• Journal of Astronomy and Space Sciences
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• v.12 no.1
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• pp.30-43
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• 1995

New UBVRI observations of triple star $\lambda$ Tau were made at Chungbuk Ntional University Observatory for 31 nights from Dec. 1990 to Jan. 1994. A total of 2930 photometric observations were obtained with 586 points for each filters, and BVRI light curves were constructed. From the primary light curves, the one times of primary minimum light was determined with a new light element. The photometric solutions of light curves for $\lambda$ Tau were calculated by using Wilson-Devinney method with our BVRI light curves and the BV light curves obtained by Grant(1959). We determined spectroscopic solutions that were satisfied with these two light curves and the radial velocity curves had been collected by Fekel and Tomkin (1982). From these values, absolute dimensions for this system were estimated. The radius and mass for the primary star are turned out to be $8.3R_\odot$ and $8.1m_\odot$, and $6.5R_\odot$ and $2.1m_\odot$ for the secondary star, respectively.

• Bulletin of the Korean Space Science Society
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• 2011.04a
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• pp.21.1-21.1
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• 2011

우리는 분리형 쌍성 11개(원궤도 7개, 타원궤도 4개), 반분리형 쌍성 7개와 접촉형 쌍성 9개(근첩촉형 3개, 접촉형 2개, 초과 접촉형 4개)를 포함하는 27개의 다양한 종류의 표준식쌍성의 분석하여 절대량을 구하였다. 표준 식쌍성은 식쌍성의 광도곡선이 적어도 두 파장 영역 이상에서 그리고 모든 위상에서 골고루 관측되었고, 쌍성의 두 구성원 별에 대하여 시선속도 곡선이 발표된 식쌍성, 즉, 이중분광선 식쌍성 (Double line spectroscopic eclipsing binariy)으로 정의한다. 우리는 표준식쌍성의 370개의 후보에 대하여 문헌을 조사하여 관측 데이터를 확보 하였다. 이중에서 시선속도곡선과 광도곡선 자료가 동시에 존재하는 식쌍성은 80개이다. 이번 연구에서 우리는 표준식쌍성의 관측 질을 고려하여 27개의 식쌍성을 선택하여 절대량을 계산하였고, 이전 연구자들이 발표한 절대량과 비교 하였다. 이 논문에서 제시한 표준식쌍성의 유용성을 확인하기 위해 소마젤란은하에서 발견한 식쌍성의 광도곡선을 분석하여 측광학적인 해를 구하는 작업을 수행하였다. 이를 위하여 표준 식쌍성을 식쌍성의 종류별로 구분하고, 소마젤란은하에서 발견된 식쌍성 20여개를 선정하였다. 선정된 식쌍성을 표준식쌍성의 광도곡선과 형태를 비교하여 초기값을 결정하였고, 반복적인 차등보정법으로 측광학적인 해를 구하였다. 이 논문에서 제시한 표준식쌍성이 소마젤란은하에서 발견된 식쌍성들의 광도곡선의 형태를 대부분 포함하는 다양한 분포로 형성되어 있고, 이에 따른 측광학적인 해가 관측과 잘 일치함을 보여주고 있다.

• Journal of Astronomy and Space Sciences
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• v.14 no.2
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• pp.233-241
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• 1997

New UBV Photometric observations for a close binary RZ Cas were obtained at the Chungbuk National University Observatory for 42 nights from October 1991 to March 1993, and standardized UBV light curves were constructed. From the primary light curves, the eight minimum times were determined by using a new light element. We confirmed the primary minimum was totality and derived the average duration was 18.1 minutes corresponding to $0.^{p}01$. The photometric and spectroscopic solutions were calculated with the obtained light curves and the radial velocity curves of Duerbeck & Hanel(1979) by using Wilson-Devinney method. From these values, the absolute dimensions of this binary system were estimated.

• Korean Journal of Optics and Photonics
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• v.4 no.1
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• pp.90-100
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• 1993

A computer routine for personal computer(PC/AT class) is developed to analysize the mode characteristics of silica based optical waveguides whose cross sections are of semi circular and other typical shapes. The basic algorithm used in the routine is to convert the wave equation into a matrix equation by expanding the wave function in terms of simple harmonic functions. The matrix elements are a set of overlap integrals of sinusoidal funtions with appropriate weight given by the distribution of refractive index over the waveguide cross section. The eigenvectors and eigenvalues of the matrix is then computed via diagonalization. We explain some practical problems that arises when implementing the algorithm into the routine. By using this routine we analyze the mode characteristics of silica based optical waveguides of semi circular and some other typical cross sections.

• Proceedings of the Korean Ceranic Society Conference
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• 2004.10a
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• pp.95.4-95.4
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• 2004

• Analytical Science and Technology
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• v.16 no.2
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• pp.152-158
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• 2003

This study was conducted to evaluate two sample digestion procedures and instrumental determination parameters for analysis of lead in bone. Amputated human legs were treated by acid digestion or microwave dissolution prior to spectrometric analysis. Inductively coupled plasma mass spectrometry (ICP-MS) and graphite furnace atomic absorption spectrometry (GF-AAS) were used for determining bone lead levels. Recovery efficiencies using standard reference material from acid digestion measured by ICP-MS were in good agreement with those of the certified value, but in cases of acid digestion by GF-AAS and microwave digestion by both two methods, recovery underestimated and overestimated, respectively. For the bone samples, the lead concentrations obtained by ICP-MS after acid digestionwere in good agreement with those by GF-AAS (correlation coefficient = 0.983), but GF-AAS gave systematically higher values than ICP-MS. While a good agreement between two analytical methods after microwave digestion was also obtained (correlation coefficient = 0.950), bone lead concentrations from microwave were relatively higher than those from acid digestion. In conclusion, the use of the simple nitric acid digestion procedure at an ambient temperature coupled to ICP-MS seems to be efficient for the determination of lead in bone in consideration for both the convenience and validity.

• Korean Journal of Optics and Photonics
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• v.10 no.1
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• pp.40-46
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• 1999

We present a new modified effective index method which can be used to analyze lightwave circuit devices in 3-dimensional structure fast and accruatly using 2-dimensional BPM (beam propagating method). This method can analyze the devices with the cross-section of rectangular, ridge, or similar shapes accurately but more quickly than the 3-dimensional BPM, which is impractical to use on account of long calculating time. As an example, we showed that the calculation error of coupling length in a directional coupler by this method is significantly less than the 2-dimensional BPM using the effective index method.

• Journal of Astronomy and Space Sciences
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• v.18 no.1
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• pp.55-62
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• 2001

We present VRI CCD photometry of W UMa type binary TY UMa. The light curves show that the secondary minimum is deeper than the primary minimum and the maximum I ($0.^{p}25$)is $0.^{m}023$ brighter than the maximum II ($0.^{p}75$). The V light curve has been analyzed and the photometric solutions have been determined by the method of Wilson & Devinney differential correction. We adopted the spot model to explain the asymetric light curve.

• Journal of the Institute of Electronics Engineers of Korea SC
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• v.37 no.4
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• pp.49-54
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• 2000

A new functional organic thin film optical waveguide ion sensor is designed, which can select a specific ion, i.e., $Ca^{2+}$ -ion. The sensing membrane was composed of PVC-PVAC-PVA copolymer matrix based on anionic cation-selective chromoionophor(ETH5294), neutral ionophore(K23El), anionic site and plasticizer and it was coated on the etched glass substrate as embeded type optical waveguide itself. The sensor sensitivity dependence on waveguide length and thickness, contence of chromoionophore, and each mode was investigated. And this sensor could detect $Ca^{2+}$ ion in concentrations ranging from 1$\times$10­6~1M(with 0.05M tris-HCI buffer solution of pH7.4) by measuring the absorbance change at 514nm of light. Utilizing thin film membrane, the fast response time and high sensitivity are obtained. Also, it is expected that this sensor can be applied to various biochemical important ions.ons.

• Journal of Astronomy and Space Sciences
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• v.26 no.3
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• pp.295-304
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• 2009

We present BV light curves of EROS 1010 which is located in the central bar of the Large Magellanic Cloud. The BV light curves including BR and I light curves observed by the EROS and OGLE projects, have been analyzed using the 2005 version of the Wilson & Devinney Differential Correction program for the photometric solutions. The absolute dimensions of EROS 1010 were calculated by adopting the distance modulus of the Large Magellanic Cloud, $m-M=18.^m3{\sim}18.^m5$.