• 한국통신학회논문지
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• 제30권5C호
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• pp.313-319
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• 2005

이 논문에서는, 상관 (correlation) 성질이 비동기 (asynchronous) 4-위상 신호 방식에 알맞은 다상 (polyphase)수열 집합을 제안한다. 제안한 수열과 이진 의사잡음 (pseudo-noise: PN) 수열을 서명수열로 (signature sequence)쓸 때 직접수열 부호분할 다중접속 (direct sequence code division multiple access: DS/CDMA) 시스템의 성능을 견주어 본다. 최대 절대 상관값으로 (maximum magnitude of correlations) 분석한 최악 성능과 모의 실험으로 얻은 평균 비트오류율 성능 모두에서 제안한 수열을 쓰면 이진 의사잡음 수열을 쓸 때보다 시스템 성능이 더 나음을 보인다.

• International Journal of Fuzzy Logic and Intelligent Systems
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• 제15권3호
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• pp.145-152
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• 2015

We consider an online selective-sample learning problem for sequence classification, where the goal is to learn a predictive model using a stream of data samples whose class labels can be selectively queried by the algorithm. Given that there is a limit to the total number of queries permitted, the key issue is choosing the most informative and salient samples for their class labels to be queried. Recently, several aggressive selective-sample algorithms have been proposed under a linear model for static (non-sequential) binary classification. We extend the idea to hidden Markov models for multi-class sequence classification by introducing reasonable measures for the novelty and prediction confidence of the incoming sample with respect to the current model, on which the query decision is based. For several sequence classification datasets/tasks in online learning setups, we demonstrate the effectiveness of the proposed approach.

• 한국전자통신학회논문지
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• 제6권4호
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• pp.539-544
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• 2011

적당한 정수 $n({\geq}1)$에 대하여 2-valued 자기상관관계를 갖는 주기가 $2^n-1$인 균형 이진 수열(balanced binary sequences)은 대역확산 통신 시스템(spread-spectrum communication system)에서 많이 응용되고 있다. 본 논문에서는 르장드르 수열에 의해 구성되는 새로운 3-valued 비선형 이진 수열을 제안한다. 이 수열은 유한체 위에서 트레이스를 이용해 생성하는 가장 우수한 수열인 m-수열, GMW 수열, Kasami 수열, No 수열을 모두 포함한다. 제안된 수열은 Klapper에 의해 제안된 이차형식 수열보다 더 낮은 상호상관관계를 갖는다.

• 한국항행학회논문지
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• 제15권5호
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• pp.735-741
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• 2011

본 논문에서는 고속 Binary CDMA 시스템에서 신호대잡음비의 추정 오차가 MMSE-DFE의 BER 성능에 미치는 영향을 분석하였다. MMSE 등화 알고리즘은 입력신호의 신호대잡음비 값이 필요하기 때문에, 프리엠블의 CAZAC 시퀀스로부터 신호대잡음비를 추정해야한다. 그러나 잡음과 ISI가 존재하는 환경에서는 정확한 신호대잡음비 추정이 불가능하므로 추정 오차가 발생하고, 이로 인해 등화기의 성능이 열화된다. 본 논문의 실험 결과는 MMSE-DFE 설계시에 SNR 추정 알고리즘의 선택 기준으로 활용될 수 있다.

• 천문학논총
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• 제30권2호
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• pp.201-204
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• 2015

The common-envelope process is a complicated phase in binary evolution. A lot of effort has been dedicated to study the common-envelope stage, but many questions related to this process are yet to be answered. If one member of the binary survives the common-envelope phase, the binary will emerge as a white dwarf accompanied by a low-mass main sequence star in close orbit, often referred as a post common-envelope binary (PCEB). SDSS J0745+2631 is among the list of newly found PCEBs from the Sloan Digital Sky Survey (SDSS). This star is proposed to be a strong eclipsing system candidate due to the ellipsoidal modulation in its light curve. In this work, we aim to confirm the eclipsing nature of SDSS J0745+2631 and to determine the stellar and orbital parameters using the software Binary Maker 3.0 (BM3.0). We detected the primary eclipse in the light curve of SDSS J0745+2631 in our follow-up observation from January 2014 using the ULTRASPEC instrument at the Thai National Observatory. The data obtained on 7th and 8th January 2014 in g filter show an evident drop in brightness during the eclipse of the white dwarf, but this eclipse is less prominent in the data taken on the next night using a clear filter. According to our preliminary model, we find that SDSS J0745+2631 hosts a rather hot white dwarf with an effective temperature of 11500K. The companion star is a red dwarf star with a temperature of 3800K and radius of 0.3100 $R_{\odot}$. The red dwarf star almost fills its Roche lobe, causing a large ellipsoidal modulation. The mass ratio of the binary given by the Binary Maker 3.0 (BM3.0) model is M2/M1 = 0.33.

• 천문학회지
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• 제25권1호
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• pp.47-64
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• 1992

Cores of globular clusters are an ideal place for close encounters between stars. The outcome of tidal capture can be stellar mergers, close binaries between normal stars (W UMa type), cataclysmic variables composed of white dwarf and normal star pairs, or low-mass X-ray binaries consisting of a neutron star and a normal star pairs. Stellar mergers can be the origin of blue stragglers in dense globular clusters although they are hard to observe. Low mass X-ray binaries would eventually become binary pulsars with short pulse periods after the neutron stars accrete sufficient amount of matter from the companion. However, large number of recently discovered, isolated millisecond pulsars (as opposed to binary pulsars) in globular clusters may imply that they do not have to gain angular speeds during the X-ray binary phase. We propose that these isolated millisecond pulsars may have formed through the disruptive encounters, which lead to the formation of accretion disk without Roche lobe filling companion, between a neutron star and a main-sequence star. Based on recently developed multicomponent models for the dynamical evolution of globular clusters, we compute the expected numbers of various systems formed by tidal capture as a function of time.

• ETRI Journal
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• 제35권6호
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• pp.1021-1028
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• 2013

Automatic facial expression recognition is a widely studied problem in computer vision and human-robot interaction. There has been a range of studies for representing facial descriptors for facial expression recognition. Some prominent descriptors were presented in the first facial expression recognition and analysis challenge (FERA2011). In that competition, the Local Gabor Binary Pattern Histogram Sequence descriptor showed the most powerful description capability. In this paper, we introduce hybrid facial representations for facial expression recognition, which have more powerful description capability with lower dimensionality. Our descriptors consist of a block-based descriptor and a pixel-based descriptor. The block-based descriptor represents the micro-orientation and micro-geometric structure information. The pixel-based descriptor represents texture information. We validate our descriptors on two public databases, and the results show that our descriptors perform well with a relatively low dimensionality.

• 한국통신학회논문지
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• 제41권12호
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• pp.1742-1744
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• 2016

본 논문은 짧은 길이의 LDPC 부호의 복호 성능을 위해 제안된 이진 섭동 복호기와 에프터버너 복호기가 동등함을 증명하였다.

• 정보처리학회논문지C
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• 제10C권7호
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• pp.851-856
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• 2003

LM 발생기는 합산 수열 발생기가 갖고 있는 최대 주기, 최대 근사 선형복잡도 및 최고 차수 상관면역도를 동시에 만족하는 발생기이며, 입출력 무상관 발생기이다. 본 논문에서는 LM 발생기를 고속화 구현하기 위하여 m-병렬 LM 수열 발생기(m-parallel LM-BSG, Lee-Moon Binary Sequence Generator)를 제안하였으며, m＝8인 병렬 발생기(8-parallel LM-BSG)를 세부 설계한다. 기존의 스트림 암호와 비교할 때, 제안된 알고리듬은 같은 안전성을 유지하면서 속도가 m＝8배 빨라짐을 알 수 있었다.

• 천문학회보
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• 제44권2호
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• pp.60.3-60.3
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• 2019

Binary systems of a white dwarf showing mass transfer activities are classified into cataclysmic variables and symbiotic stars. In the case of cataclysmic variables, the companion is usually a late type main sequence star filling its Roche lobe, where material is transferred through the inner Lagrangian point to form an accretion disk around the white dwarf. The disk becomes unstable and highly viscous when the surface density exceeds the critical density, leading to dwarf nova outbursts. In contrast, symbiotic stars are wide binary systems having a giant as the mass donor. Some fraction of giant stellar wind is accreted to the white dwarf giving rise to various symbiotic activities. In particular, half of symbiotics show Raman O VI at 6830 and 7088, which are important spectroscopic probe of mass transfer process. Monitoring observations using 1 m class telescopes will produce valuable information regarding the mass loss and mass transfer to white dwarf stars, shedding much light on the last stage of stellar evolution of low and intermediate mass stars.