• Publications of The Korean Astronomical Society
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• v.30 no.2
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• pp.401-403
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• 2015

We present the 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 ($z_s=0.245$) is severely distorted by a nearby elliptical galaxy ($z_l=0.08$), via gravitational lensing. The system is analysed by several methods, including surface brightness fitting, gravitational lens modeling, and spectral energy distribution fitting. From Galfit and Ellipse we measure basic parameters of the galaxy, such as the effective radius and the average surface brightness within it. gravlens yields the total mass inside the Einstein radius ($R_{Ein}$), and MAGPHYS gives us an estimate of the stellar mass inside $R_{Ein}$. By comparing these parameters, we confirm that the lens galaxy is an elliptical galaxy on the Fundamental Plane and calculate the stellar mass fraction inside $R_{Ein}$, and discuss the results with regards to the initial mass function.

• Publications of The Korean Astronomical Society
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• v.30 no.2
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• pp.525-527
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• 2015

We prepare a catalog of the morphological types of 5840 galaxies within z = 0.01. We determine the morphological types by visual inspection using color images from the Sloan Digital Sky Survey (SDSS) DR7. The majority of the sample galaxies are SDSS spectroscopic target galaxies, but we add ~ 900 galaxies whose redshifts are available in the NASA Extra Galactic Database (NED). The fraction of elliptical and lenticular galaxies is ~ 0.06 while spiral galaxies comprise ~ 30% of the sample with a bar fraction of ~ 0.6. About half of sample are dwarf galaxies of which ~ 35% are dwarf elliptical-like galaxies. There is a strong correlation between the morphological types and luminosities of the galaxies, i.e., high luminosities in the early type galaxies and low luminosity in the late type galaxies. The mean luminosity of dwarf elliptical-like galaxies is similar to that of irregular galaxies.

• Proceedings of the KSEEG Conference
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• 2003.04a
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• pp.196-197
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• 2003

Several masses of the alpine type ultramafic rocks are found within the Precambrian Kyeonggi gneiss complex, western part of Chungnam province. They occur as discontinuous isolated lenticular bodies along the fault line(NNE direction), dominant tectonic directions of Kyeonggi gneiss complex. The ultramafic rocks occur as fault contacts with the adjacent Precambrian metamorphic and metasedimentary rocks. (omitted)

• Nuclear Engineering and Technology
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• v.50 no.2
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• pp.259-267
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• 2018

Focused ion beam-scanning electron microscope and electron backscattered diffraction examinations were conducted in the center of a $73\;GWd/t_U\;UO_2$ fuel. They showed the formation of subdomains within the initial grains. The local crystal orientations in these domains were close to that of the original grain. Most of the fission gas bubbles were located on the boundaries. Their shapes were far from spherical and far from lenticular. No interlinked bubble network was found. These observations shed light on previous unexplained observations. They plead for a revision of the classical description of fission gas release mechanisms for the center of high burn-up $UO_2$. Yet, complementary detailed observations are needed to better understand the mechanisms involved.

• Proceedings of the Korea Information Processing Society Conference
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• 2015.04a
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• pp.927-928
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• 2015

무안경 3D 입체 디스플레이 장치는 패럴렉스 배리어(parallax barrier)와 렌티률러 렌즈(Lenticular lens)의 기반의 장치로 구분된다. 무안경 업체 디스플레이 장치를 통하여 입체영상을 디스플레이하기 위해서는 다중 시점(multi-view) 촬영 영상들의 서브픽셀 인터레이싱 방법을 통하여 하나의 영상으로 합성되어야 한다. 본 연구는 렌티큘러 렌즈 기반의 입체 디스플레이 장치에서 렌티큘러 렌즈의 속성에 따라 적응적으로 서브픽셀 인터레이싱 될 수 있는 기법을 제안하기 위한 사전 연구로서 기존에 발표된 서브픽셀 인터레이싱 기법의 종류를 분류하고 각 기법의 특성을 분석하고자 한다.

• Korean Journal of Optics and Photonics
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• v.21 no.2
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• pp.61-68
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• 2010

Optical simulation methods were applied to the edge-lit LED backlight for LCD TV applications in order to optimize the optical structure of the light guide plate(LGP), and thus to improve the uniformity properties by removing the bright spots caused by LED's. The edge-lit LED backlight consisted of three white LED's with a lamp cover, a light guide plate, and a reflection film. When there was no pattern on the entrance side surface of the LGP, the illuminance uniformity was sensitively dependent on the distance d between the LED and the entrance surface. The illuminance uniformity increased with d but its increasing rate slowed down when d was beyond ~ 1.5 mm. When micro-patterns such as a lenticular lens array (LLA) or a serration pattern were formed on the entrance surface, the illuminance uniformity was improved substantially even for the case of very small d. At the same simulation condition, the lightguide with serration pattern showed a better uniformity than that with LLA pattern. Additional improvement could be achieved by changing the refractive index of the micro-patterns. These results suggest that using micro-patterns is a very effective way to reduce the bright spots due to their refracting function for the concentrated incident rays onto the LGP.

• Publications of The Korean Astronomical Society
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• v.27 no.4
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• pp.263-264
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• 2012

We present the properties of dust and the near-infrared spectral features in nearby early-type galaxies. The properties of dust are obtained from the AKARI far-infrared all-sky survey diffuse map. The AKARI/IRC is used for the near-infrared spectra. We improve spectral data with the new dark subtraction method on the basis of the knowledge acquired in our laboratory experiments of the engineering-model detector for the IRC. We have succeeded in fitting the continuum by a power-law function and detecting CO and SiO absorption features in early-type galaxy spectra. Comparing the properties of dust and near-infrared spectral features, we find that the power-law slope depends on dust temperature, but not on the dust mass, which suggests that low-luminosity AGNs may contribute to the changes in the power-law slope and dust temperature.

• Publications of The Korean Astronomical Society
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• v.32 no.1
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• pp.151-153
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• 2017

Early-type galaxies (ETGs) are generally dominated by old low-mass stars, which are not very productive of dust, and hot interstellar plasmas, which are very destructive of dust. Thus ETGs provide harsh environments for survival of dust. It has been found that some ETGs contain a large amount of dust, and yet its supply mechanism is not understood well. We present the result of a systematic study of dust in ETGs with the AKARI mid- and far-infrared all-sky surveys. From the AKARI result and the Ks band data obtained by ground-based telescopes, we find that there is a global correlation between the dust mass and stellar luminosity. We also compare the AKARI all-sky survey result with the CO data to discuss origins of dust in ETGs.

• The Korean Journal of Quaternary Research
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• v.2 no.1
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• pp.13-24
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• 1988

The deposit (named Kanweoldo deposit) unconformably overlain by the Holocene tidal deposit is mainly exposed along the tidal channel of the Sajangpo tidal flat of Cheonsu Bay, west coast of Korea. The Kanweoldo deposit's sedimentary textures, sedimentary structures and erosion surfaces of the stratigraphic events have been investigated. The Kanweoldo deposit is mainly composed of mud, silt and sandy mud. The sedimentary criteria indicating intertidal deposit i.e. lenticular bedding, thinly and coarsely interlayered bedding, wavy lamination and flaser bedding are positively found in the Kanweoldo deposit. The deposit is semi-consolidated and brown in color, and has erosional contact (stratigraphic boundary) with the overlying Holocene tidal deposit. Considering such Kanweoldo deposit's sedimentary characteristics and stratigraphic relation with the Holocene tidal deposit, the Kanweoldo deposit seems to be deposited under intertidal environment during Riss-Wurm interglacial period and subaerially exposed and eroded during the last glacial period.

• Proceedings of the Korea Contents Association Conference
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• 2009.05a
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• pp.115-119
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• 2009

Digital is the main topic of 21C design. Experts analyzed that pop art and related cultural products are becoming popular as digital generations of twenties to forties are centered of new art culture. This survey is to suggest the differentiated jewelry products which are out of the existing products as combining the embodiment of various colors by using celebrities who are taken kindly to and the lenticular which can be image converted through an optical illusion. As public's living standard is getting improved, design elements would come into the spotlight. Therefore, this research is expected to work as the part of an epoch-making design in the jewelry industry by extending the design field.