• 천문학회보
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• 제44권2호
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• pp.74.3-74.3
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• 2019

SCUBA-2 North Ecliptic Pole survey, one of the ongoing JCMT large programs, is designed to obtain 850 ㎛ imaging data over ~4 deg² around the NEP based on the AKARI NEP-Wide survey. By August 2019, the program is 50 % complete in terms of observing time, increasing the submillimeter coverage by a factor of 2 with the comparable depth. The rms measured in the deepest center is 0.92 mJy/beam, slightly above the 850 ㎛ confusion limit. With 4 σ detection, the source count is 50 % complete at 9 mJy. The surface density of submillimeter galaxies at this flux limit is 200 deg^-2. Multi-wavelength identification of the 850 ㎛ sources was done through the likelihood analysis based on the far-infrared (250-500 ㎛), mid-infrared (18 ㎛), near-infrared (2-4 ㎛), and optical (i-band) source catalog. We are going to present morphologies and physical properties of 850 ㎛ selected submillimeter galaxies with the help of ancillary multi-wavelength datasets over the NEP area.

• 대한원격탐사학회지
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• 제39권2호
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• pp.233-246
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• 2023

수문순환의 이해와 효율적 수자원 관리의 측면에서 토양수분의 중요성이 조명되고 있으나, 국내에는 양질의 지점 토양수분 자료의 부재로 그 활용도가 매우 낮은 실정이다. 때문에 인공위성 기반의 토양수분을 적용할 때에도, 기준자료가 되는 지상 관측자료가 없어 객관적인 평가 및 교정이 어려운 실정이다. 코즈믹 레이 중성자 탐지센서(cosmic-ray neutron probe, CRNP)를 활용한 토양수분 관측소는 위성 자료의 검보정을 위한 기준 자료 생산에서 핵심적인 역할을 수행할 수 있다. CRNP는 비침습식으로 설치가 가능하여 토양층 교란과 식생 환경의 피해를 최소화할 수 있고, 공간 대표성을 가진 중간 규모의 관측 범위를 가지고 있다는 장점이 있다. 이러한 특징은 지형이 복잡하고 식생이 우거진 지형이 많은 우리나라에서의 활용이 용이하다는 장점으로 이어진다. 따라서 본 연구는 한국형 코즈믹 레이 토양수분 관측 시스템(Korean cOsmic-ray Soil Moisture Observing System, KOSMOS) 구축의 일환으로, CRNP를 활용한 토양수분 관측소의 국내 적용성을 평가하고자 수행되었다. CRNP 관측소는 전력 및 설치 부지 확보의 용이성과 추후 타 수문기상 인자와의 효율적 활용을 고려하여, 한강홍수통제소의 홍천군 군업리 관측소에 병행 설치되었다. CRNP 토양수분 자료의 평가를 위해 12개소의 지점 토양수분 센서를 추가로 설치하였으며, 시간 안정성 분석을 통해 공간적 대표성을 평가하였다. CRNP에서 생성되는 중성자는 평균 1,087 counts per hour 정도로 설마천 관측소에 비해 낮게 나타나 홍천 관측소의 환경이 더 습윤한 환경임을 알 수 있었다. 관측된 중성자 자료의 중성자 보정과 초기교정을 통해 토양수분을 산정하였으며, 산정된 토양수분 자료는 짧은 교정 기간에도 지점 자료와의 검증에서 r=0.82로 높은 상관성을 보여주었고, root mean square error=0.02 m³/m³의 높은 정확도를 보여주었다. 추후 계절성을 반영할 수 있도록 연간 자료가 축적된 후 재교정을 수행하면 보다 높은 정확도를 보여줄 것으로 판단된다. 이러한 결과는 CRNP 토양수분 자료의 우수성을 검증한 선행연구들과 더불어, KOSMOS 구축 시 양질의 토양수분 자료를 생산할 수 있음을 시사한다.

• 한국지반공학회:학술대회논문집
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• 한국지반공학회 2008년도 춘계 학술발표회 초청강연 및 논문집
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• pp.697-703
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• 2008

Excessive water leakage phenomenon happens through damage of nation core zone of about 17,000 storage of water facilities or collapse of dam is worried, is being damaged or enforce dilapidated fill dam core zone's repair reinforcement. Example that use grouting method of construction considering construction and economic performance etc. recently by repair reinforcement way about defect of dam is increased. Permeation grouting method repair & reinforcement of fill dam countermeasure is preferred in nation. Do that is economical to decide these repair reinforcement effect and grouting effect estimation method that do not give damage to dam is effective. Therefore, observing electricity resistivity Survey change of dam since grouting reinforcement using Electric resistivity Survey inquiry of seismic survey method in this research, Wished to verify grouting effect whether is possible as Electric resistivity Survey, and study whether integrity of dam through repair reinforcement defined.

• 천문학논총
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• 제23권2호
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• pp.17-23
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• 2008

From the short-period variability survey (SPVS), we obtained time-series BV CCD images in the region of an open cluster M50 (NGC 2323) for 10 nights from 2008 February 9 to 27. The observation was performed using a small refracting telescope (${\phi}$=155mm, f=1050mm) in Bohyunsan Optical Astronomy Observatory (BOAO). M50 is included in the observing field of ASAS (The All Sky Automated Survey). In the region of M50, we found 8 new variable stars including two ${\delta}$ Scuti stars with short-periods and very small amplitudes. There are known nine variable stars by the catalogues of ASAS and GCVS in the region. We confirmed the variability of the known variable stars for six and non-variability for three.

• 대한지구과학교육학회지
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• 제5권2호
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• pp.166-174
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• 2012

This study is purposed to survey on astronomical observation experiences of elementary students and teachers. Survey samples are 182 elementary students and 51 elementary teachers, and 8 students and 2 teachers among them are interviewed. The results of this study show that most elementary students are not interested in observing constellations, planets, and moon. Also most elementary students and teachers are not taught to observe astronomical objects. Finally, regarding the difficulty of astronomical practice, teachers pointed out that lack of knowledge about astronomy.

• 천문학논총
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• 제22권4호
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• pp.141-149
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• 2007

Preliminary time-series observations for short-period variability survey (SPVS) were carried out using a 155mm refractor and a $2k{\times}3k$ CCD camera at Bohyunsan Optical Astronomy Observatory. We found 21 new variable stars in the $90'{\times}60'$ test field region : 9 eclipsing binary stars, $5{\delta}$ Scuti type stars, a ${\gamma}$ Doradus type star, and 6 long period variables. The observing field center is R.A. $05^h\;00^m\;00^s$, DEC. $50^{\circ}\;00'\;00"$ (J2000.0). The period and amplitude ranges for the short-period variables, i.e., ${\delta}$ Scuti stars, were 0.052day - 0.107day and 0.012mag - 0.064mag, respectively.

• 천문학회보
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• 제44권1호
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• pp.62.1-62.1
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• 2019

Current large observational projects perform both static and dynamic sky surveys. The Thirty-Minute Target of Opportunity (TMT) is the project focusing on the dynamic sky survey using Korea Microlensing Telescope Network (KMTNet) that is the best observing system to investigate the dynamic sky. TMT aims to perform and experiment on following components : 1) to select transient or variable sources having hour to day scale cadences for future science cases, 2) to optimize the observation strategy for these objects, 3) to provide automated photometric pipelines for the time series data, and 4) to test the data release environment for all astronomers. In the near future, it is expected that a huge number of events will be alerted through large area surveys such as LSST. Therefore, the TMT project will provide opportunities to prepare the future large survey era as well as to understand the nature of interesting astronomical events.

• Geomechanics and Engineering
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• 제30권4호
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• pp.337-343
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• 2022

The electrical resistivity method is a well-known geophysical method for observing underground conditions, (such as anomalies) and the properties of soil and rock (such as porosity, saturation, and pore fluid characteristics). The shape of electrodes used in an electrical resistivity survey depends on the purpose of the survey and installation conditions. Most electrodes for field applications are cylindrical for sufficient contact with the ground, while some are conically sharpened at their tips for convenient penetration. Previous study only derived theoretical equations for rod-shaped electrodes with spherical tips. In this study, the theoretical resistance for two cylindrical electrodes with conical tips is derived and verified experimentally. The influence of the penetration depth and tip on the measurement is also discussed.

• 한국조사연구학회지:조사연구
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• 제11권2호
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• pp.161-176
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• 2010

본 논문은 학위논문에 사용된 여론조사 자료의 품질을 평가하였으며, 또한 학위논문에 사용되는 데이터의 품질평가 모형을 제시하였다. 데이터의 품질평가와 평가모형에 사용한 평가지표는 한국조사연구학회에서 제시한 조사윤리강령 제3조의 16가지 항목을 사용하였다. 연구결과 학위논문에 사용된 여론조사 데이터의 품질은 낮은 수준임을 확인할 수 있었다. 16개 항목별로 석 박사학위에 따른 유의적인 차이가 있는지를 확인하기 위하여 두 집단 간 비율 차이 검정을 실시한 결과 표집오차와 분석방법의 수에서만 차이가 있을 뿐 다른 지표에서는 차이가 나타나지 않았다. 끝으로 학위논문에 사용된 여론조사 자료의 질을 평가하기 위한 품질평가를 위해 9가지 주요 평가지표에 가중치를 부여하는 모형을 제시하였다.

• 천문학회보
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• 제36권2호
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• pp.121-121
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• 2011

Thanks to KMTNet's wide field of view, it is time to implement imaging survey of extensive area of clusters of galaxies in the southern sky with modern instrument. As part of potential long-term survey of nearby (D < 50 Mpc) well-known clusters of galaxies, we propose a wide-field and deep survey of Fornax cluster as a first step of the project. By imaging the 400 square deg region (100 fields) enclosed within the five times virial radius of the Fornax cluster, in three SDSSfilters(g', r', i'), we can provide an unprecedented view of structure of Fornax cluster using sample from giant to dwarf galaxies. We will secure galaxies with brightness comparable to the limiting magnitude (r'=23.1 AB mag) of SDSS. Furthermore, we also request extremely deep (limiting surface brightness of ~ 28 mag $arcsec^{-2}$forr'band) survey for the central region (16 square degree, i.e., four fields) of Fornax cluster. This will allow us to detect the diffuse intracluster light (ICL) that permeates clusters as a valuable tool for studying the hierarchical nature of cluster assembly. In order to complete whole survey, about 285 hr observing time (without overhead) is required. By combining data available at other wavelengths, it will offer unique constraints on the formation of large-scale structure and also provide important clues for theories of galaxy formation and evolution. Our proposed survey will be implemented in the close collaboration with researchers in various countries (Germany, Australia, UK, USA) and ongoing project (e.g., SkyMapper).