• Journal of the Korean Society of Clothing and Textiles
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• v.23 no.8
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• pp.1206-1217
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• 1999

This study is focused on 'mysticism' in fashion which is recently marked as one of the cultural phenomenon emerging at the end of the century, First of all the concept of 'mysticism' and 'occultism' are reviewed to define the mysticism in fashion. Mysticism as a cultural phenomenon is also examined in historical and social context. With these theoretical basis articles which were publshed in 1990s from Korean newspapers and magazines which reported cultural phenomenon related to mysticism are analyzed and categorized. Finally these categories are applied to fashion phenomenon and 'mysticimsm in fashion' is analyzed and clearly examined as a fashion trend. As a result mysticism in fashion that has arose as an end of the century phenomenon within the historical and social context could be categorized into five groups such as 'primitive religion' ' Christianity ' 'oriental philosophy' 'universe' and 'magic and witchcraft'.

• The Bulletin of The Korean Astronomical Society
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• v.36 no.2
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• pp.55.2-55.2
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• 2011

We present the current research activities of the Center for the Exploration of the Origin of the Universe, a center established at Seoul National University with the Creative Research Initiative program. Our activities focus on observational studies of distant objects such as gamma-ray bursts, quasars, and proto-cluster of galaxies, but we also carry out other observational and theoretical studies in related topics. We also developed a new instrument, Camera for Quasars at Early Universe (CQUEAN) in collaboration with Kyunghee University group, and have secured observing facilities such as UKIRT and McDonald 2.1m observatory. Our research highlights include results such as the discovery of high redshift quasars and gamma ray bursts, the discovery of tidal disruption event at z=0.38 and peculiar gamma ray burst events, analysis of proto-clusters of galaxies, the discovery of brown dwarfs, and development of CQUEAN and its usage at the McDonald observatory.

• The Bulletin of The Korean Astronomical Society
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• v.41 no.1
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• pp.31.3-31.3
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• 2016

Exploring a universe with gravitational waves (GWs) was only theoretical expectation for long time. In September 2015, the Laser Interferometer GW Observatory (LIGO) first detected GWs emitted from the collision of two stellar-mass black holes in cosmological distance (1.3 billion light years) on Earth. This confirms the existence of black-hole binary mergers, and further, opens a new field of GW astronomy. We begin our discussion with a list of important GW sources that can be detectable on Earth by large-scale laser interferometers such as LIGO. Focusing on compact objects such as neutron stars and black holes, we then discuss possible research in the context of GW astronomy. By coordinating with existing observatories, searching for electromagnetic waves or particles from astronomical objects, around the world, multi-messenger astronomy for the universe's most cataclysmic phenomena (e.g. gamma-ray bursts) will be available in the near future.

• The Bulletin of The Korean Astronomical Society
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• v.39 no.1
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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.

• The Bulletin of The Korean Astronomical Society
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• v.39 no.1
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• pp.32.1-32.1
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• 2014

Astronomical observations strongly suggest that the expansion rate of our universe is currently under acceleration. The nature of the so-called dark energy causing the acceleration is unknown, and it is one of the fundamental mysteries in the present day theoretical cosmology. Here we briefly review the current state of cosmic dark energy research in both theoretical and observational sides. Constraints on dynamical dark energy models (e.g., w-fluid, quintessence, and modified gravity) with recent observational data from type Ia supernovae, cosmic microwave background radiation, and large-scale structures in the universe indicate a preferred direction toward the simplest ${\Lambda}$CDM world model. We also discuss some issues regarding the early dark energy model and the spherical collapse of matter in the presence of dark energy.

• Journal of The Korean Astronomical Society
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• v.28 no.2
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• pp.109-117
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• 1995

The morphology and strength of the primordial magnetic field which is generated spontaneously in the early universe are studied for three models: (1) inflation (2) primordial magnetized bubble and (3) primordial turbulence models, We calculate the power spectra of magnetic field that are scale-free and proportional to $k^{1.5},k^{3{\sim}4}$ and $k^{2/3}$, respectively. The configurations of magnetic field having these power spectra are visualized. To constrain the present strength of the primordial magnetic field we calculate the anisotropy of the microwave background radiation in Bianchi type I universe with globally homogeneous magnetic field. From the COBE limit of the quadrupole moment of $({\delta}T/T)_{l=2}$ the present strength of horizen-scale magnetic fields $B_p$ is constrained to be less than $9{\times}10^{-8}G$.

• Publications of The Korean Astronomical Society
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• v.30 no.2
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• pp.611-616
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• 2015

The Antarctic high plateau offers exceptional conditions for infrared and terahertz astronomy, as well as for programs requiring long, uninterrupted periods for measurements made with high cadence and photometric precision (i.e. time domain astronomy). In this review we summarise the special conditions of the Antarctic plateau which facilitate these observing regimes. We also outline some high profile science programs in each that could be conducted most effectively from the Antarctic high plateau, involving the first light in the Universe, the life cycle of our Galaxy, and the equation of state for the Universe. Three high plateau sites are under particular consideration for furthering such scientific programs{Dome A, Dome F and Ridge A. We summarise the activity underway at each site, which includes the building of new stations and the construction of facilities for optical, infrared and terahertz astronomy, as well as the plans for their future development.

• Publications of The Korean Astronomical Society
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• v.30 no.2
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• pp.367-369
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• 2015

The FastSound project is a galaxy redshift survey using Subaru/FMOS to detect $H{\alpha}$ emitting galaxies at z ~ 1:3, for the purpose of probing the origin of the accelerated expansion of the universe. The survey has detected ~4,000 galaxy redshifts in a total area of $30deg^2$, and detected the redshift space distortion at this redshift range for the first time. The redshift space distortion (RSD) signal will be used to derive a measurement of the growth rate of large scale structure, which will provide a test for modified gravity as a possible origin of accelerated cosmic explansion. Here we present an overview and the current status of the project.

• Korean Journal of Logic
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• v.6 no.1
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• pp.33-50
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• 2003

본 논문에서 필자는 기존의 양상 허구주의의 번역 체계가 가지고 있는 세가지 난점을 극복할 수 있는 양상 허구주의의 새로운 번역 체계를 제시한다. 이 세 난점이란 (1) 많은 세계들의 존재를 받아들이지 않을 수 없게 된다. (2) 세계 간의 비교를 하게 하는 양상 진술문을 제대로 번역할 수 없다 (3) 어떤 양상 진술문에 내해 잘못된 진리치를 부여한다 이다. 이 세 난점을 극복하기 위한 필자의 제안은 세계-양화사의 범위 안에 등장하는 양화사들이 주어진 세계 내의 사물들만을 범위 내에 포함하는 루이스의 초기 번역 체계나 비한정적 양회사를 도입하는 루이스의 후기 번역 체계를 받아들이는 대신, 양화사를 조금씩 조금씩 비한정시키는 (unrestrict) 시키는 것이며, 필지 공식 번역 체계는 우주 (세계)의 부분전체론적 합으르 정의되는 "다우주(muitiverse)"라는 새로운 용어를 도입함으로써 얻어진다. 필자의 공식 번역 체계는 다음과 같다: P가 가능하다 iff PW에 의하면 P가 잠인 다우주가 존재한다 P가 필연적으로 참이다 iff PW에 의하면 모든 다우주에서 P가 참이다 마지막으로 필자는 비한정적인 세계 간의 비교를 하게 하는 양상 진술문을 적절하게 번역하기 위해서 필자의 번역 체계에 약간의 수정을 가한다.

• The Bulletin of The Korean Astronomical Society
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• v.43 no.2
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• pp.40.3-40.3
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• 2018

This dissertation presents the results on two-dimensional Redshift space distortion (hereafter RSD) analyses of the large-scale structure of the universe using spectroscopic data and on improvement of modeling of the RSD effect. RSD is an effect caused by galaxies' peculiar velocity on their clustering feature in observation along the line of sight and is thus intimately connected to the growth rate of the structure in the universe, from which we can test the origin of cosmic acceleration and Einstein's theory of gravity at cosmic scales in the end. However, there are several challenges in modeling precise and accurate RSD effect, such as non-linearities and the existence of an exotic component, e.g. massive neutrino. As part of endeavors for modeling more precise and accurate galaxy clustering in redshift space, this dissertation includes a series of works for this issue. (More detailed descriptions were omitted.)