• Restorative Dentistry and Endodontics
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• 제24권4호
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• pp.585-603
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• 1999

Esthetic availabilities used as an esthetic restorative maternals can be determined by the optical coincidence among materials, enamel and dentin. Enamel is highly translucent. That's why esthetic materials need to correspond the close translucency of enamel. But the translucent materials are affected by the background color. So it should be predicted that the color of estorative materials depend on the any thickness and the spectral reflectance of the background on which they are placed. The object of this investigation, under above hypothesis, was to determine and analyze how they affect the final color according to the thickness, translucency and background color (white, black and dentin) fill three commercial light cured composite resins(Charisma, Spectrum TPH and Z100). And correlation was analyzed to find out the possibility of the prediction when using the certain background color and thickness of materials. Followings are the result 1. The I shade of CHA showed the lowest contrast ratio($Co_7$) while the B3 shade of Z100 showed the highest contrast ratio(p<0.05). 2. The value of $L^*$ and $b^*$ on the white and dentin background is increased with decreasing thickness. And there are significant relationships between increasing thickness and each value(R>0.085). But there is a little change of $L^*$ and $b^*$ value on the black background regardless of the thickness(p>0.05). 3. For the $a^*$ value, there was little difference in values as a function of thickness and changed irregularly regardless of thickness in all background. 4. The pattern of increasing value of $L^*$ and $b^*$ with decreasing thickness was similar to the group of white and dentin background. In both dentin one showed lesser change of value. 5. The values of $L^*a^*b^*$ measured on the different background with same thickness showed the recognizable color difference(${\Delta}E^*$>2) when the thickness was below 2.6mm. 6. Contrast ratio was increased with increasing thickness with significant relationship (R>0.9). 7. Spectral reflectance of composite resins that calculated from Kubelka-Munk equation was showed little difference compared with observed value w1th decreasing thickness.

• 천문학회보
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• 제41권2호
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• pp.63.3-63.3
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• 2016

We present the two-dimensional distribution of stellar populations in five E+A galaxies from GMOS-N/IFU spectroscopy (GN-2015B-Q-15). Numerical simulations demonstrated that E+A galaxies formed by major mergers contain young stellar populations (e.g. A-type stars) that are centrally-concentrated within scales of 1 kpc. However, several IFU studies reported that A-type stars are widely distributed on ${\gg}$ 1kpc scales. In contrast, Pracy et al. (2013) found a central concentration of A-stars and strong negative Balmer absorption line gradients within 1 kpc scales for local (z < 0.03) E+A galaxies. They claimed that previous studies failed to detect the central concentration because the E+A galaxy samples in previous studies are too far (z ~ 0.1) to resolve the central kpc scales. To verify Pracy et al.'s argument and the expectation from simulations, we selected five E+A galaxies at 0.03 < z < 0.05. Furthermore, we selected the targets in the mid-infrared green valley (Lee et al. 2015). Thanks to good seeing (${\sim}0.4^{{\prime}{\prime}}{\simeq}0.33kpc$) of our observation, we are able to resolve the central 1 kpc region of our targets. We found that all five galaxies have negative Balmer line gradients, but that three galaxies have flatter gradients than those reported in Pracy et al. We discuss the results in relation with galaxy merger history.

• Bulletin of the Korean Chemical Society
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• 제30권10호
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• pp.2403-2407
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• 2009

Second-order rate constants have been measured for two series of nucleophilic displacement reactions, i.e., reactions of 4-nitrophenyl benzoate with Z-substituted phenoxides and those of Y-substituted phenyl benzoates (1a-h) with 4-chlorophenoxide (4-ClPhO–) in 80 mol% $H_2O$/20 mol% DMSO at 25.0 ${\pm}\;0.1\;{^{\circ}C}$. The Br$\phi$nsted-type plot for reactions of 4-nitrophenyl benzoate with Z-substituted phenoxides exhibits an excellent linear correlation with ${\beta}_{nuc}$ = 0.72. Reactions of 1a-h with 4-chlorophenoxide result in also a linear Br$\phi$nsted-type plot with ${\beta}_{lg}$ = –0.62, a typical ${\beta}_{lg}$ value for a concerted mechanism. The Hammett plots correlated with ${\sigma}^o\;and\;{\sigma}^-$ constants show many scattered points for reactions of 1a-h with 4-chlorophenoxide. In contrast, the corresponding Yukawa-Tsuno plot exhibits an excellent linear correlation with $\rho_Y$ = 2.26 and r = 0.53, indicating that expulsion of the leaving group occurs at the rate-determining step (RDS) either in a concerted mechanism or in a stepwise pathway. However, a stepwise mechanism with leaving group departure being the RDS is excluded since the leaving Y-substituted phenoxide is less basic and a better nucleofuge than the incoming 4-ClPh$O^-$. Thus, the reactions have been concluded to proceed through a concerted mechanism, in which bond formation between the nucleophile and electrophilic center is more advanced than expulsion of the leaving group in the transition state on the basis of the magnitude of ${\beta}_{nuc}\;and\;{\beta}_{lg}$ values.

• 천문학회보
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• 제44권1호
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• pp.38.4-38.4
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• 2019

Ultra-diffuse galaxies (UDGs) are intriguing in the sense that they are much larger than dwarf galaxies but have much lower surface brightness than normal galaxies. To date, UDGs have been found only in the local universe. Taking advantage of deep and high-resolution HST images, we search for UDGs in massive galaxy clusters in the distant universe. In this work, we present our search results of UDGs in three massive clusters of the Hubble Frontier Fields: Abell 2744 (z=0.308), Abell S1063 (z=0.348), and Abell 370 (z=0.375). These clusters are the most distant and massive among the host systems of known UDGs. The color-magnitude diagrams of these clusters show that UDGs are mainly located in the faint end of the red sequence. This means that most UDGs in these clusters consist of old stars. Interestingly, we found a few blue UDGs, which implies that they had recent star formation. The radial number densities of UDGs clearly decrease in the central region of the clusters in contrast to those of bright galaxies which keep rising. This implies that a large fraction of UDGs in the central region were tidally disrupted. These features are consistent with those of UDGs in nearby galaxy clusters. We estimate the total number of UDGs (N(UDG)) in each cluster. The abundance of UDGs shows a tight relation with the virial masses (M_200) of thier host systems: M_200 \propto N(UDG)^(1.01+/-0.05). This slope is found to be very close to one, indicating that efficiency of UDGs does not significantly depend on the host environments. Furthermore, estimation of dynamical masses of UDGs indicates that most UDGs have dwarf-like masses (M_200 < 10^11 M_Sun), but a few UDGs have $L{\ast}$-like masses (M_200 > 10^11 M_Sun). In summary, UDGs in distant massive clusters are found to be similar to those in the local universe.

• 감성과학
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• 제16권3호
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• pp.373-386
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• 2013

본 연구에서는 이미지 감상자가 선호하는 화질의 객관적 평가 항목들의 범위를 구체화하고 실제 이미지를 기반으로 화질의 선호도를 측정하는 방식을 따랐다. 즉, 무기준법(No-Reference)을 기반으로 하고 화질 평가 요소를 다이내믹 레인지, 컬러, 콘트라스트로 규정하였다. 샘플 사진 수집은 인터넷 갤러리에서 추천수 30회 이상을 기준으로 감상자들이 선호하는 풍경사진 200장의 이미지를 선정하였다. 그리고 세 가지 객관적 화질 평가 항목에 의한 정규분포분석을 통하여 총점을 백점 기준으로 환산하여 최종적으로 예상되는 화질의 선호도를 측정하였다. 본 실험에서 적용한 실제 사진 샘플의 다이내믹 레인지 측정값은 10 stop, LAB 평균은 L:54.7, A:2.96, B:-15.84, RSC 콘트라스트는 376.9로 나타났다. 총 200장 샘플 사진의 정규분포 z값은 다이내믹 레인지가 0.21, LAB 평균이 LAB 평균이 L:0.15, A:0.38, B:0.13, RSC 콘트라스트가 0.08을 나타냈다. 표준정규분포 표에서 위의 z값이 나타날 확률을 상위 백분율로 나타내면 실제 사진 샘플의 다이내믹 레인지는 8.32%, LAB 평균은 LAB 평균은 L:5.96%, A:14.8%, B:5.17%, RSC 콘트라스트는 3.19%를 나타낸다. 즉 화질 평가 모형에 사용된 실제 사진 샘플의 상위 백분율을 100점으로 환산한 다이내믹 레인지는 91.68점, LAB 평균은 91.36점, RSC 콘트라스트는 96.81점이다. 따라서 세 가지 객관적 화질 평가 항목에 의한 총점의 평균은 94.99점으로 나타낼 수 있었다. 즉 본 연구에서 제안한 화질 측정 모형을 통하여 실제 사진 샘플에 대한 선호도를 수치적으로 측정할 수 있었다. 이와 같은 연구를 통하여 이미지 감상자가 선호하는 화질의 재현 성능 범위를 구체화하고 예상되는 화질의 선호도를 수치화하는 실용적인 연구 결과를 제안하였다.

• 한국응용곤충학회지
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• 제59권1호
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• pp.15-22
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• 2020

국내에 호박을 가해하는 두 과실파리는 Zeugodacus 속으로 분류된다. 호박꽃과실파리(Z. scutellata) 수컷은 큐루어(Cuelure)에 유인되어 포장에서 이 과실파리의 발생을 모니터링 하는 데 이용된다. 이에 반해, 호박과실파리(Z. depressa) 수컷을 유인하는 물질은 아직 알려지지 않았다. 단백질 먹이 유인제가 대부분의 과실파리를 유인하게 되는데 여기에 terpinyl acetate (TA)를 추가하여 호박과실파리의 유인력을 높였다. 본 연구는 TA-단백질먹이 유인제를 이용하여 호박 재배지에서 호박과실파리의 연중 발생을 모니터링 하는 데 목적을 두었다. TA-단백질먹이 유인제의 효율성을 증명하기 위해 호박꽃과실파리를 대상으로 큐루어와 TA-단백질먹이 유인제를 이용하여 2019년 한 해 동안 발생을 모니터링하고 이 두 유인제로 얻어진 연중 모니터링 자료를 비교하였다. 두 유인제를 이용한 호박꽃과실파리의 연중 발생 패턴은 10월 하순을 제외하면 유사하였다. TA-단백질먹이 유인제는 10월 하순 시기에도 지속적인 호박꽃과실파리의 포획을 보였는데 이는 9월 하순 이후 호박꽃과실파리의 성충 휴면 유기에 따른 유인 행동 차이로 이해되고 있다. TA-단백질먹이 유인제를 이용한 호박과실파리의 연중 모니터링은 크게 두 개의 발생 최성기를 보여 하나는 7월 중순이고 다른 하나는 8~9월에 나타나며 포획된 개체들의 80% 이상이 암컷이었다. 이러한 TA-단백질먹이 유인제의 두 과실파리류에 대한 유인 효과를 바탕으로 스피노사드(spinosad) 살충제를 가미한 수화제를 제조하고 호박 재배지에 살포하였다. 처리 7 일경과 후 약 70% 이상의 방제 효과를 기록하였다. 그러나 이 방제 효과는 처리 이후 기간이 경과하면서 낮아지는 경향을 나타냈다. 이상의 결과는 TA-단백질먹이 유인제를 이용하여 야외 호박 재배지에서 호박과실파리의 연중 모니터링이 가능하다는 것을 보여 주었다. 또한 스피노사드를 가미한 TA-단백질먹이 유살제가 이들 호박과실파리류 방제에 응용될 수 있다는 것을 제시하고 있다.

• 한국측량학회:학술대회논문집
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• 한국측량학회 2004년도 춘계학술발표회논문집
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• pp.239-243
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• 2004

It does not exist almost that Most satellite image has both high spectral and spatial resolution. In order to apply the satellite image for to be actual, we need numerical and analytical technique development to improve the resolution. Specially in the function of solid illustration, we represent the solid image through the image generation to solid screen. The main function includes magnification, reduction, screen center movement, Panning, territory magnification. The method to process the image includes histogram and contrast modulation. Afterwards, we will develop the function includes 3-dimension cursor to control the elevation position and calculate the ground coordination automatically. There is the layer control includes the representation and the edition of 3D vector, extraction the Z value by On the Ground and digital elevation.

• 한국음향학회:학술대회논문집
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• 한국음향학회 1999년도 학술발표대회 논문집 제18권 2호
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• pp.355-360
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• 1999

이 연구는 폴란드어의 음성. 음운 체계를 조음 음성학에 기초를 두어 살펴보고, 한국어의 음성. 음운과 대조한다 모음은 한국어가 많고, 자음은 폴란드어가 더 많다. 한국인이 구별하기 힘든 모음 /i/와 /y/의 차이점과 슬라브어에서 유일하게 폴란드어에만 있는 비모음을 알아보고, 한국어에 없는 자음 $/\'{3}/$와, 중설연구개음 $/\'{k},\;\'{g},\;\'{s},\;\'{z},\;\'{c},\;\'{3},\;\'{n}/$과 기본적으로 자음에서 일어나는 음운 규칙들을 살펴본다. 모음 변화는 형태론과 연관지어 살펴보아야 하므로 여기에서는 제외한다. 폴란드어와 한국어의 음성. 음운 대조는 첫째, 모음과 자음 분절음의 대조, 둘째, 음운 현상의 대조, 셋째, 음절구조상의 대조로 분류하고, 분절음의 대조에 초점을 두고 조음표상에 대조를 이음과 함께 표시한다.

• 한국정보디스플레이학회:학술대회논문집
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• 한국정보디스플레이학회 2008년도 International Meeting on Information Display
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• pp.388-391
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• 2008

A new reset waveform with negative ramp pulse was proposed. Comparative experiments between the negative and positive waveforms were performed. During reset period, IR distributions and luminance of black and white conditions were measured with the 42-inch XGA PDP module. The negative waveform improved contrast ratio about 15.4 ~ 22.5 % than the positive waveform by lowing the black luminance in reset period. Z bias (= Vbb) of the positive waveform was 27 V higher than the negative waveform.

• 한국소성가공학회:학술대회논문집
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• 한국소성가공학회 2002년도 금형가공 심포지엄
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• pp.225-230
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• 2002

As in most metal forming processes, die and lubrication are of vital importance in hydrostatic extrusion. An efficient die design and lubrication system selection reduce the pressure required for a given reduction ratio by lowering friction at the billet-die interface. In contrast to the conventional macroscopic extrusion, fine-wire fabrication requires higher extrusion pressure and effect of friction is much more significant. Forming fine Au, Ag, and Cu wire with hydrostatic extrusion process in cold condition, the effect of extrusion die angle, lubrication and billet's initial diameter was studied.