• 대한화학회지
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• 제30권2호
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• pp.216-223
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• 1986

Dansyl 유도화된 아미노산의 광학이성질체를 분리하기 위해 광학활성인 L-arginine과 몇가지 금속(구리, 아연, 카드뮴, 니켈)의 킬레이트를 이동상에 첨가하여 역상 칼럼내에서 분리를 시도했다. 구리 킬레이트 이외의 것은 광학이성질체의 분리가 안되었다. 아미노산의 광학이성질체의 분리 거동은 이동상의 pH 및 유기용매조성, 완충용액의 종류와 농도, 금속의 종류와 킬레이트 농도에 의해 영향을 받음을 알 수 있었다. Valine, metionine, leucine, phenylalanine은 D형이 먼저 용리되고 serine과 alanine은 L형이 먼저 용리되었으며 threonine은 D형과 L형의 분리현상이 나타나지 않았다. 이러한 분리거동은 리간드 교환반응에 의한 (D, L-DNS-AA) (M) (L-Arg) 3종류 착물이 형성될때의 입체 특이성효과로써 설명할 수 있다.

• 대한화학회지
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• 제22권6호
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• pp.386-395
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• 1978

여러 농도와 온도에서 Poly(trans-5-methyl-L-proline)을 trifluoroethanol 용매에서 정방향 변광회전, trifluoroethanol-n-butanol (1 : 4) 용매에서 역방향 변광회전을 시키면서 변광회전속도를 측정하였다. 이 두 방향의 변광회전 현상은 폴리머농도에 대하여 1차 반응이었다. 활성화에너지를 측정하기 위하여 변형된 Arrhenius식을 유도하였는데 이식은 물리적 성질과 농도와의 관계나 반응차수가 불확실한 반응에 이용할 수 있다. 정방향과 역방향 변광회전의 활성화에너지는 잔기몰당 각기 32.5와 33.5kcal이었고 이값은 polyproline 변광회전의 활성화에너지 (아미드결합의 공명에너지)보다 잔기몰당 10kcal가 높다. 이 과량의 활성화에너지는 폴리머아미드 결합이 시스-트란스 이성질화현상이 일어날 때 카르보닐기와 메틸기 사이에 생기는 입체장애에 의한 것이다.

• Journal of Microbiology and Biotechnology
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• 제19권1호
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• pp.65-71
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• 2009

Microbial oxidoreductive systems have been widely used in asymmetric syntheses of optically active alcohols. However, when reused in multi-batch reaction, the catalytic efficiency and sustainability of non-growing cells usually decreased because of continuous consumption of required cofactors during the reaction process. A novel method for NADPH regeneration in cells was proposed by using pentose metabolism in microorganisms. Addition of D-xylose, L-arabinose, or D-ribose to the reaction significantly improved the conversion efficiency of deracemization of racemic 1-phenyl-1,2-ethanediol to (S)-isomer by Candida parapsilosis cells already used once, which afforded the product with high optical purity over 97%e.e. in high yield over 85% under an increased substrate concentration of 15 g/l. Compared with reactions without xylose, xylose added to multi-batch reactions had no influence on the activity of the enzyme catalyzing the key step in deracemization, but performed a promoting effect on the recovery of the metabolic activity of the non-growing cells with its consumption in each batch. The detection of activities of xylose reductase and xylitol dehydrogenase from cell-free extract of C. parapsilosis made xylose metabolism feasible in cells, and the depression of the pentose phosphate pathway inhibitor to this reaction further indicated that xylose facilitated the NADPH-required deracemization through the pentose phosphate pathway in C. parapsilosis. moreover, by investigating the cofactor pool, the xylose addition in reaction batches giving more NADPH, compared with those without xylose, suggested that the higher catalytic efficiency and sustainability of C. parapsilosis non-growing cells had resulted from xylose metabolism recycling NADPH for the deracemization.

• 천문학회지
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• 제36권3호
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• pp.167-175
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• 2003

There is accumulating evidence for a strong link between nuclear starbursts and AGN. Molecular gas in the central regions of galaxies plays a critical role in fueling nuclear starburst activity and feeding central AGN. The dense molecular ISM is accreted to the nuclear regions by stellar bars and galactic interactions. Here we describe recent observational results for the OB star forming regions in M51 and the nuclear star burst in Arp 220 - both of which have approximately the same rate of star formation per unit mass of ISM. We suggest that the maximum efficiency for forming young stars is an Eddington-like limit imposed by the radiation pressure of newly formed stars acting on the interstellar dust. This limit corresponds to approximately 500 $L_{\bigodot} / M_{\bigodot}$ for optically thick regions in which the radiation has been degraded to the NIR. Interestingly, we note that some of the same considerations can be important in AGN where the source of fuel is provided by stellar evolution mass-loss or ISM accretion. Most of the stellar mass-loss occurs from evolving red giant stars and whether their mass-loss can be accreted to a central AGN or not depends on the radiative opacity of the mass-loss material. The latter depends on whether the dust survives or is sublimated (due to radiative heating). This, in turn, is determined by the AGN luminosity and the distance of the mass-loss stars from the AGN. Several AGN phenomena such as the broad emission and absorption lines may arise in this stellar mass-loss material. The same radiation pressure limit to the accretion may arise if the AGN fuel is from the ISM since the ISM dust-to-gas ratio is the same as that of stellar mass-loss.

• 대한방사선기술학회지:방사선기술과학
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• 제42권1호
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• pp.47-51
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• 2019

This study was conducted from July 1 to September 30, 2018 using Optically Stimulated Luminescence Dosimeter(OSLD) and photoluminescent glass dosimeter(PLD) to measure the 3-month exposure dose and the cumulative dose in the active working area of the nuclear medicine worker Respectively. As a result, the cumulative dose for three months in the worker and work area was measured as 1.97 mSv and 2.02 mSv in the PLD. The mean surface dose and the mean depth dose of the OSLD were measured to be 2.04 mSv. The difference in the total surface dose measured by the PLD and the OSLD was 0.66mSv and the total mean surface dose was 0.07mSv. The difference between the total depth dose and the total depth dose was 0.1mSv and 0.02mSv, respectively. It was found that the dose value of the OSLD was higher than that of the PLD. In addition, it was found that the maximum difference of 0.01mSv was observed between the PLD and the OSLD of the worker. For the dose measurement of the two dosimetry systems, there was no significant difference between the PLD and the OSLD in the surface dose of 0.239 (p>0.05). Also, the significance of PLD and OSLD in the deep dose was 0.109, which was not statistically significant (p>0.05).

• Bulletin of the Korean Chemical Society
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• 제13권3호
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• pp.268-274
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• 1992

An attempt to improve the second harmonic generation (SHG) efficiency of MAP (methyl (2,4-dinitrophenyl)aminopropanoate) by modifying the substituents on the amino group of MAP is described. Several MAP analogues have been prepared using optically active amino acids alanine, phenylalanine and serine, and their SHG efficiencies measured. None of the MAP analogues exhibited SHG efficiencies as high as that of MAP. X-ray crystal structures of three MAP analogues have been determined. In the crystal structures of two of them, which were the derivatives of phenylalanine, two crystallographically-independent molecules existing in the asymmetric unit are aligned almost antiparallel. These structures are consistent with the very low SHG efficiencies of these compounds. On the other hand, the crystal structure of a serine derivative reveals substantial alignment of the dinitroaniline chromophore along the polar axis. However, the angle of 86.2° between the molecular charge tranfer axis and the polar axis of the crystal is still far away from the optimum value of 54.74° for the phase-matchable SHG. The structure is consistent with the SHG efficiency of this compound which is much higher than those of the phenylalanine derivatives but still lower than that of MAP. This study demonstrates the importance of the orientation of molecules in the crystal lattice in determining secod-order nonlinear optical properties of crystalline materials.

• 천문학논총
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• 제36권3호
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• pp.47-63
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• 2021

와이즈/네오와이즈 자료를 사용하여 1형 활동은하핵의 근적외선 장기 변광 특성을 살펴보았다. 활동은하핵은 밀리퀘이사 목록을 사용해 가시광에서의 등급 제한을 두어 선정하였고, 여러 번의 다중시점 측광 자료를 확보하기 위해 황도북극과 황도남극에 가까운 대상으로 한정하였다. 이후 와이즈와 네오와이즈 데이터베이스에서 해당 대상들의 측광 자료를 추출하였다. 일부 근적외선에서 검출되지 않은 경우와 관측 횟수가 지나치게 적은 경우를 제외하고 총 73개의 1형 퀘이사 및 활동은 하핵, 140개의 측광학적으로 선택된 활동은하핵 후보에 대해 W1 (3.4 ㎛), W2 (4.6 ㎛) 밴드 광도곡선을 구성하고 이를 이용해 변광 분석을 수행하였다. 변광 여부를 판단하기 위해 초과 분산 값과 변광의 유의확률 P_var를 계산하였다. 초과 분산이 포아송 오차에 의해 추정되는 오차값보다 큰 경우, 그리고 P_var이 0.95보다 크거나 같은 경우를 변광으로 판단했는데, 활동은하핵 73개 중 19개, 활동은하핵 후보 140개 중 12개가 W1, W2 밴드 모두에서 변광 대상으로 판단되었다. W1 밴드보다 W2 밴드에서 변광 대상으로 판단되는 숫자가 작게 나타났는데, 이는 긴 파장으로 갈수록 변광의 정도가 작아짐을 시사하는 것으로 보인다. 약 9 ~ 26%의 대상들이 근적외선 변광을 보였다. 감쇠 랜덤워크 모형을 사용하여 변광 폭(σ)과 완화 시간(τ), W1과 W2 밴드 사이의 시간 지연 등을 추정하였다. 변광 폭 및 완화시간은 W1 등급과 큰 상관관계를 보이지 않았으며, 두 변수 사이에도 특별히 두드러지는 상관관계가 나타나지 않았다. 단, 감쇠 랜덤워크 모형을 사용해서 시간 규모를 추정할 때 광도곡선의 분량이 충분한지를 감안하면, 완화시간이 짧은 대상들에 대해서는 변광 폭과 완화시간이 음의 상관관계를 보인다고도 볼 수 있다. 대상의 개수가 통계적으로 유의미한 결과를 제시하기에는 부족하다. X선 광도와 변광 특성을 비교했을 때에는 상관관계를 찾아보기 어려웠으나, 앞으로 얻어질 X선 탐사자료와 전천 스펙트럼 탐사자료와 결합한 추가 연구가 기대된다. 전체 대상 중에서는 시간에 따라 (W1-W2) 색이 변하는 것으로 판단되는 흥미로운 대상이 4개가 존재했는데, 이들의 특성에 대해서는 추후 연구가 더 필요할 것으로 전망한다.

• 대한화학회지
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• 제55권3호
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• pp.502-508
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• 2011

[ $Nd_{2x}Cd_{2-3x}SiO_4$ ]($0.01{\leq}x{\leq}0.21$) [S1-S3: x=0.01, 0.11 and 0.21] 고용체를 졸-겔 방법을 통해 합성하였다. X선 분말회절(XRD) 측정은 $P2_1$/m 공간군의 단사정계를 보여준다. 평균 결정 크기는 20-45 nm이다. 주사전자현미경(SEM)으로 살펴본 모양은 구형의 특성을 보인다. 에너지 분산 X 선 분광기(EDS) 결과로부터 모든 구성 원소의 존재를 확인하였다. ~750 nm에서의 흡수 밴드는 $Nd^{3+}$ 이온의 $^4I_{9/2}{\rightarrow}^4F_{7/2}+^4S_{3/2}$ 전이에 기인한다. 10, 40, 77, 300 K에서 S1-S3의 전자 상자성 공명 (EPR) 선모양은 $Nd^{3+}$ 이온의 빠른 스핀 격자 이완에 기인하는 폭이 넓은 구분되지 않은 등방성의 선모양을 보여준다.

• 한국전기전자재료학회:학술대회논문집
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• 한국전기전자재료학회 2009년도 하계학술대회 논문집
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• pp.151-151
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• 2009

Recently, there has been increasing interest in amorphous oxide semiconductors to find alternative materials for an amorphous silicon or organic semiconductor layer as a channel in thin film transistors(TFTs) for transparent electronic devices owing to their high mobility and low photo-sensitivity. The fabriction of amorphous oxide-based TFTs at room temperature on plastic substrates is a key technology to realize transparent flexible electronics. Amorphous oxides allows for controllable conductivity, which permits it to be used both as a transparent semiconductor or conductor, and so to be used both as active and source/drain layers in TFTs. One of the materials that is being responsible for this revolution in the electronics is indium-zinc-tin oxide(IZTO). Since this is relatively new material, it is important to study the properties of room-temperature deposited IZTO thin films and exploration in a possible integration of the material in flexible TFT devices. In this research, we deposited IZTO thin films on polyethylene naphthalate substrate at room temperature by using magnetron sputtering system and investigated their properties. Furthermore, we revealed the fabrication and characteristics of top-gate-type transparent TFTs with IZTO layers, seen in Fig. 1. The experimental results show that by varying the oxygen flow rate during deposition, it can be prepared the IZTO thin films of two-types; One a conductive film that exhibits a resistivity of $2\times10^{-4}$ ohm${\cdot}$cm; the other, semiconductor film with a resistivity of 9 ohm${\cdot}$cm. The TFT devices with IZTO layers are optically transparent in visible region and operate in enhancement mode. The threshold voltage, field effect mobility, on-off current ratio, and sub-threshold slope of the TFT are -0.5 V, $7.2\;cm^2/Vs$, $\sim10^7$ and 0.2 V/decade, respectively. These results will contribute to applications of select TFT to transparent flexible electronics.

• 한국근적외분광분석학회:학술대회논문집
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• 한국근적외분광분석학회 2001년도 NIR-2001
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• pp.1527-1527
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• 2001

Glucose, fructose and sucrose being the main sugars that can be found in natural fruit juice. Many instrumental methods, such as GC, LC, electrochemical or spectrometric methods provide information about both the total content of sugars and the specific concentration of each carbohydrate[1]. The simplicity of sample handling and measurement in the near IR(NIR) wavelength region, which allows the use of long pathlength, optical glass cells and optical fibers, makes NIR a good alternative for sugar determination [2]. In the present study, six varieties of persian grapes were harvested at intervals through august to october and analysed for sugars by NIR. The results were processed by principal component regression (PCR) and partial least squares (PLS) analysis. Sample juice was prepared by squeezing through gauze from crashed grape. This solution was treated by zinc ferrocyanide prior to analysis in order to eliminate colored compounds and all optically active nonsugar substances. For glucose and fructose the most characteristic wavelengths were 1456nm corresponding to the first harmonic O-H stretching and the second at 2062nm corresponding to O-H stretching and deformation; secondary characteristic combination bands were also seen at 2265 nm (O-H and C-C stretching) and at 2240 nm (C-H and C-C stretching). However these spectra were taken over a wavelength range from 1100-2500nm at room temperature of 25-$30^{\circ}C$. To test the accuracy of the described procedure, samples of six varieties of grape were analysed by the proposed NIR and a standard method[2]. Good agreement were found between these two sets of the results. To perform the recovery studies , samples of grape juices previously analysed by the proposed method, were spiked with known amounts of each individual sugars and then analysed again. Relative standard deviations varied from 1.4 to 1.8% for six independent measurements of individual and total sugar concentration. In the analysis of real and synthetic samples, precise and accurate results were obtained , providing accuracy errors lower than 1.9% in all cases. Average recoveries of ${97}{\pm}{4%}$ for total sugar and between ${95}{\pm}{5%}$ and ${99}{\pm}{2%}$ for sing1e sugars demonstrate the applicability of the methodology developed to the direct analysis of grape Juice.