• 분석과학
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• 제8권3호
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• pp.249-258
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• 1995

Polyazine, polyazomethine ( I ) 및 ( II )는 각각 p-benzoquinone과 hydrazine hydrate, p-phenylenediamine, 그리고 diaminomaleonitrile을 dimethylsulfoxide(DMSO)하에서 중합하여 얻었다. Polyazine, polyazomethine ( I ) 및 ( II )의 IR spectra 분석결과 $1600cm^{-1}$ 부근에서 Schiff base의 특성 peak인 -C=N-를 확인하였다. 또한 각 polyazine, polyazomethine ( I ) 및 ( II )를 conc. $H_2SO_4$에 용해시켜 UV/VIS spectrum 측정결과 protonate (>$C\limits^{\small\oplus}=NH-$)에 해당되는 것으로 생각되는 흡수 band가 300nm 부근에서 나타났으며 350~415nm 부근에서 전하이동전이와 같은 흡수로 생각되는 흡수 band가 나타났다. Polyazine, Polyazomethine ( I ) 및 ( II )의 자체 전기전도도는 약 $10^{-14}{\sim}10^{-11}{\Omega}^{-1}cm^{-1}$로 나타났으며 $I_2$를 도핑한 후 최고 전기전도도가 $10^{-2}{\Omega}^{-1}cm^{-1}$ 정도로 약 $10^{12}{\sim}10^9$배 향상되었다.

• 한국재료학회지
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• 제27권4호
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• pp.216-220
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• 2017

The effect of electron beam (EB) irradiation on the electrical properties of Zn-Sn-O (ZTO) thin films fabricated using a sol-gel process was investigated. As the EB dose increased, the saturation mobility of ZTO thin film transistors (TFTs) was found to slightly decrease, and the subthreshold swing and on/off ratio degenerated. X-ray photoelectron spectroscopy analysis of the O 1s core level showed that the relative area of oxygen vacancies ($V_O$) increased from 10.35 to 12.56 % as the EB dose increased from 0 to $7.5{\times}10^{16}electrons/cm^2$. Also, spectroscopic ellipsometry analysis showed that the optical band gap varied from 3.53 to 3.96 eV with increasing EB dose. From the results of the electrical property and XPS analyses of the ZTO TFTs, it was found that the electrical characteristic of the ZTO thin films changed from semiconductor to conductor with increasing EB dose. It is thought that the electrical property change is due to the formation of defect sites like oxygen vacancies.

• Macromolecular Research
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• 제12권3호
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• pp.322-324
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• 2004

Poly(1-dodecyl-2,5-pyrrylene vinylene) (PDPV) has an extended 1t-conjugated structure and exhibits characteristic spectroscopic features. The PDPV we prepared has an absorption maximum at 510nm and its long absorption tail at ca. 750nm in methylene chloride is due to the long 1t-conjugated system connected to vinyl group. The large red-shift of emission was 625nm upon excitation at 480nm, which suggests the existence of a low emissive state. The emission of PDPV in less-polar solvents decreased markedly relative to that in the more-polar solvents; this observation was ascribed possibly to quenching by a strong vibrational mode of the dodecyl groups of PDPV in less-polar solvents. Furthermore, the emission from the high-energy side had a single decay component (0.1㎱, 49.96%), while that from the low-energy side had two components (0.6㎱, 27.1 %; 2.7㎱, 22.87%). We characterized the redox properties of PDPV by cyclic voltammetry. Every redox peak showed irreversible behavior; the oxidation peaks appeared at 1.7,0.8, and 0.6V and the reduction peak at -0.5V.

• 센서학회지
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• 제18권5호
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• pp.365-371
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• 2009

In this study, we have fabricated a fiber-optic pH sensor which is composed of a light source, plastic optical fibers and a spectrometer. As an indicator, a phenol red is used, and a pH liquid solution is prepared by mixing of phenol red and various kinds of pH buffer solutions in these experiments. The emitting light from a light source is guided by plastic optical fibers to the pH liquid solution, and the optical characteristic of a light is changed in the pH liquid solution according to its color change. Therefore, we have measured the intensities and wavelength shifts of the modulated lights, which are changed due to the color variations of phenol red at different pH values, by using of a spectrometer for spectral analysis. Also, the relationships between the pH values of liquid solutions and the optical properties of modulated light according to the change of color of phenol red are obtained.

• 한국재료학회지
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• 제27권6호
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• pp.345-349
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• 2017

The effects of electron beam(EB) irradiation on the electrical and optical properties of InGaZnO(IGZO) thin films fabricated using a sol-gel process were investigated. As the EB dose increased, the electrical characteristic of the IGZO TFTs changed from semiconductor to conductor, and the threshold voltage values shifted to the negative direction. X-ray photoelectron spectroscopy analysis of the O 1s core level showed that the relative area of oxygen vacancies increased from 14.68 to 19.08 % as the EB dose increased from 0 to $1.5{\times}10^{16}electrons/cm^2$. In addition, spectroscopic ellipsometer analysis showed that the optical band gap varied from 3.39 to 3.46 eV with increasing EB dose. From the result of band alignment, it was confirmed that the Fermi level($E_F$) of the sample irradiated with $1.5{\times}10^{16}electrons/cm^2$ was located at the closest position to the conduction band minimum(CBM) due to the increase of electron carrier concentration.

• 한국진공학회지
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• 제9권3호
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• pp.254-257
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• 2000

MBE 법으로 GaAs 기판 위에 성장시킨 $Cd_{1-x}Mg_x/Te$ 박막시료를 조성비(x=0, 0.23, 0.43)에 따라 타원편광 분석기로 측정하여 연구하였다. 기존에 보고된 고상시료(bulk)의 결과와 비교한 결과, 첫째 $E_0$ 밴드갭 에너지 아래에서 나타나는 간섭무늬를 확인할 수 있었고, 이는 박막이 투명함을 보여주는 사실이며 그 결과 이번 시료의 우수성을 확인할 수 있었다. 둘째 $E_2$밴드갭 에너지 영역에서 종전의 고상시료에서 측정 발표된 값보다도 매우 높고 명확한 <$\varepsilon_2$> 값이 측정되어, $E_2$와 $E_0$' 밴드갭 에너지가 명확히 분리되는 것을 보았다. 간섭무늬를 제거하기 위해 다층구조계산(multilayer calculation)을 수행하여 x=0.23일 때의 $E_0$ 밴드갭 에너지를 볼 수 있었다.

• 한국잠사곤충학회지
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• 제53권2호
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• pp.118-123
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• 2015

알코올의 농도 변화에 따른 실크단백질의 구조전이 효과에 대하여 살펴보기 위하여 백옥잠 누에고치를 이용하여 실크단백질 용액을 제조하였다. 알코올의 농도를 100%, 70%, 50%로 조절하여 제조한 실크 비드의 적외선 분광 분석을 하였다. 고농도(100%) 알코올로 처리한 실크단백질은 전형적인 ${\beta}-sheet$ 구조를 반영하는 $1265cm^{-1}$ 부근에서 흡수대를 보였으며 모델 약물로 사용한 4HR의 특성 피크는 관찰되지 않았다. 알코올의 농도를 70%, 50%로 조절하여 처리한 경우에는 모델 약물의 흡수대인 $2933cm^{-1}$ 부근, $1069cm^{-1}$ 부근, 그리고 $973cm^{-1}$ 부근의 흡수대가 발현되었다. 이러한 결과는 알코올의 농도에 따라 조성되는 실크단백질의 미세 구조에 차이가 있음을 나타내며, 보다 정밀한 실크단백질 구조 제어를 위한 추가 연구가 필요한 것으로 생각된다.

• 천문학회지
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• 제29권spc1호
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• pp.63-64
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• 1996

The nature of distant faint blue field galaxies remains a mystery, despite the fact that much attention has been devoted to this subject in the last decade. Galaxy counts, particularly those in the optical and near ultraviolet bandpasses, have been demonstrated to be well in excess of those expected in the 'no-evolution' scenario. This has usually been taken to imply that galaxies were brighter in the past, presumably due to a higher rate of star formation. More recently, redshift surveys of galaxies as faint as B$\~$24 have shown that the mean redshift of faint blue galaxies is lower than that predicted by standard evolutionary models (de-signed to fit the galaxy counts). The galaxy number count data and redshift data suggest that evolutionary effects are most prominent at the faint end of the galaxy luminosity function. While these data constrain the form of evolution of the overall luminosity function, they do not constrain evolution in individual galaxies. We are carrying out a series of observations as part of a long-term program aimed at a better understanding of the nature and amount of luminosity evolution in individual galaxies. Our study uses the luminosity-linewidth relation (Tully-Fisher relation) for disk galaxies as a tool to study luminosity evolution. Several studies of a related nature are being carried out by other groups. A specific experiment to test a 'no-evolution' hypothesis is presented here. We have used the AUTOFIB multifibre spectro-graph on the 4-metre Anglo-Australian Telescope (AAT) and the Rutgers Fabry-Perot imager on the Cerro Tolalo lnteramerican Observatory (CTIO) 4-metre tele-scope to measure the internal kinematics of a representative sample of faint blue field galaxies in the red-shift range z = 0.15-0.4. The emission line profiles of [OII] and [OIII] in a typical sample galaxy are significantly broader than the instrumental resolution (100-120 km $s^{-l}$), and it is possible to make a reliable de-termination of the linewidth. Detailed and realistic simulations based on the properties of nearby, low-luminosity spirals are used to convert the measured linewidth into an estimate of the characteristic rotation speed, making statistical corrections for the effects of inclination, non-uniform distribution of ionized gas, rotation curve shape, finite fibre aperture, etc.. The (corrected) mean characteristic rotation speed for our distant galaxy sample is compared to the mean rotation speed of local galaxies of comparable blue luminosity and colour. The typical galaxy in our distant sample has a B-band luminosity of about 0.25 L$\ast$ and a colour that corresponds to the Sb-Sd/Im range of Hub-ble types. Details of the AUTOFIB fibre spectroscopic study are described by Rix et al. (1996). Follow-up deep near infrared imaging with the 10-metre Keck tele-scope+ NIRC combination and high angular resolution imaging with the Hubble Space Telescope's WFPC2 are being used to determine the structural and orientation parameters of galaxies on an individual basis. This information is being combined with the spatially resolved CTIO Fabry-Perot data to study the internal kinematics of distant galaxies (Ing et al. 1996). The two main questions addressed by these (preliminary studies) are: 1. Do galaxies of a given luminosity and colour have the same characteristic rotation speed in the distant and local Universe? The distant galaxies in our AUTOFIB sample have a mean characteristic rotation speed of $\~$70 km $s^{-l}$ after correction for measurement bias (Fig. 1); this is inconsistent with the characteristic rotation speed of local galaxies of comparable photometric proper-ties (105 km $s^{-l}$) at the > $99\%$ significance level (Fig. 2). A straightforward explanation for this discrepancy is that faint blue galaxies were about 1-1.5 mag brighter (in the B band) at z $\~$ 0.25 than their present-day counterparts. 2. What is the nature of the internal kinematics of faint field galaxies? The linewidths of these faint galaxies appear to be dominated by the global disk rotation. The larger galaxies in our sample are about 2"-.5" in diameter so one can get direct insight into the nature of their internal velocity field from the $\~$ I" seeing CTIO Fabry-Perot data. A montage of Fabry-Perot data is shown in Fig. 3. The linewidths are too large (by. $5\sigma$) to be caused by turbulence in giant HII regions.

• 미생물학회지
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• 제49권2호
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• pp.205-210
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• 2013

루마진 단백질은 발광 세균인 Photobacterium 종에서 추출된 형광성 단백질이다. 형광성을 지닌 최소 크기의 Photobacterium leiognathi 야생형 아미노-말단 도메인 루마진 단백질(N-terminal domain of lumazine protein 118 wt)과 여러 영역에 tryptophan을 생성시킨 돌연변이 단백질들(N-LumP 118 V41W, S48W, T50W, D64W, A66W)을 코드하는 유전자들을 위치 지정 돌연변이(Site Directed Mutagenesis)와 중합효소 연쇄 반응(Polymerase Chain Reaction)을 통해 제조하였다. 위의 유전자들이 포함된 재조합 플라스미드를 대장균에 형질 전환시켜 과발현시키는 최적의 조건을 찾았으며, 발현된 야생형 및 돌연변이 아미노-말단 영역 루마진 단백질을 6X-His tag system을 이용하여 정제 하였다. 흡광 및 형광 분광광도계를 이용한 실험 결과 이들 단백질들은 리간드인 6,7-dimethyl-8-ribityllumazine과 결합하여 형광성을 보유함을 보였다. 따라서 이들은 형광성을 지니게 되는 최소 크기의 루마진 단백질일 뿐만 아니라 형광성을 지닌 아미노산인 tryptophan이 여러 위치에 유일하게 존재함으로써 배향성 및 거리 등의 단백질의 구조 및 결합에 관한 심도 있는 연구에 탐침자로써 유용하게 활용 될 수 있을 것이다.

• Bulletin of the Korean Chemical Society
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• 제21권10호
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• pp.1041-1043
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• 2000

We present the effects of temperature (between 10 K and 298 K) and of hole concentration on the frequency and intensity of characteristic phonons in polycrystalline $La_2CuO_4-related$ compounds using FT-IR spectros-copy. The influences of the concentration of carrier doped on the phonon modes are prominent in the IR spectra of $La_2CuO_4-related$ compounds. For $La_2-xSrxCuO_4({\chi}=$ 0.00, 0.03, 0.07, 0.10, and 0.15) and electrochemically (or chemically) oxidized $La_2CuO_4$, the intensities of the transverse oxygen mode around 680cm $-^1$ which cor-responds mainly to Cu-O(1) stretching vibration in the basal plane of CuO6 octahedron, are decreased and dis-appeared depending on the Sr-substitution rate and the amount of excess oxygen, while the longitudinal oxygen mode around 510 cm $-^1$ corresponding to the Cu-O(2) stretching in the basal plane of CuO6 octahedron are near-ly invariable. In particular, after two cycles of cooling-heating between 10 K and 298 K for these sample, the phonons around 680 cm $-^1$ are blue shif 13-15 cm $-^1$, while the phonons around 510 cm $-^1$ are nearly constant. The introduction of the charge carrier by doping would give rise to the small contraction of CuO6 oc-tahedron as Cu $^3+$ requires a smaller site than Cu $^2+$, which results in the shortening of the Cu-O(1) bond length and Cu-O(2) bond length with the increased La-O(2) bond length. These results in the frequency shift of the characteristic phonons. The IR spectra of $La_2Li0.5Cu0.5O_4$ which exhibits an insulator behavior despite the $Cu^3+$ of nearly 100%, corroborate our IR interpretations. The mode around 710 cm $-^1$ corresponding to Cu-O(1) stretching vibration is still strongly remained even at low temperature (10 K). Thus, we conclude that the con-duction electrons formed within $CuO_2$ planes of $La_2CuO_4-related$ superconductors screen more effectively the transverse oxygen breathing mode around 680 $cm-^1$ depending on the concentration of the doped charge carrier in $La_2CuO_4-related$ compounds, which might use as a superconductivity probe.