• 한국안광학회지
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• 제13권4호
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• pp.155-160
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• 2008

목적: ICL 렌즈 시술 후 잔류난시가 측정될 경우 시술에 사용된 ICL 렌즈의 상태를 분석할 수 있는 프로그램의 개발이 본 연구의 목적이다. 방법: ICL 렌즈 시술 후 측정된 잔류난시를 분석하여 시술된 ICL 렌즈의 회전각 및 ICL 렌즈의 대응 MR 처방식을 산출하는 식을 유도하였다. 이 식에 의해 계산된 ICL 렌즈 회전각 및 시술된 ICL렌즈의 대응 MR 처방식을 윈도우 화면에서 시각적으로 편리하게 확인할 수 있는 프로그램을 델파이 6.0언어를 사용하여 개발하였다. 결과: ICL 렌즈 시술 후 측정된 잔류난시를 분석하여 시술된 ICL 렌즈의 회전각 및 대응 MR처방식을 산출하는 식을 유도하여 시술 후 ICL 렌즈의 상태를 분석할 수 있는 프로그램을 개발하였다. 개발된 프로그램으로 우리는 시각적으로 편리하게 시술 후의 ICL 렌즈의 상태를 분석할 수 있게 되었다. 결론: 개발된 프로그램에 임상사례를 적용해 본 결과 개발된 프로그램은 시술 후의 ICL 렌즈의 상태를 분석하는데 효과적인 것으로 판단되었다.

• Bulletin of the Korean Chemical Society
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• 제27권6호
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• pp.886-892
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• 2006

The interaction between tetraethylammonium chloride (TEACl) with ICl and tetraethylammonium iodide (TEAI) and aza-15-crown-5 (A15C5) with $I_2$ and ICl have been examined spectrophotometrically in acetonitrile solution. The results of TEACl-ICl indicate the formation of $ICl_2$ - through equilibrium reaction. In the case of TEAI-$I_2$ and A15C5-$I_2$, the equilibrium formation of $I_3$ - is confirmed. The interaction of TEAI-ICl begins with the simultaneous production of $I_2$ and IC$I_2$ - (at TEAI/ICl < 0.5) as well as continues with the simultaneous consumption of $I_2$ and formation of I$I_3$ - (at TEAI/ICl > 0.5). Similar behavior is also observed for A15C5-ICl system. However, the changes are seen at A15C5/ICl mole ratios less and more than 0.66. Several equations have been suggested for the formation of detected species. The formation constants of various reactions were evaluated from the computer fitting of the absorbance-mole ratio data. IR spectra of A15C5 and 1:1 A15C5:ICl or A15C5:$I_2$ complexes are compared and the effect of complexation on absorption bands is discussed.

• 천문학회보
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• 제43권2호
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• pp.33.3-34
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• 2018

Galaxy clusters contain a diffuse component of stars outside galaxies, that is observed as intracluster light (ICL). Since the ICL abundance increases during various dynamical exchanges of galaxies, the amount of ICL can act as a measurement tool for the dynamical stage of galaxy clusters. There are two prominent ICL formation scenarios; one is related to the brightest cluster galaxy (BCG) major mergers, and the other to the tidal stripping of galaxies. However, it is still under debate as to which is the main ICL formation mechanism. In this study we improve on earlier observational constraints of the ICL origin, by investigating it in a massive fossil cluster at z~0.47. Fossil clusters are believed to be dynamically matured galaxy clusters which have dominant BCGs. Recent simulation studies imply that, BCGs have assembled 85~90% of their mass by z~0.4 (e.g., Contini et al. 2014). Thus our target is an optimal test bed to examine the BCG-related scenario. Our deep images and Multi-Object Spectroscopic observations of the target fossil cluster (Gemini North 2018A) allow us to extract the ICL distribution, ICL color map and ICL fraction to cluster light. We will present a possible constraint of the ICL origin and discuss its connection to the BCG and the host galaxy cluster.

• 천문학회보
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• 제46권2호
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• pp.42.2-42.2
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• 2021

Intraclusterlight (ICL) is diffuse light from stars that are bound to the clusterpotential, not to individual member galaxies. Understanding the formationmechanism of ICL provides critical information on the assembly and evolution ofthe galaxy cluster. Although there exist several competing models, the dominantproduction mechanism is still in dispute. The ICL measurement between z=1 and 2strongly constrains the formation scenario of the ICL because the epoch is whenthe first mature clusters begin to appear. However, the number of high-redshiftICL studies is small mainly because of observational challenges. In this study, based on deep HST WFC3/IR data, we measured ICL of 10 galaxy clusters atredshift beyond unity, which nearly doubles the sample size in this redshiftregime. With careful handling of systematics including object masking, skyestimation, flatfielding, dwarf galaxy contamination, etc., we quantified thetotal amount of ICL, measured the color profile, and examined the transitionbetween BCG and ICL.

• 대한치과보철학회지
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• 제62권1호
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• pp.47-53
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• 2024

부분 무치악 환자가 임플란트 고정성 보철물 치료를 받은 경우 interproximal contact loss (ICL)은 가장 빈번하게 발생하는 합병증이다. 일반적으로 보고되는 임플란트 보철물의 ICL은 자연치의 이동에 따른 임플란트 보철물과 자연치 사이에서 발생하는 경우가 대부분이다. 임플란트 보철물과 자연치 사이에서 발생하는 ICL의 원인은 여러가지가 있다. 임플란트 보철물 사이에서 발생하는 ICL에 대한 보고는 거의 없으며, 이는 임플란트 보철물과 자연치 사이에서 발생하는 ICL의 원인만으로는 설명하기 어렵다. 본 증례에서는 임플란트 보철물 사이에서 발생하는 ICL을 증례보고하고, 이에 대한 원인 및 대처방법을 논의하고자 한다.

• 노동경제논집
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• 제37권4호
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• pp.89-112
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• 2014

본고는 사회적 형평성과 효율성의 관점에서 직접지원(grant)과 소득연계상환식 학자금융자(ICL)를 결합한 정부의 바람직한 대학교육 지원체계를 이론적으로 제시한다. 교육투자 위험이 큰 경우에는 소득연계상환식 학자금 융자(ICL)가 일반적 학자금 융자에 비해 지원 수혜자의 초기 소득과 관계없이 바람직함을 보인다. 그리고 그 조달 방식이나 운영에 있어서는 민간 자본시장을 통해 위험 프리미엄을 포함하는 대출이자로 조달하는 것보다는 정부에 의한 조세조달 방식이 적정함을 주장한다. 현행 학자금 융자제도가 ICL을 초기 소득 수준별로 선별적으로만 도입하고 있어 개선이 필요하다는 점과 ICL의 현행 조세조달 방식을 정당화하고 있다는 점에서 본고는 일정부분 정책적 함의를 갖는다.

• 천문학회보
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• 제42권1호
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• pp.52.1-52.1
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• 2017

Galaxy clusters are the most massive gravitationally bound systems and thus probably the most recent objects to form. One of promising routes to understand the assembly history of galaxy clusters is to measure observable quantities of components in clusters that are sensitive to the evolutionary state of the cluster. Recent deep observations on the nearby clusters show distinct diffuse intracluster light (ICL), that the light from stars are not bound any individual cluster galaxy, however until now this component has not been well studied due to its faint nature, with typical brightness of ~100 times fainter than the sky background. As shown in galaxy cluster simulation studies, the ICL abundance increases during various dynamical exchanges of galaxies such as the disruption of dwarf galaxies, major mergers between galaxies and the tidal stripping of galaxies. Thus, the ICL is an effective tool to measure the evolutionary stage of galaxy clusters. Moreover, the investigation of the ICL evolution mechanism will allow us understand the galaxy evolution process therein. In this pilot study, we target the Coma cluster, where the existing ICL studies are limited only in the central region. With large and uniform deep optical images from the Subaru telescope, available only recently (Okabe et al. 2014), we are developing a robust ICL measurement technique, extracting the ICL surface brightness and color profiles, which will allow us to study the origin of the ICL and its connection to the evolutionary history of the Coma cluster. For the next phase, we plan to utilize the plenty of spectroscopy data from the MMT telescope to compare ICL properties with the star formation history of the brightest cluster galaxies (BCG), and discuss the ICL formation mechanism of the Coma cluster by comparing the distribution of cluster galaxies with the distribution of diffuse light inside the Coma cluster.

• 생명과학회지
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• 제15권4호
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• pp.542-547
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• 2005

시스플래틴이나 마이토마이신 C (MMC)와 같은 DNA 사슬간 교차결합 (interstrand cross-link ; ICL) 물질에 대해 Brca1 결손세포들이 보이는 높은 감수성은 Brca1 단백질이 세포의 ICL복구반응에 중요한 역할을 담당하고 있음을 암시하고 있다. Brca1 단백질은 재조합 의존성 또는 재조합 비의존성 경로를 통한 DNA 이중사슬 절단(double-strand break ; DSB) 복구에 필수적인 역할을 담당한다. 최근 본인이 속한 연구그룹에서 재조합 의존성 경로를 통한 세포의 ICL복구반응에 Brca1이 관여한다는 것을 밝혀 보고한바 있다. 본 연구에서는 Brca1 단백질의 재조합 비의존성 복구반응에 대한 관여여부를 $p53^{-/-}$와 $p53^{-/-}\;Brcal^{-/-}$ 세포주를 사용하여 연구하였다. 교차결합 복구 실험에서 Brca1 결손 세포주는 Brca1 정상 세포주보다 현저히 낮은 활성을 보였다. 또한, Brca1 결손세포 주의 MMC 에 대한 감수성과 ICL복구능이 Brca1 단백질 발현을 통해 회복되는 것을 확인하였다. 흥미롭게도, Brca1의 11번 엑손 결손세포주 $(Brca1^{\Delta11})$는 높은 MMC저항성과 ICL 복구능을 보였다. 이러한 결과들을 종합하여 볼 때, Brca1 단백질은 ICL복구에 재조합 의존성 경로뿐만 아니라 재조합 비의존성 경로를 통해서도 관여하며, 이러한 활성에는 엑손 11 부분이 아닌 N 말단의 RING 핑거 도메인이나 C 말단의 BRCT도메인이 중요하다는 것을 알 수 있다.

• 천문학회보
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• 제46권1호
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• pp.29.2-29.2
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• 2021

Intracluster light (ICL) is composed of the stars diffused throughout the galaxy cluster but does not bound to any galaxy. The ICL is a ubiquitous feature of galaxy clusters and occupies a significant fraction of the total stellar mass in the cluster. Therefore, the ICL components are believed to help understand the formation and evolution of the clusters. However, in the numerical study, one needs to perform the high-resolution cosmological hydrodynamic simulations, which require an expensive calculation, to trace these low-surface brightness structures (LSB). Here, we introduce the Galaxy Replacement Technique (GRT) that focuses on implementing the gravitational evolution of the diffused ICL structures without the expensive baryonic physics. The GRT reproduces the ICL structures by a multi-resolution cosmological N-body re-simulation using a full merger tree of the cluster from a low-resolution DM-only cosmological simulation and an abundance matching model. Using the GRT, we show the preliminary results about the evolution of the ICL in the on-going simulations for the various clusters.

• The Journal of Advanced Prosthodontics
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• 제11권2호
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• pp.88-94
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• 2019

PURPOSE. This study was conducted to investigate patterns of adjacent tooth displacement in the posterior implant with interproximal contact loss (ICL) by 3-D digital superimposition method. MATERIALS AND METHODS. Posterior partially edentulous patients, restored with implant fixed partial prostheses before 2011 and suffered from food impaction of ICL between 2009 and 2011, were included. Two dental casts, at the time of delivery and at the time of food impaction in a same patient, was converted into 3-D digital models through scanning and superimposition was performed to assess chronologic changes of the dentition. Directions of tooth displacement were evaluated and the amount of ICL was calculated. Correlations between the amount of ICL and elapsed time, or between the amount of ICL and age after function, were assessed at a significance level of P<.05. RESULTS. A total number of 13 patients (8 males, 5 females) with a mean age of $65.76{\pm}9.94years$ and 17 areas (4 maxillae, 13 mandibles) were included in this retrospective study. Teeth adjacent to the implant restoration showed complex displacements but characteristic tendency according to the location of the arch. The mean amount of ICL was $0.33{\pm}0.14mm$. Elapsed time from function to ICL was $61.47{\pm}31.27months$. There were no significant differences between the amount of ICL and elapsed time, or age (P>.05). CONCLUSION. Natural teeth showed various directional movements to result in occlusal change in the arch. The 3-D superimposition of chronologic digital models was a helpful method to analyze the changes of dentition and individual tooth displacement adjacent to implant restoration.