• 한국조사연구학회지:조사연구
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• 제10권3호
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• pp.157-172
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• 2009

추출된 표본을 바탕으로 관심 모집단의 특성을 파악하는 조사연구에 있어서는 실제로 표본이 추출되는 표본추출틀의 모집단 대표성이 매우 중요하다. 표본추출틀이 관심 모집단을 적절한 수준으로 포함하지 못하는 경우 심각한 표본추출틀 편향이 발생하게 되고 이로 인하여 효율적인 추출법에 의하여 추출된 표본의 통계적 신뢰도 역시 손상된다. 그러나 대규모 조사를 위한 표본추출틀의 구축은 시간과 비용의 측면에서 비효율적이고 따라서 국가에서 제공하는 전수 조사 기반의 표본추출틀이 흔히 사용된다. 대표적으로 국내의 가구조사를 위한 표본추출틀로는 매 5년마다 시행되는 인구주택총조사 기반의 자료가 사용된다. 그러나 인구주택총조사 기반 표본추출틀의 경우 인구주택총조사 시점과 실제 조사 시점과의 시간적 차이로 인한 표본추출틀의 모집단 대표성에 문제가 발생하게 된다. 특별히 인구 유동성이 심한 서울과 같은 대도시의 경우 시간의 경과에 따른 모집단 분포의 변화가 심하게 나타나리라 예측할 수 있다. 따라서 본 연구에서는 2008 서울서베이 가구 조사를 위해 새롭게 표본추출틀을 구축한 것과 새 표본추출틀을 기초로 하여 표본을 추출한 사례를 다룬다. 기존 인구주택총조사 기반 표본추출틀이 시간이 지남에 따라 대표성을 상실하는 문제점을 지적하고 주민등록 DB와 과세대장 DB를 기반으로 한 새로운 표본추출틀을 2008년 서울서베이 가구조사를 위한 표본추출틀로 제시하였다. 새롭게 작성된 표본추출틀로부터의 가구표본추출과정과 가중치 및 모평균 추정량 또한 제시되었다.

• 천문학회지
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• 제36권3호
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• pp.249-260
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• 2003

ASTRO-F is the next generation Japanese infrared space mission of the Institute of Space and Astronautical Science. ASTRO-F will be dedicated to an All Sky Survey in the far-infrared in 4 bands from 50-200microns with 2 additional mid-infrared bands at 9microns and 20microns. This will be the first all sky survey in the infrared since the ground breaking IRAS mission almost 20 years ago and the first ever survey at 170microns. The All Sky Survey should detect 10's of millions of sources in the far-infrared bands most of which will be dusty luminous and ultra-luminous star forming galaxies, with as many as half lying at redshifts greater than unity. In this contribution, the ASTRO-F mission and its objectives are reviewed and many of the mission expectations are discussed.

• 천문학회보
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• 제35권1호
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• pp.77.2-77.2
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• 2010

A high redshift quasar is useful to investigate the early part of our universe. Since they are one of the brightest objects in the early universe, they can provide us with clues of the growth of super massive black holes and the early metal enrichment history. To discover the high redshift quasars, we designed a survey of wide area and moderate depth; Infrared Medium-deep Survey (IMS), a J-band imaging survey of ~200 $deg^2$ area where the multi-wavelength data sets exist. To obtain the J-band data, we are using the United Kingdom Infra-Red Telescope (UKIRT), and so far we have covered ~20 $deg^2$ with Y- or J-bands over three observing runs during 2009. We used color-color diagrams of multi-wavelength bands including i, z, Y, J, K, $3.6{\mu}m$ and $4.5{\mu}m$ to select high redshift quasars. The major challenge in the selection is many M/L/T dwarfs, low redshift galaxies, and instrumental defects that can be mistaken as a high redshift quasar. We describe how such contaminating sources can be excluded by adopting multiple color-color diagrams and eye-ball inspections. So far, our selection reveals two quasar candidates at z~7.

• 천문학회보
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• 제35권2호
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• pp.37.1-37.1
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• 2010

A high redshift quasar is useful to investigate the early part of our universe. Since they are one of the brightest objects in the early universe, they can provide us with clues of the growth of super massive black holes and the early metal enrichment history. To discover the high redshift quasars, we designed a survey of wide area and moderate depth; Infrared Medium-deep Survey (IMS), a J-band imaging survey of ~200 deg2 area where the multi-wavelength data sets exist. To obtain the J-band data, we are using the United Kingdom Infra-Red Telescope (UKIRT), and so far we have covered~40 deg2 with Y- or J-bands over 36 observing nights. We used color-color diagrams of multi-wavelength bands including i, z, Y, J, K, $3.6{\mu}m$ and $4.5{\mu}m$ to select high redshift quasars. The major challenge in the selection is many M/L/T dwarfs, low redshift galaxies, and instrumental defects that can be mistaken as a high redshift quasar. We describe how such contaminating sources can be excluded by adopting multiple color-color diagrams and eye-ball inspections. So far, our selection reveals one quasar candidates at z~7 and a few candidates at z~6. In this poster presentation, we will update the current status of the quasar selection in the IMS fields.

• 한국원자력학회:학술대회논문집
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• 한국원자력학회 2004년도 추계학술발표회 발표논문집
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• pp.1455-1456
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• 2004

• 한국원자력학회:학술대회논문집
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• 한국원자력학회 2005년도 춘계학술발표회
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• pp.1191-1192
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• 2005

• 한국과학교육학회지
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• 제10권2호
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• pp.39-47
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• 1990

The purpose of this survey is to investigate the status on attitudes toward science among the elementary school students in Korea. The attitudes toward science were measured with TOSRA(Test of Science-Related Attitudes) Which was developed by Fraser, B.J.. This survey were male 963 elementary school students of $4^{th}-6^{th}$ in Seoul and Kyeong gi Province as an object. The major findings of the study are as follows: 1. The overall attitudes toward science of measured elementary school students shows a positive tendency. 2. Male students exhibited significantly(p<0.001)more positive attitudes toward science than females. 3. There were no differences(p<0.05) between the students in Seoul and Kyeong gi Province in attitudes toward science. 4. Attitudes toward science of elementary school students in this population steadily declined from grade four to grade six. The sharpest decline was seen at grade six.

• Journal of Acupuncture Research
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• 제28권2호
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• pp.1-11
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• 2011

Objectives : The aim is to comprehend the difference of moxibustion used according to applied body parts (knee pain, neck pain, back pain) to oriental doctors running clinic in Seoul. Methods : A sampling of 288 oriental doctors running clinic in Seoul was done and the doctors were asked to fill out 20 questions by interviewing directly from Nov. 23. 2009 to Jan. 9. 2010. Results : The result shows that moxibustion was used for knee pain and back pain more than neck pain. The type of moxibustion mostly used was sticker moxibustion for all three symptoms. Burn marks were left mostly in knee and back pain. Most large volume of moxa was used to back pain. More than half of the oriental doctors used 1-3 acupoints for one procedure and on average 2-3 sessions was done. Patients with knee pain and back pain had more than 4 sessions compared to neck pain. Treatments were mostly done 3 times a week, and as for total treatment period, it took less than 1 week for acute symptom, and it took more than 1 week and less than 5 weeks for chronic symptom. Conclusions : This research shows that the method of moxibustion used differs according to the area of treatment(knee pain, neck pain, back pain) by survey of oriental doctors through direct interviews.

• 한국작물학회:학술대회논문집
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• 한국작물학회 2002년도 추계 학술대회지
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• pp.44-44
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• 2002

• 천문학회보
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• 제16권
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• pp.14.1-14.1
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• 1991