• 응용통계연구
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• 제29권4호
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• pp.657-678
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• 2016

본 연구는 영화 흥행에 미치는 온라인 구전 변수들의 영향을 다루었다. 2012년 부터 2015년까지 4년 동안 국내에서 개봉한 총 관객 수 50만 이상인 276편의 영화에 대한 통계분석 결과 개봉 후 포털의 평가자 수, 개봉 후 블로그 수, 개봉 후 뉴스 수와 같은 온라인 구전의 크기를 나타내는 변수들이 온라인 구전의 방향을 나타내는 개봉 후 포털의 평점이나 혹은 영화의 내재적 속성을 나타내는 변수들로서 감독, 배우, 배급사, 등급, 국적, 개봉 월, 개봉 계절 등 보다 영화 흥행과 더욱 연관성이 있었다.

• 대한화학회지
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• 제36권1호
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• pp.87-94
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• 1992

본 연구는 폴리스티렌(PS), 폴리메틸메타크릴레이트(PMMA), 및 폴리부타디엔(PB) 등 동종 중합체들(homopolymers), 그리고 폴리스티렌-폴리메틸메타크릴레이트 block 혼성중합체들(SM block copolymers) 및 스티렌-폴리부타디엔 star shaped 혼성중합체들(PS-PB star shaped copolymers)을 선택하여 다리걸친 폴리스티렌 겔 상에서의 용리거동을 비교 조사하였다. 선택한 이동상으로는 테트라히드로퓨란(THF), 톨루엔(TOL), 클로로포름(CHL), 메틸렌클로라이드(MC), 테트라히드로퓨란-시클로헥산(CH) 혼합용매의 5가지 시스템이며, 이동상 변화에 따른 시료들의 hydrodynamic 부피와 머무른 부피 사이에 플롯의 이동에 관한 현상을 조사하였으며, 또한 시료의 머무름을 예측하기 위해 다중 다단계 회귀분석(multiple stepwise regression analysis)을 수행한 결과, 각 중합체들에 대한 적절한 크기 파라미터를 찾았다. 또한, network-limited 분리 메카니즘에 의해 GPC에서 시료와 겔사이의 상호작용에 대한 분포계수 $K_p$를 각 이동상 시스템에서 구하였는데, PS와 PB의 kp값은 거의 1에 가까운 값을 나타내었고 PMMA인 경우는 적합 용매에서는 분자량이 증가할수록 $K_p$값은 다소 감소하였으나 부적합 용매에서는 분자량이 증가함에 따라 $K_p$값은 함께 증가하였다. 혼성중합체의 $K_p$값은 조성 및 분자량에 따라 달라짐을 알 수 있었고, 이로부터 SM block 혼합중합체의 형태는 무작정상(random phase)을 가지는 것으로 예측된다. 아울러 $K_p$값을 이용하여 동종중합체 및 폴리스티렌 혼성중합체들의 분자량을 측정하기 위해 이들의 새로운 머무름 파라미터$(V_r-V_o)/K_p$와 log[η]M을 플룻을 한 결과 좋은 직선성을 보이는 하나의 보편적 검정곡선을 얻었다.

• Journal of Astronomy and Space Sciences
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• 제34권3호
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• pp.199-205
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• 2017

A high resolution spectroscopic observation of the red supergiant star RM_1-390 in the Large Magellanic Cloud was made from a 3.6 m telescope at the European Southern Observatory. Spectral resolving power was R=20,000, with a signal-to-noise ratio S/N > 100. We found the atmospheric parameters of RM_1-390 to be as follows: the effective temperature $T_{eff}=4,250{\pm}50K$, the surface gravity ${\log}\;g=0.16{\pm}0.1$, the microturbulent velocity $v_{micro}=2.5km/s$, the macroturbulence velocity $v_{macro}=9km/s$ and the iron abundance $[Fe/H]=-0.73{\pm}0.11$. The abundances of 18 chemical elements from silicon to thorium in the atmosphere of RM_1-390 were found using the spectrum synthesis method. The relative deficiencies of all elements are close to that of iron. The fit of abundance pattern by the solar system distribution of r- and s-element isotopes shows the importance of the s-process. The plot of relative abundances as a function of second ionization potentials of corresponding chemical elements allows us to find a possibility of convective energy transport in the photosphere of RM_1-390.

• 한국임상약학회지
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• 제25권3호
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• pp.131-137
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• 2015

Background: The protective effect of metformin against breast cancer is inconclusive. Objective: To evaluate the effect of metformin on breast cancer risk and mortality in patients with type 2 diabetes. Method: A comprehensive literature search was performed for pertinent articles published prior to June 30, 2014, using PubMed and EMBASE. Study heterogeneity was estimated with $I^2$ statistic. The data from the included studies were pooled and weighted by random-effects model. The quality of each included study was assessed on the basis of the 9-star Newcastle-Ottawa Scale and publication bias was evaluated by visual inspection of a funnel plot. Results: Ten studies were included in the meta-analysis of the association of metformin and breast cancer risk. By synthesizing the data from the studies, the pooled odds ratio (OR) was 0.72 (95% CI: 0.59, 0.87) (p = 0.0005). Three cohort studies were included for meta-analysis of the association between metformin and breast cancer-related mortality. Metformin was associated with a significant decrease in mortality (Risk ratio: 0.68; 95% CI: 0.51, 0.90, p = 0.007). Conclusion: The present meta-analysis suggests that metformin appears to be associated with a lower risk of breast cancer incidence and mortality in patients with type 2 diabetes.

• Geomechanics and Engineering
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• 제9권6호
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• pp.689-707
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• 2015

Progressive increase in population causing land scarcity, which is forcing construction industry to build multistory buildings having underground basements. Normally, basements are constructed for parking facility. This research work evaluates important factors which have caused the collapse of pile-anchor system at under construction five star hotel. 21 m deep excavation is carried out, to have five basements, after installation of 600 mm diameter cast in-situ contiguous concrete piles at plot periphery. To retain piles and backfill, soil anchors are installed as pit excavation is proceeded. Before collapse, anchors are designed by federal highway administration procedure and four anchor rows are installed with three strands per anchor in first row and four in remaining. However, after collapse, system is modeled and analyzed in plaxis using mohr-coulomb method. It is investigated that in-appropriate evaluation of soil properties, additional surcharge loads, lesser number of strands per anchor, shorter grouted body length and shorter pile embedment depth caused large deformations to occur which governed the collapse of east side pile wall. To resume work, old anchors are assumed to be standing at one factor of safety and then system is analyzed using finite element approach. Finally, it is concluded to use four strands per anchor in first new row and five strands in remaining three with increase in grouted and un-grouted body lengths.

• 천문학회보
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• 제35권2호
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• pp.67.2-67.2
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• 2010

We present results of searching for the Very Low Luminosity Objects (VeLLOs; internal luminosity : $L_{int}$ < $0.1(d/140pc)^2\;L\odot$) in the Gould's Belt clouds using observations from 3.6 to 70 micron by the Spitzer Space Telescope. The clouds are California, Chamaeleon I, III, Musca, Lupus V, VI, Scorpius, Serpens, Corona Australis, Cepheus, and IC 5146 having the properties of active low-mass star-forming such as the Taurus cloud. The observing sensitivity of the Spitzer data is estimated to be about $L_{int}\;\geq\;5\times10^{-3}(d/140pc)^2\;L\odot$, a factor of 20 better than that of the Infrared Astronomical Satellite (IRAS). The observing data were processed by the c2d Legacy pipeline. As the criteria to select the VeLLOs, we slightly modified previous ones by Dunham et al. The most important criterion is a flux density at 70 micron that is directly converted to the internal luminosity. Also, we used additional criteria to remove the contamination of evolved stars and extragalaxies which have colors or SEDs very similar to YSOs. We identified a total of 64 new embedded VeLLO candidates with $L_{int}$ < $0.1(d/140pc)^2\;L\odot$, consisting of 8 in California, 15 in Chamaeleon-Musca, 13 in Scorpius-Lupus, 20 in Serpens, 3 in Corona Australis, 3 in Cepheus, and 2 in IC 5146. The classification of the spectral index (${\alpha}$) fitted to the shape of the Ks-24 micron SEDs shows most of VeLLO candidates (89%) are in types of Class I and Flat spectrum. We plot various diagrams based on their 2MASS-Spitzer bands colors and magnitudes to discuss properties of the VeLLOs. This search will lead us new adventure toward a future systematic study of the VeLLOs.

• Animal cells and systems
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• 제16권4호
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• pp.329-336
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• 2012

This study evaluated ecological health, using various biomarkers and bioindicators, of pale chub (Zacco platypus) as a sentinel species, in Daejeon Stream, South Korea, during AprilMay 2011. The biomarkers and bioindicators were compared among three sites of control: Reference ($C_z$), transition ($T_z$), and the urban zones ($U_z$); and the 7-Ethoxyresorufin-O-deethylase (EROD) activity, DNA damage, acetylcholinesterase (AChE) activity, and vitellogenin (VTG) concentrations were more significantly increased in the $U_z$ than in the $C_z$. Also, physiological markers such as condition factor, liver somatic index, visceral somatic index, and gonad somatic index were significantly increased in the $U_z$ than in the $C_z$. For the health assessments, three categorized parameters of blood chemistry, molecular biomarkers, and physiological bioindicators were standardized and calculated as a star-plot, representing values of Integrated Health Response (IHR). Values of IHR had more significant (P<0.05) increases in the $U_z$ than any other zones, indicating an impairment of ecological health by organic matter, nutrients (N, P), and toxic chemicals. This study is based on low levels of biological organization approach of molecular and physiological biomarkers and bioindicators, so further study of high-levels of biological organization approach such as community and population is required for overall range of health assessments. The approach of IHR values, however, may be useful in providing early warning of future impacts on ecological health.