• 천문학회보
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• 제35권1호
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• pp.58.1-58.1
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• 2010

We carried out simultaneous 22GHz $H_2O$ and 44GHz $CH_3OH$ maser line surveys of about 1000 galactic YSOs using KVN 21m telescopes. The sources consist of low-mass, intermediate-mass, high-mass YSOs in different evolutionary stages. We will present the preliminary results.

• Journal of Astronomy and Space Sciences
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• 제15권1호
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• pp.1-26
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• 1998

The structure of the magnetic funnel element in the intermediate polar is con-sidered in terms of an important site for the X-ray absorption and the reemis-sion of the X-ray as the optical light. In this paper the column density and the optiacl depth vary with the filling factor, which is introduced to characterize the structure of matter in the magnetic funnel element. The results of the en-ergy dopendence of the X-ray spectrum and the modulation depth of the X-ray light curve are discussed.

• 천문학회보
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• 제42권1호
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• pp.44.4-45
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• 2017

We report the first detection of RR Lyrae variable stars in the Crater II dwarf galaxy, a recently discovered ultra-faint satellite of the Milky Way. Based on B, V time series photometry obtained with the Korea Microlensing Telescope Network (KMTNet) at CTIO, Chile, we have identified ~45 fundamental-mode (ab-type) and ~2 first-overtone (c-type) RR Lyrae stars by adopting template light-curve fitting method. Our preliminary analysis suggests an Oosterhoff-intermediate classification of this galaxy from the mean period of the RRab stars, <$P_{ab}$> ${\simeq}0.63$ days, and the location of them on the period-amplitude diagram. We discuss the properties of the RR Lyare stars in this galaxy.

• 한국우주과학회:학술대회논문집(한국우주과학회보)
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• 한국우주과학회 1999년도 한국우주과학회보 제8권2호
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• pp.13-14
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• 1999

No Abstract, See Full Text

• 한국우주과학회:학술대회논문집(한국우주과학회보)
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• 한국우주과학회 2000년도 한국우주과학회보 제9권2호
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• pp.89-89
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• 2000

No Abstract, See Full Text

• 한국우주과학회:학술대회논문집(한국우주과학회보)
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• 한국우주과학회 2011년도 한국우주과학회보 제20권1호
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• pp.31.1-31.1
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• 2011

In this study, we investigated alignment state estimation performances of the three methods i.e. merit function regression (MFR), differential wavefront sampling (DWS) and Multiple Design Configuration Optimization (MDCO). The three target optical systems are 1) a two-mirror Cassegrain system for deep space Earth observation, 2) intermediate size three-mirror anastigmat for Earth ocean monitoring, and 3) extremely large segmented optical system for astronomical observation. We ran alignment state estimation simulation for several alignment perturbation cases including 1mm to 10mm in decenter and from 0.1 to 1 degree in tilt perturbation error for the two-mirror Cassegrain system. In general, we note that MDCO shows more competitive estimation performance than MFR and DWS. The computational concept, case definition and the simulation results are discussed with implications to future works.

• 대한수학회보
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• 제54권5호
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• pp.1619-1625
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• 2017

The aim of this short note is to give a simple proof of the non-rationality of the double cover of the three-dimensional projective space branched over a sufficiently general quartic.

• 한국통신학회:학술대회논문집
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• 한국통신학회 2004년도 추계종합학술대회 논문 초록집
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• pp.117-117
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• 2004

• 한국멀티미디어학회논문지
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• 제9권8호
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• pp.971-981
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• 2006

쉬어-왑 분해 렌더링은 볼륨 렌더링 방법 중 가장 빠르지만 영상의 화질이 좋지 않다는 단점이 있다. 본 연구에서는 쉬어-왑 렌더링의 빠른 속도를 유지하며 화질을 개선하는 방법을 제안한다. 화질 개선의 첫 번째 방법은 중간영상(intermediate image) 기반의 수퍼샘플링(supersampling) 기법이다. 객체 좌표와 영상 좌표간의 변환을 효율적으로 수행하여 임의 비율의 영상 확대를 빠르게 수행한다. 화질 개선의 두 번째 방법은 선-적분(pre-integrated) 렌더링을 사용하는 것이다. 기존의 선-적분 기반 쉬어-왑 렌더링은 빈-공간 도약(empty space leaping)을 하지 못하여 속도가 저하되는 문제가 있지만, 본 연구에서 제안하는 겹친 최소-최대 지도(overlapped min-max map) 자료구조를 사용하면 빈-공간 도약을 수행하여 속도 문제를 해결한다. 본 제안 방법을 통해 광선추적법(ray-tracing) 수준의 고화질 렌더링 영상을 빠른 시간에 생성할 수 있다.

• 천문학회보
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• 제40권2호
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• pp.33.1-33.1
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• 2015

M85 is a nearby merger remnant galaxy located at the northern part of the Virgo Cluster. Because of its remarkable merging features, it is an interesting object to investigate its formation history. Globular clusters are a great tracer of the formation history of early-type galaxies, so that we study the globular cluster system of M85. It has been already found that there are "intermediate-color" globular clusters as well as blue and red ones based on the photometric survey using CFHT/Megacam. For follow-up research, we obtain the spectra of 21 globular clusters in the central region of M85 using Gemini-N/GMOS. We estimate their ages and metallicities based on the strength of Lick indices. We detect the intermediate-age population (~ 2 Gyr) with solar metallicities, comprising about 50% of the observed globular clusters, as well as old and metal-poor population. It suggests that M85 experienced a major merging event around 2 Gyr ago. We discuss these results regarding to the formation history of M85.