• 천문학회보
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• 제36권1호
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• pp.51.1-51.1
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• 2011

Red dusty Active Galactic Nuclei (AGNs) are suspected to mid-stage between ULIRG and AGN phase. As well as, red AGNs are suspected that they have more than 50% of whole AGN population. In order to understand the character of red AGNs, Black Hole (BH) mass of red AGN is a key property and can not measured by existing method such as reverberation mapping and single epoch method. Thus we still don't know their character and properties in clearly. To estimate properties of red AGNs without the effect of dust-obscuration, we have obtained Near InfraRed (NIR) spectra of 31 reverberation mapped AGNs and 49 Palomar-Green(PG) Quasi-Stellar Object (QSO) by using the infrared camera (IRC) for AKARI with unique wavelength range $2.5-5.0{\mu}m$. From this spectra, we measured the FWHM and luminosity of brackett ${\alpha}$ and ${\beta}$ at 4.0, 2.6 micron meter for deriving new BH mass estimators based on the properties of Brackett line emission.

• 대한수학회논문집
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• 제20권2호
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• pp.231-238
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• 2005

In this paper, we study the arithmetic properties of orders in a quaternion algebra over a dyadic local field and we find the mass formula of orders.

• 터널과지하공간
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• 제12권3호
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• pp.220-228
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• 2002

절리암반에서의 열유동을 수치해석적으로 분석하였다. 1차원 모델 해석을 통하여 한 조의 절리군이 열전도에 미치는 영향을 비교 분석하고, 이론해와 비교하였다. 절리 내에 물이 전혀 없는 경우, 절리는 열 차단제의 역할을 하며 정상상태에서도 온도의 불연속이 관찰되었다. 따라서 암반 내 존재하는 절리가 완전 건조상태인 경우에는 개별적인 절리의 열차단 효과를 일일이 고려하여야 정확한 결과를 얻을 수 있다 그러나 절리 내에 물이 부분적으로 혹은 완전히 포화된 경우에는 열차단 효과가 현저히 줄어들어 온도 분포에 미치는 영향이 현저히 감소하였다. 따라서 절리 암반을 통한 열전도는 암반을 무결암의 열적 성질과 불연속면의 열적 성질을 포함한 열적 이방성 연속체로 가정함으로써 가능하다 할 수 있다. 절리의 포화 정도가 증가할수록 절리가 열유동에 미치는 영향이 감소하므로 암반의 열전달 특성은 등방에 가까워지며, 따라서 복잡한 모델을 이용한 해석보다는 현지 암반의 열물성을 정확히 측정하는 것이 더욱 중요함을 알 수 있었다.

• 한국정밀공학회지
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• 제12권9호
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• pp.22-29
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• 1995

An experimental method to identify the rigid properties (mass, moment of inertia, center of mass) of mounted structures is presented. A direct system identification method is developed and applied to identify the mass, damping and stiffness martix directly from the translational response of vibration testing. Conventional method is sensitive to noise since it needs artificial rotational response of temporary center of mass which is made by the linear transformation of translational response. A presented method needs only the translational response, and it is robuster to noise than conventional method. Several experimental and numerical implementations show the presented method is effective.

• 대한용접접합학회:학술대회논문집
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• 대한용접접합학회 2009년 추계학술발표대회
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• pp.205-209
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• 2009

Wetting properties between silver-copper-titanium braze alloys with different titanium contents up to 2.8 mass% and hexagonal boron nitride ceramics were investigated using sessile drop method at 1123K in Argon. The final contact angle is less than $30^{\circ}$ when the Ti content was over 0.41 mass%. Meanwhile, the contact angle curves show different behavior. In case of using braze alloy containing 2.8 mass% of titanium, the initial contact angle is acute angle just after the melting of braze. In case of brazes containing titanium less than 2.26 mass%, the contact angle is larger than $90^{\circ}$ at the beginning and slowly decreases to acute angle. The reaction layer of titanium nitride is observed at the interface. In addition, the reaction of Ti in the braze and N in the bulk h-BN seemed to show diffusion limited spreading.

• 천문학회보
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• 제39권1호
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• pp.36.2-36.2
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• 2014

We present results of the analysis of FLS 1718+59, a galaxy-galaxy gravitational lens system in the Spitzer First Look Survey (FLS) Field. A background galaxy (z = 0.245) is severely distorted by an elliptical galaxy (z = 0.08), by gravitational lensing. We analyze this system by several methods, including Ellipse and Galfit fitting, gravitational lens modeling (gravlens), and SED fitting. Properties of the lens galaxy can be obtained: from Galfit we measure the effective radius and the average surface brightness inside it, and from gravlens we estimate the total mass inside the Einstein radius (lensing mass). We use these parameters to check that the lens galaxy is located on the Fundamental Plane. Also, we conduct SED fitting for the lens galaxy and estimate the stellar mass, and compare this with the lensing mass of the lens galaxy to check the M-L relation.

• 천문학회보
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• 제37권2호
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• pp.80.1-80.1
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• 2012

The $2.5-5.0{\mu}m$ spectrum of AGN was poorly understood due to the atmosphere effect beyond $2{\mu}m$. Nevertheless, the $2.5-5.0{\mu}m$ range includes several important lines, such as $Br{\beta}$ ($2.63{\mu}m$), $Br{\alpha}$ ($4.05{\mu}m$), PAH (3.3${\mu}m$) and many molecular or atomic lines. We compile $2.5-5.0{\mu}m$ spectra of 79 AGNs and QSOs from infrared camera (IRC) on AKARI infrared astronomy satellite. Our $2.5-5.0{\mu}m$ spectra will provide an access to full wavelength spectra of AGNs for the first time. Moreover, we present the Brackett line properties, FWHMs and luminosities, of AGNs. Using these Brackett line properties, we derive new black hole (BH) mass estimators. The new BH mass estimators using NIR hydrogen lines will be very useful to estimate BH mass of dusty red AGNs in the future.

• 한국지반공학회:학술대회논문집
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• 한국지반공학회 2004년도 춘계학술발표회
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• pp.407-414
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• 2004

Interfacial properties between rock mass and shotcrete play a significant role in the transmission of loads from the ground to shotcrete. These properties have a major effect on the behaviours of rock mass and shotcrete. They, however, have merely been assumed in most of numerical analyses, and little care has been taken in identifying them. This paper aimed to identify interfacial properties including cohesion, tension, friction angle, shear stiffness, and normal stiffness, through direct shear tests as well as interface normal compression tests for shotcrete/rock cores obtained from a tunnel sidewall. Mechanical properties such as compression strength and elastic modulus were also measured to compare them with the time-dependent variation of interfacial properties. Based on experiments, interfacial properties between rock and shotcrete showed a significant time-dependent variation similar to those of its mechanical properties. In addition, the time-dependent behaviours of interfacial properties can be well regressed through exponential and logarithmic functions of time.

• 화약ㆍ발파
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• 제25권1호
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• pp.67-77
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• 2007

본 연구에서는 NATM 터널 시공사이클에서 필수적으로 수행되는 천공작업 시 획득할 수 있는 정보를 통해 굴착 대상 암반의 특성을 평가하는 방안에 대해 고찰하였다. 활용 가능한 천공데이터는 천공속도, 피트압, 토크 등이 있으며, 이러한 인자들과 암반 특성들과의 상관관계를 규명하고자 하며 이러한 결과를 토대로 향후 정량적 발파설계를 위한 가이드라인을 제안하고자 하였다.

• 한국콘크리트학회:학술대회논문집
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• 한국콘크리트학회 2008년도 추계 학술발표회 제20권2호
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• pp.489-492
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• 2008

물/결합재비가 0.4이면서 5%의 실리카퓸이 혼입된 3가지 매스콘크리트 배합과 실리카퓸이 혼입되지 않은 1가지 매스콘크리트 배합에 대해 단열온도상승실험과 자기수축실험을 실시하여 실리카퓸이 매스콘크리트의 수화발열특성과 자기수축에 미치는 영향을 규명하고, 그 결과를 통해 실리카퓸의 매스콘크리트에 대한 적용 가능성을 검토하였다. 실험결과, 매스콘크리트 배합의 경우에는 실리카퓸을 혼입하여도 수화반응속도가 거의 증가하지 않으면서 최종단열온도상승량이 5$^{\circ}$C 정도 감소하는 것으로 나타났으며, 콘크리트의 극한자기수축량은 실리카퓸의 혼입여부에 상관없이 거의 동일한 것으로 나타났다. 따라서 실무에서 매스콘크리트 구조물의 시공에 실리카퓸을 적용하면 내구성뿐만 아니라 수화열 균열제어에도 이점이 있을 것으로 판단된다.