• 한국식품저장유통학회지
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• 제6권4호
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• pp.411-416
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• 1999

닭고기에 감마선 3, 7 kGy를 조사한 후 저장 기간 및 온도에 따라 육색변화, 단백질 분해, TBA가, 산가, 휘발성 염기태 질소 등을 측정였다. 육색변화에서 조사직후 조사선량에 관계없이 저장기간의 경과에 따라 metmyoglobin은 함량이 다소 증가되는 경향이었고 냉동저장에서는 조사에 따른 영향없이 저장기간에따라 점차 감소하는 경향이었다. 전기영동 결과는 감마선조사군과 비조사군 사이의 변화는 거의 없었으며, 저장기간에따라 약 105 kDa의 단백질 subunit 가 분해되기 시작하여 8주후에는 완전소실 되었고, 특히 약 32 kDa에서 40 kDa의 분자량을 가진 단백질 subunit의 경우 모든 시험군에서 저장기간에 따라 서서히 분해되면서 소실되거나 두개의 분획으로 분리 되어 새로운 band를 형성하였다. 한편, TBA가의 경우 냉장, 냉동 저장시료 모두 저장기간 및 감마선 조사 선량의 증가에 따라 크게 증가하였고 산가는 조사선량의 증가에 따라서는 오히려 감소하였다. VBN함량 변화의 경우에는 냉장 저장 8주후의 비조사 시료는 7 kDy조사 시료에 비해 약 4배의 증가를 나타내었다.

• Nuclear Engineering and Technology
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• 제54권3호
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• pp.1062-1070
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• 2022

In the present communication, pure and stable α-Bismuth Oxide (Bi₂O₃) nanoparticles (NPs) were synthesized by low temperature solution combustion method using urea as a fuel and calcined at 500℃. The synthesized sample was characterized by using powder X-ray Diffraction (PXRD), Scanning Electron Microscopy (SEM), Energy dispersive X-ray analysis (EDAX), Transmission Electron Microscopy (TEM), Fourier Transform Infrared Spectroscopy (FTIR) and UV-Visible absorption spectroscopy. The PXRD pattern confirms the formation of mono-clinic, stable and low temperature phase α-Bi₂O₃. The direct optical energy band gap was estimated by using Wood and Tauc's relation which was found to be 2.81 eV. The characterized sample was studied for X-ray/gamma ray shielding properties in the energy range 0.081-1.332 MeV using NaI (Tl) detector and multi channel analyzer (MCA). The measured shielding parameters agrees well with the theory, whereas, slight deviation up to 20% is observed below 356 keV. This deviation is mainly due to the influence of atomic size of the target medium. Furthermore an accurate theory is necessary to explain the interaction of X-ray/gamma ray with the NPs.The present work opens new window to use this facile, economical, efficient, low temperature method to synthesize nanomaterials for X-ray/gamma ray shielding purpose.

• 생약학회지
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• 제37권4호
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• pp.221-228
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• 2006

A lectin was purified from Serrognathus platymelus castanicolor larvae and named as SPL. The purification was carried out by ion-exchange chromatography on DEAE Sephadex A-50 and gel filtration chromatography on Sephadex G-200. The purity of the protein was verified by polyacrylamide gel electrophoresis and the purified lectin agglutinated erythrocytes of rabbit and human A, B, O, AB. SPL was tested it's ability to enhance the expressions of cytokines, $IL-1\alpha$, IL-2, IL-6, $TNF\alpha$ and $IFN\gamma$ by human peripheral blood mononuclear cells (PBMC) obtained from healthy donors. mRNA analyses were performed by RT-PCR at the moment of 1, 4, 8, 24, 48, 72 and 96 h after stimulation of PBMC with purified SPL. The patterns of IL-2 band were slightly expressed from 24 h and the strongest band was appeared at 96 h. The expressions of $IL-1\alpha$ and IL-6 mRNA were strong from 1 to 8 h and those of $TNF\alpha$ were from 48 to 96 h. The mRNA encoding $IFN\gamma$ were not detected. The addition of SPL for macrophage cultures induced production of nitric oxide (NO) by cells in a dose-dependent manner. NO release was partially inhibited by $TNF\alpha$ antibodies. These results suggest that SPL has the ability to enhance cytokine expressions in PBMC and to induce the NO release by TNFa in macrophage cultures from PBMC cultures.

• 한국진공학회지
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• 제6권3호
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• pp.249-254
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• 1997

Fe가 첨가된 반절연성 InP(100)의 특성을 photoreflectance(R) 측정으로 조사하였다. 관측한 PR 신호로부터 300K에서 띠간격 에너지($E_o$)와 넓어지기 변수(broadening parameter:$\Gamma$)는 각각 1.336eV 및 11.2meV의 값을 얻었다. 측정온도를 300~80K로 낮춤에 따라 PR 신호는 엑시톤과 2차원의 띠사이 전이가 중첩된 형태(300K)에서 전형적인 엑시톤 에 의한 전이형태(80K)로 변함을 알았다. 또한 Varshni 계수 $\alpha=-0.94\pm$0.07meV/K, $\beta=587\pm$35.2K와 Bose-Einstein 계수 aB=33.6$\pm$2.02meV, $\theta=165\pm$33K의 값을 얻었다. 그리고 등온 및 등시 열처리를 수행한 후 측정 결과, 온도 $300^{\circ}C$에서 10~20분 정도 열처리시켰을 때 InP 시료의 결정성이 가장 좋아짐을 정성적으로 알 수 있었다.

• 한국재료학회지
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• 제15권8호
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• pp.508-513
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• 2005

[ $TiO_2-Fe_2O_3$ ] nanocomposite powders for magnetic photocatalyst were synthesized by sol-gel process, in which $TiO_2$ photocatalytic layer was formed on the surface of $\gamma-Fe_2O_3$ magnetic core. Transmission electron microscopy (TEM) observation and X-ray diffractometry (XRD) analysis revealed that$\gamma-Fe_2O_3$ nanoparticles, $10\~20nm$ in diameter, were coated by $TiO_2$ shell of 5nm in thickness and $TiO_2$ was anatase phase. Also hydroxyl group (-OH) used to decompose organic compounds was detected by Fourier transformation infrared spectrometry(FT-IR) analysis. UV-Visible spectrophotometry results showed that light absorption occurred in the wavelength range of $400\~700 nm$, and the band gap energy $(E_g)$ of powder was 1.8 eV. Finally it was found that the coercivity $(H({ci})$ and saturation magnetization $(M_s)$ of the powder were 79 Oe and 14.8 emu/g, respectively as experimental vibrating sample magnetometer (VSM) measurements.

• Tuberculosis and Respiratory Diseases
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• 제47권3호
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• pp.347-355
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• 1999

배경: Phospholipase C(PLC)는 세포의 성장, 분화, 변형(transformation)과 관련된 세포내 신호 전달과정에 중추적인 역할을 하는 효소이다. 이들 중 PLC-$\gamma$는 tyrosine kinase의 인산화에 의해 주로 활성화되는 데, 최근에 phosphatidic acid(PA), phosphatidy-linositol 3, 4, 5-trisphosphate($PIP_3$), tau 단백에 의한 활성화 기전이 밝혀진 바 있다. 특히 tau 단백은 bovine brain에서 arachidonic acid와 함께 PLC-$\gamma$를 활성화시키는 것으로 알려져 PLC-$\gamma$와 $PLA_2$ 사이의 cross-talk이 이루어질 가능성이 제시되고 있다. 최근 보고에 의하면 tau 단백과 같은 기전으로 PLC-${\gamma}1$ 활성화시키는 단백이 bovine lung에서 발견되었고, 이 활성화 단백을 정제 및 클론하여 AHNAK 단백임이 확인된 바 있다. 또한 PLC-${\gamma}1$이 유방암, 대장암, 위암 등에서 증가되어 있어 발암 과정과 연관되어 있음이 보고되어 왔으나 PLC-${\gamma}1$의 활성화 단백인 AHNAK 단백에 대해서는 질병과 관련되어 연구된 것이 아직 없는 실정이며 저자 등은 폐암 조직과 정상 폐조직에서 AHNAK 단백의 발현 양상을 연구하여 폐암의 발암과정에 AHNAK 단백이 관여함을 밝히고자 하였다. 대상 및 방법: 아주대학교 병원에 내원하여 폐암으로 수술을 받은 환자의 폐암 조직과 동일 환자의 정상 폐조직에서 AHNAK 단백의 발현양상을 western blot 분석과 면역조직화학적 염색방법을 통하여 조사하였다. 결과: 14예의 편평상피암 세포조직 중 8예 (57.1 %)와 14예의 선암 세포조직 모두에서 정상 대조군에 비해 AHNAK 단백의 발현이 증가하였고, 70 kDa~200kDa의 여러가지 분자량을 가지는 띠모양으로 나타났다. 면역조직화학적 염색에서도 정상 폐조직보다 폐암 조직내에서 강한 발색반응을 보였다. 결론: PLC-${\gamma}1$의 활성화 단백인 AHNAK 단백이 폐암 조직에서 정상 조직보다 과발현된 것은, AHNAK 단백이 PLC-${\gamma}1$을 활성화시켜 폐암의 발생 기전에 관여할 수 있음을 뒷받침한다고 하겠다.

• 한국전기전자재료학회:학술대회논문집
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• 한국전기전자재료학회 2006년도 추계학술대회 논문집 Vol.19
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• pp.79-80
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• 2006

A stoichiometric mixture of evaporating materials for $CdIn_2S_4$ single crystal thin films was prepared from horizontal electric furnace. To obtain the single crystal thin films, $CdIn_2S_4$ mixed crystal was deposited on thoroughly etched semi-Insulating GaAs(100) substrate by the Hot Wall Epitaxy (HWE) system. The temperature dependence of the energy band gap of the $CdIn_2S_4$ obtained from the absorption spectra was well described by the Varshni's relation. $E_g(T)=2.7116 eV-(7.74{\times}10^{-4} eV)T^2/(T+434)$. The crystal field and the spin-orbit splitting energies for the valence band of the $CdIn_2S_4$ have been estimated to be 0.1291 eV and 0.0248 eV, respectively, by means of the photocurrent spectra and the Hopfield quasicubic model. These results indicate that the splitting of the ${\Delta}so$ definitely exists in the ${\Gamma}_5$ states of the valence band of the $AgInS_2$/GaAs epilayer. The three photocurrent peaks observed at 10K are ascribed to the $A_1-$, $B_1-$, and C1-exciton peaks for n = 1.

• 센서학회지
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• 제15권6호
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• pp.397-405
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• 2006

Single crystal $AgGaSe_{2}$ layers were grown on thoroughly etched semi-insulating GaAs(100) substrate at $420^{\circ}C$ with hot wall epitaxy (HWE) system by evaporating $AgGaSe_{2}$ source at $630^{\circ}C$. The crystalline structure of the single crystal thin films was investigated by the photoluminescence and double crystal X-ray diffraction (DCXD). The carrier density and mobility of single crystal $AgGaSe_{2}$ thin films measured with Hall effect by van der Pauw method are $4.05{\times}10^{16}/cm^{3}$, $139cm^{2}/V{\cdot}s$ at 293 K, respectively. The temperature dependence of the energy band gap of the $AgGaSe_{2}$ obtained from the absorption spectra was well described by the Varshni's relation, $E_{g}(T)$=1.9501 eV-($8.79{\times}10^{-4}{\;}eV/K)T^{2}$/(T+250 K). The crystal field and the spin-orbit splitting energies for the valence band of the $AgGaSe_{2}$ have been estimated to be 0.3132 eV and 0.3725 eV at 10 K, respectively, by means of the photocurrent spectra and the Hopfield quasicubic model. These results indicate that the splitting of the ${\Delta}So$ definitely exists in the ${\Gamma}_{5}$ states of the valence band of the $AgGaSe_{2}$. The three photocurrent peaks observed at 10 K are ascribed to the $A_{1}-$, $B_{1}-$, and $C_{1}-$exciton peaks for n=1.

• 센서학회지
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• 제14권3호
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• pp.160-168
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• 2005

ZnO epilayer were synthesized by the pulesd laser deposition(PLD) process on $Al_{2}O_{3}$ substrate after irradiating the surface of the ZnO sintered pellet by the ArF(193 nm) excimer laser. The epilayers of ZnO were achieved on sapphire ($Al_{2}O_{3}$) substrate at a temperature of $400^{\circ}C$. The crystalline structure of epilayer was investigated by the photoluminescence. The carrier density and mobility of ZnO epilayer measured with Hall effect by van der Pauw method are $8.27{\times}1016cm^{-3}$ and $299cm^{2}/V{\cdot}s$ at 293 K, respectively. The temperature dependence of the energy band gap of the ZnO obtained from the absorption spectra was well described by the Varshni's relation, $E_{g}(T)$=3.3973 eV-($2.69{\times}10^{-4}$ eV/K)$T^{2}$/(T+463K). The crystal field and the spin-orbit splitting energies for the valence band of the ZnO have been estimated to be 0.0041 eV and 0.0399 eV at 10 K, respectively, by means of the photocurrent spectra and the Hopfield quasicubic model. These results indicate that the splitting of the ${\Delta}so$ definitely exists in the ${\Gamma}_{6}$ states of the valence band of the ZnO. The three photocurrent peaks observed at 10 K are ascribed to the $A_{1}-$, $B_{1}-$, and $C_{1}-$exciton peaks for n = 1.

• 천문학회보
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• 제37권2호
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• pp.82.1-82.1
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• 2012

GRB100205A is a Gamma Ray Burst (GRB) which is suspected to be at redshift z=11-13 due to its very red H-K color($(H-K)_{vega}=2.1{\pm}0.5$). We observed a field centered at GRB100205A with Wide Field Camera (WFCAM) at United Kingdom Infrared Telescope (UKIRT) in Hawaii, in order to search a quasar that could be located around the GRB. The images were obtained in J, H, and K filters covering a square area of $0.78deg^2$. Our J-, H-, and K-band data reach the depths of 22.5, 22.1, and 21.0 mag (Vega) at $5{\sigma}$, respectively. Also using z-band image observed by CFHT, we find 8 candidates that have colors consistent with a quasar at z=11-13(non-detection in z-, J-band and $(H-K)_{vega}$ > 1.6). However, the shallow depths of J-, H-band are not enough to verify their true nature. Instead, we identify many red objects to be old or dusty galaxies at $z{\geq}3$. The number density of such objects appears about twice or more than that of the field of Cosmological Evolution Survey (COSMOS) and Ultra Deep Survey (UDS) of UKIRT Infrared deep sky survey (UKIDSS). On scales between 0.18' and 15' the correlation function is well described by a power law with an exponent of ${\approx}-0.9$ and this implies that those objects are like galaxies. It is interesting that many red galaxies exist in the region where the GRB was detected.