• 대한전자공학회논문지SP
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• 제44권5호
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• pp.28-34
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• 2007

위성 영상에서 도로를 효과적으로 추출하기 위한 히스토그램 기반 도로 경계선 추출자를 제안하였다. 제안한 추출자를 이용해 도로 경계선 양측의 도로와 비도로 영역 각 화소의 방향성 히스토그램 차를 계산하고, 그 에지 강도 맵을 구하여 도로의 경계선을 추출하였다. 그리고 원영상과 분할된 도로 군집 영상의 에지 강도 맵을 계층적으로 구하여 직선 도로와 곡선 도로를 추출한 다음, 도로의 연결성을 기반으로 하여 전체 도로망을 구성하였다. 제안한 추출자는 칼라 유사도를 계산하는 기존 방법과 달리 히스토그램 차를 기반으로 하기 때문에 잡영에 강건하게 도로를 추출할 수 있으며, 도로 경계선의 위치와 도로 폭도 함께 추출할 수 있을 뿐만 아니라 도로군집을 자동식별하기 때문에 다양한 분광특성의 도로들도 쉽게 추출할 수 있다. 제안한 추출자를 이용하여 1m의 공간 해상도를 갖는 IKONOS 위성 영상에 대해 실험하여 잡영에 강건하게 도로가 추출됨을 확인하였고, 직선 도로 뿐만 아니라 곡선도로 추출도 용이함을 확인하였다.

• 한국컴퓨터정보학회논문지
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• 제29권5호
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• pp.155-164
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• 2024

본 연구는 ESG 등급이 제공되지 않는 국내 공공기관의 ESG 등급을 추정하는 비지도 학습 기반 군집모형을 제안한다. 이를 위해, 스펙트럼 군집과 k-means 군집에서 최적의 클러스터 수를 비교했고, 그 결과의 신뢰성을 보장하기 위해 성능지표인 Davies-Bouldin Index (DBI)를 계산했다. 결과적으로, 스펙트럼 군집과 k-means 군집에서 각각 0.734 및 1.715의 DBI 값을 산출했는데, 이는 값이 작을수록 우수한 성능을 의미하므로 스펙트럼 군집의 우수성을 확인하였다. 게다가, T-검정 및 ANOVA를 이용하여 ESG 비재무 데이터 간 통계적으로 유의미한 차이를 밝혀내고, 상관계수를 이용하여 ESG 항목 간 상관관계를 확인했다. 본 연구는 이러한 결과를 바탕으로 기존 ESG 등급 없이 공공기관별 ESG 성과 순위를 추정할 가능성을 제시한다. 이는 최적의 클러스터 수를 계산한 다음, 각 클러스터 내 ESG 데이터의 평균 총합을 결정함으로써 달성된다. 따라서, 제안된 모델은 다양한 국내 공공기관의 ESG 등급을 평가하는 근거로 활용될 수 있고, 국내 지속가능경영 실천과 성과관리에 유용할 것으로 기대된다.

• 천문학회보
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• 제37권2호
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• pp.81-81
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• 2012

Since the ultraviolet (UV) flux of an integrated population is a good tracer of recent star formation activities, UV observations provide an important constraint on star formation history (SFH) in galaxies. We present UV color-magnitude relations (CMRs) of early-type dwarf galaxies in the Virgo cluster, based on Galaxy Evolution Explorer (GALEX) UV data and the Extended Virgo Cluster Catalog (EVCC, Kim, S. in prep.). The EVCC covers an area 5.4 times larger (750 deg2) than the footprint of the classical Virgo cluster catalog by Binggeli and collaborators. We secure 1304 galaxies as members of the Virgo cluster and 526 galaxies of them are new objects not contained in the VCC. Morphological classification of galaxies in the EVCC is based on the optical image ("Primary Classification") and spectral feature ("Secondary Classification") of the SDSS data. We find that dwarf lenticular galaxies (dS0s) show a surprisingly distinct and tight locus separated from that of ordinary dwarf elliptical galaxies (dEs), which is not clearly seen in previous CMRs. The dS0s in UV CMRs follow a steeper sequence than dEs and show bluer UV-optical color at a given magnitude. Most early type dwarf galaxies with blue UV colors (FUV-r < 6 and NUV-r < 4) are identified as those showing spectroscopic hints of recent or ongoing star formation activities. We explore the observed CMRs with population models of a luminosity-dependent delayed exponential star formation history. The observed CMR of dS0s is well matched with models with relatively long delayed star formation. Our results suggest that dS0s are most likely transitional objects at the stage of subsequent transformation of late-type progenitors to ordinary red dEs in the cluster environment. In any case, UV photometry provides a powerful tool to disentangle the diverse subpopulations of early-type dwarf galaxies and uncover their evolutionary histories.

• ETRI Journal
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• 제40권2호
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• pp.227-236
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• 2018

Ultra-dense small cell networks (UD-SCNs) have been identified as a promising scheme for next-generation wireless networks capable of meeting the ever-increasing demand for higher transmission rates and better quality of service. However, UD-SCNs will inevitably suffer from severe interference among the small cell base stations, which will lower their spectral efficiency. In this paper, we propose a software-defined networking (SDN)-based hierarchical agglomerative clustering (SDN-HAC) framework, which leverages SDN to centrally control all sub-channels in the network, and decides on cluster merging using a similarity criterion based on a suitability function. We evaluate the proposed algorithm through simulation. The obtained results show that the proposed algorithm performs well and improves system payoff by 18.19% and 436.34% when compared with the traditional network architecture algorithms and non-cooperative scenarios, respectively.

• 천문학회지
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• 제49권3호
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• pp.83-92
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• 2016

The Toothbrush radio relic associated with the merging cluster 1RXS J060303.3 is presumed to be produced by relativistic electrons accelerated at merger-driven shocks. Since the shock Mach number inferred from the observed radio spectral index, M_radio ≈ 2.8, is larger than that estimated from X-ray observations, M_X ≲ 1.5, we consider the re-acceleration model in which a weak shock of M_s ≈ 1.2 - 1.5 sweeps through the intracluster plasma with a preshock population of relativistic electrons. We find the models with a power-law momentum spectrum with the slope, s ≈ 4.6, and the cutoff Lorentz factor, γ_e,c ≈ 7-8×10⁴ can reproduce reasonably well the observed profiles of radio uxes and integrated radio spectrum of the head portion of the Toothbrush relic. This study confirms the strong connection between the ubiquitous presence of fossil relativistic plasma originated from AGNs and the shock-acceleration model of radio relics in the intracluster medium.

• 천문학회지
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• 제37권5호
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• pp.471-476
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• 2004

We propose an analytical model to estimate the influence of a merger on the thermal SZ effect. Following observations we distinguish between subsonic and transonic mergers. Using analytical velocity fields and the Bernoulli equation we calculate the excess pressure around a moving subcluster for an incompressible subsonic gas. Positive excess around the stagnation point and negative excess on the side of the subcluster lead to characteristic signatures in the SZ map, of the order of $10\%$ compared to the unperturbed signal. For a transonic merger we calculate the change in the thermal spectral SZ function, resulting from bow shock accelerated electrons. The merger shock compression factor determines the power law tail of the new non-thermal electron population and is directly related to a shift in the crossover frequency. This shift is typically a few percent towards higher frequencies.

• 천문학회지
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• 제32권2호
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• pp.75-82
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• 1999

Diffuse radio emission in Abell 2256 was detected above 3 $\sigma$ with DRAO observations at 1420 MHz. The halo size is $\~13' {\times}10' (\~1h^{-1}_{50}\;Mpc$) in full extent and is elongated along a position angle of about $112^{\circ}$. The total flux density contained in the halo is 30$\pm$10 mJy at 1420 MHz and its spectral index is -2.04$\pm$0.04, showing no evidence for steepening up to 1420 MHz. Using the size estimate, yields a more reliable equipartition magnetic field strength which is $0.34(1 + k)^{2/7}{\mu}G$. In addition, five new radio sources are identified.

• 제어로봇시스템학회:학술대회논문집
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• 제어로봇시스템학회 1996년도 한국자동제어학술회의논문집(국내학술편); 포항공과대학교, 포항; 24-26 Oct. 1996
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• pp.343-346
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• 1996

A new method for on-line induction motor fault detection is presented in this paper. This system utilizes unsupervised-learning clustering algorithm, the Dignet, proposed by Thomopoulos etc., to learn the spectral characteristics of a good motor operating on-line. After a sufficient training period, the Dignet signals one-phase ground fault, or a potential failure condition when a new cluster is formed and persists for some time. Since a fault condition is found by comparison to a prior condition of the machine, on-line failure prediction is possible with this system without requiring information on the motor of load characteristics.

• KSII Transactions on Internet and Information Systems (TIIS)
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• 제14권8호
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• pp.3257-3269
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• 2020

Articulation disorders are characterized by an inability to achieve clear pronunciation due to misuse of the articulators. In this paper, a method of detecting such disorders by comparing to the standard pronunciations is proposed. This method defines the standard pronunciations from the speeches of normal children by clustering them with three features which are the Linear Predictive Cepstral Coefficient (LPCC), the Mel-Frequency Cepstral Coefficient (MFCC), and the Relative Spectral Analysis Perceptual Linear Prediction (RASTA-PLP). By calculating the distance between the centroid of the standard pronunciation and the inputted pronunciation, disordered speech whose features locates outside the cluster is detected. 89 children (58 of normal children and 31 of children with disorders) were recruited. 35 U-TAP test words were selected and each word's standard pronunciation is made from normal children and compared to each pronunciation of children with disorders. In the experiments, the pronunciations with disorders were successfully distinguished from the standard pronunciations.

• 천문학회지
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• 제16권1호
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• pp.23-30
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• 1983

About two hundred stars within 50 pc from the sun, whose tangential velocity larger than 100 km/sec, have been selected on the basis of their proper motions and trigonometric parallaxes. A list of them along with their photoelectric UBV data and spectral types is given. The criterion on the tangential velocity, $v_t$ > 132 km/sec, was adopted for selection of high-velocity stars. The H-R diagram of these nearby high-velocity stars resembles that of a globular cluster, with the turnoff around $B-V{\approx}0.35$ and $M_v{\approx}4.0$, and the subdwarfs among these high-velocity stars are fainter than the main-sequence stars of Hyades by the amount of $1^m.25{\pm}0^m.30$ in the region with B-V < 1.40 on the average.