcher's results, 12) literature review. Follow-up of concrete questions for each of the criterias have been developed.

• Journal of the Korean Statistical Society
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• 제35권2호
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• pp.201-212
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• 2006

The technique of foldover is usually used by experimenters to de-alias the effects that are interesting in follow-up experiment. Employing a $2^{k-p}$ design with resolution III or higher, Li and Lin (2003) developed an algorithm and used computer programs to search its corresponding optimal foldover design for selected 16-run and 32-run experiments. Based on the minimum aberration criterion, the strong combined-optimal design, defined by Li and Lin, is the better choice of the initial design. In this article, we apply the technique of blocking to find the strong combined-optimal designs. Furthermore, we will tabulate all 16-run and 32-run strong combined-optimal designs and their corresponding core foldover plans for practical use. Some new designs that have not appeared in the other literature but constructed by the technique of blocking are also proposed in this article.

• 천문학회보
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• 제41권2호
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• pp.58.1-58.1
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• 2016

During the year 2016 the newly installed NYSC (National Youth Science Center) 1m optical telescope was officially commissioned. Calls for future observational programmes were announced. During test observations we carried out an observational project aimed at follow-up observations of transiting extrasolar planets. To predict future transits we developed the "TransitSearch" code implemented in Python utilizing transit information from the Open Exoplanet Catalogue. During three nights in April and June 2016 we observed planetary transits of HAT-P-3b and TrES-3b. Preliminary light curves of the transit events are presented alongside with best-fit models. From this experience we plan to improve the optical alignment and photometric performance by operating the 1m NYSC telescope in a strongly out-of-focus mode for transit observations.

• 천문학회보
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• 제44권1호
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• pp.58.1-58.1
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• 2019

Gravitational-wave (GW) sources for the next decades would be in majority binaries consisting of neutron stars and/or black holes reside in the extragalactic environment. For example, GW170817 was the first extragalactic neutron star - neutron star binary found by GW observations and it was proved the power of multi-messenger astronomy (MMA) including the KMTNet observations. With the ever increased sensitivity, the $3^{rd}$ observation run (O3) led by the advanced LIGO and advanced Virgo this year aims to search for more 'standard' populations as well as 'exotic' ones expected by stellar evolution. I will present highlights of on-going efforts by researchers in Korea and those in abroad for estimating physical parameters of a source. Mass, spin, distance, and location are prerequisite information to constrain theoretical understanding of the source formation and evolution. Furthermore, these information are to be shared with the international community for follow-up multi-messenger observations. I will present the observational accuracy expected for the future GW observations and discuss their implications. If time allows, I will make a few remarks on prospects of O3 with KAGRA collaborations, which many domestic researchers are closely involved in.

• 천문학회보
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• 제44권1호
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• pp.61.4-61.4
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• 2019

The key science goal of the KMTNet Supernova Program (KSP) is to detect and study the early explosions of supernovae using one fifth of the KMTNet time. The BVI-band observations of the nearby target fields mostly closer than 30 Mpc distance and the follow-up spectroscopy provide valuable information on the early phase of the supernovae. These data can also be used for the studies of optical transients such as novae, dwarf novae, variable stars, and active galactic nuclei. Stacked images of several hundred images obtained from the time domain observations can be used for the search of low surface brightness galaxies reaching $28mag\;arcsec^{-2}$. Results and status of the KSP including ${\geq}20$ infant supernovae and ${\geq}100$ faint dwarf galaxies will be presented in this talk.

• 한국정보과학회논문지:소프트웨어및응용
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• 제36권8호
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• pp.623-632
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• 2009

본 논문에서는 연속시점에서 촬영한 CT 영상에서 대응되는 폐결절을 추적 관찰하기 위한 폐결절 정합 방법을 제안한다. 제안 방법은 다음과 같은 다섯 단계로 구생된다. 첫째, 분할된 폐를 포함하는 최적경계볼륨의 중심으로 위치 차이를 보정한다. 둘째, 초기 CT 영상과 추적 CT 영상에서 가장 높은 밝기값을 가지고 있는 갈비뼈 구조를 포함하는 관상최대강도투사 영상을 생성한다. 셋째, 두 관상최대강도투사 영상 간의 정규화된 평균 밝기값 차이를 통해 강체 변환을 최적화한다. 넷째, 강체 정합 후에 폐결절 중심 간의 유클라디안 거리 측정을 통해 대응되는 폐결절 대응 후보를 정의한다. 마지막으로, 폐결절을 매칭하기 위하여 초기 CT 영상 내에 폐결절 템플릿과 추적 CT 영상 내에 탐색 볼륨 간의 템플릿 매칭을 수행 한다. 본 제안 방법의 결과를 평가하기 위하여 육안 평가, 정확성 및 수행시간 측정을 수행하였다. 실험결과 관상최대강도투사를 기반으로 하는 강체정합과 지역적 템플릿 매칭을 이용하여 폐결절이 정확하고 빠르게 정합됨을 알 수 있었다.