• 천문학회보
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• 제45권1호
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• pp.58.1-58.1
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• 2020

The Multipupose InfraRed Imaging System (MIRIS) Paα Galactic Plane Survey (MIPAPS) covers the whole Galactic plane with the latitude range of -3° < b < +3°. Next to the first result in l = 96°-116° (Cepheus), we present the results in l = 276°-296° (Carina). This region with the direction toward the inner Galaxy, has much higher extinction but much more Paα-emitting sources than Cepheus. We list up the detected Paα sources, and compare them with the WISE H II region catalog (there are 308 H II regions and candidates in this region) and VPHAS+ Hα image. By detecting the Paα and Hα recombination lines, 71 H II region candidates are newly confirmed as definite H II regions, out of which 53 H II regions are detected at Paα. For the Paα-detected sources, we measure the Paα and Hα fluxes and estimate the E(B-V) color excesses for the extended sources.

• 한국의류학회지
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• 제18권5호
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• pp.749-764
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• 1994

It was assumed that a consumer forms images of all the factors related to clothing merchandise such as trademarks, stores, products and prices that he/she perceives in the market and those images deforming his/her preference for a particular piece of clothes and intention of purchase. Under this assumption, this research was designed to find out important factors of clothes that help a consumer form an image of the clothes, among other attributes of the merchandise, and how this image is related to the existing extraneous variables such as the trademark image, the consumer's self image, the price, etc. in leading the consumer to purchase the particular clothes in the end. In the empirical research, a preliminary survey was conducted to select brands of womenswear that were suitable for this study and as the result, 16 brands were chosen. Then one trademark, one store and two products from each of the 16 brands were selected. With these materials, 32 stimulus sheets were prepared, and each of them was composed of 3 photos of a brand's catalog and logo, the interior of a selected store that carried products of the brand, and formal suits selected from each brand's spring/summer 1993 collections. Subjects were 460 women in the age groups of 20-50s who live in Seoul Metropolitan area. Each of the subjects was provided with a survey questionnaire and 16 stimulus sheets. The main findings of this research prove that consumers follow a certain selection process model when they purchase clothes: consumers, first, from images of merchandise based on the trademarks, stares, and products and those formed images work il.: medium variables and in the end they help the consumers decide whether to buy the products.

• 천문학회보
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• 제36권2호
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• pp.113.1-113.1
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• 2011

The Leo ring in the M96 group is unique in its morphology and size among the intergalactic gas features found in nearby universe. Its ring-like structure of 200 kpc on diameter appears to be orbiting around the M105-NGC 3384 pair with $1.67{\times}109\;M{\odot}$ of HI gas. While the origin of the ring - whether it is primordial or tidally stripped - is yet unclear, the optical and gas properties of dwarf galaxies associated with the gas ring help us to understand the formation process of this large scale intergalactic HI cloud. At the first step, we present the optical catalog of dwarf galaxy candidates in the Leo ring using deep optical images with MegaCam on the CFHT. Image convolution method is used in order to detect very faint dwarf galaxies. Comparing the ALFALFA HI data from the literature, we have identified that 4 dwarf candidates coexist with HI clumps. There are also 27 HI dwarfs with no optical counterpart and 12 optical dwarfs with no HI clump. In this work, we probe the optical and global gas properties of these dwarfs.

• 천문학회보
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• 제43권2호
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• pp.57.2-57.2
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• 2018

In astronomical observation, sequential device control and real-time data processing are important to maximize observing efficiency. We have developed series of automatic observing software (KAOS, KHU Automatic Observing Software), e.g. KAOS30 for the 30 inch telescope in the McDonald Observatory and KAOS76 for the 76 cm telescope in the KHAO. The series consist of four packages: the DAP (Data Acquisition Package) for CCD Camera control, the TCP (Telescope Control Package) for telescope control, the AFP (Auto Focus Package) for focusing, and the SMP (Script Mode Package) for automation of sequences. In this poster, we introduce KAOS10 which is being developed for controlling a small telescope such as aperture size of 10 cm. The hardware components are the QHY8pro CCD, the QHY5-II CMOS, the iOptron CEM 25 mount, and the Stellarvue SV102ED telescope. The devices are controlled on ASCOM Platform. In addition to the previous packages (DAP, SMP, TCP), KAOS10 has QLP (Quick Look Package) and astrometry function in the TCP. QHY8pro CCD has RGB Bayer matrix and the QLP transforms RGB images into BVR images in real-time. The TCP includes astrometry function which adjusts the telescope position by comparing the image with a star catalog. In the future, We expect KAOS10 be used on the research of transient objects such as a variable star.

• KSII Transactions on Internet and Information Systems (TIIS)
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• 제14권4호
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• pp.1543-1561
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• 2020

Taxonomy of human brain activity is a complicated rather challenging procedure. Due to its multifaceted aspects, including experiment design, stimuli selection and presentation of images other than feature extraction and selection techniques, foster its challenging nature. Although, researchers have focused various methods to create taxonomy of human brain activity, however use of multivariate pattern analysis (MVPA) for image recognition to catalog the human brain activities is scarce. Moreover, experiment design is a complex procedure and selection of image type, color and order is challenging too. Thus, this research bridge the gap by using MVPA to create taxonomy of human brain activity for different categories of images, both colored and gray scale. In this regard, experiment is conducted through EEG testing technique, with feature extraction, selection and classification approaches to collect data from prequalified criteria of 25 graduates of University Technology PETRONAS (UTP). These participants are shown both colored and gray scale images to record accuracy and reaction time. The results showed that colored images produces better end result in terms of accuracy and response time using wavelet transform, t-test and support vector machine. This research resulted that MVPA is a better approach for the analysis of EEG data as more useful information can be extracted from the brain using colored images. This research discusses a detail behavior of human brain based on the color and gray scale images for the specific and unique task. This research contributes to further improve the decoding of human brain with increased accuracy. Besides, such experiment settings can be implemented and contribute to other areas of medical, military, business, lie detection and many others.

• 한국문헌정보학회지
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• 제42권3호
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• pp.61-79
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• 2008

본 연구는 해외 소장 고문헌의 DB구축과 공동활용 방안을 다루기 위해 해외 소장 고문헌의 정리. 해외 소장 고문헌 DB 시스템의 문제점 및 개선방안. 해외 소장 고문헌의 공동활용 방안을 다룬 것이다. 본 연구를 통해 밝혀진 사실은 다음과 같다. 해외 소장의 고문헌을 정리하기 시작한 것은 국립중앙도서관이 1982년부터 해외기관에 소장된 고문헌을 영인하여 간략목록으로 발행하는 차원에서 시작되었다. 려강출판사가 일본소재 한국고문헌목록 1-4를 발간하여 기초자료로 제공하였다. 국립문화재연구소는 일본, 미국. 프랑스 등의 해외기관에 소장된 고문헌을 조사하여 일부의 목록집을 발행하였고. 국사편찬위원회는 일본소재 고문서 목록을 조사하고 그중 가치 있는 것을 선별하여 목록으로 간행하였다. 해외 소장 고문헌의 DB 시스템에서는 국립중앙도서관의 한국고전적종합목록시스템, 국립문화재연구소의 해외소장한국전적문화재시스템, 국사편찬위원회의 한국사데이터베이스시스템 및 NF목록/원문서비스시스템의 특성이 기술되었고, 각 DB상의 문제점이 파악되었으며 그에 대한 몇 가지 대안도 제시되었다. 공동활용 방안에 있어서는 고문서 정리를 위한 목록 형식 덴 기술(시안)은 새로운 표준안으로 채택될 수 있도록 수정되어야 하고, 관련 기간들은 서지기록을 작성하거나 원문 텍스트를 디지타이징할 때 표준을 준수해야 한다. 고문헌의 DB 구축과 관리를 위한 전문 인력의 양성과 교육이 이루어져야 한다. 긍극적으로는 디지털화된 자원의 공유를 위한 기술개발, 고문헌 컨텐츠의 이용과 개선, 공공의 이용과 참여, 국제적이 이용이 가능하도록 할 수 있는 국가차원의 전담기구가 설립되어야 한다.

• 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.

• 한국기록관리학회지
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• 제2권1호
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• pp.119-131
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• 2002

본 연구는 디지털도서관 콘텐츠를 관리할 KORMARC/EAD 통합시스템을 설계하고 구현하였다. 본 연 구의 목적은 명지대학 디지털도서관의 국제한국학 콜렉션과 단행본을 관리할 메타데이터를 설계하고 아울러 기록물정보관리의 모형 구축을 위한 기초 자료를 제시하는 것을 목적으로 한다. 메타데이터를 설계하기 위해서 기록물의 목록 규칙과 관련된 네 가지 종류의 자료 즉 국제표준기록물기술[ISAD(G)], 미국 기록물/필사본 기계가독목록(USMARC AMC), EAD 및 Ebind를 참조하였다. 시스템은 검색 모드와 입력 모드로 구성된다. 검색은 KORMARC를 이용하여 단행본과 콜렉션을 통합 검색할 수 있으며 콜렉션인 경우 링크를 통해서 EAD/XML을 활용한 인벤토리로 연결된다. 인벤토리는 기록물에 대한 상세 정보 뿐 아니라 PDF 형식의 전문 이미지 데이터를 제공하며 단행본인 경우 KORMARC 의 856 태그를 이용하여 전문 이미지 데이터를 제공한다. 입력 모드는 목록과 인벤토리 정보를 입력할 수 있는 스크린을 제공한다. 시스템에 대한 이용자 만족도, 시스템의 개선점 및 향후 콜렉션을 포함한 다양한 기록물 관리 시스템을 구현하기 위한 기초 자료를 얻기 위하여 설문지를 이용하여 시스템을 평가해 보았다. 평가 분석 결과는 향후 시스템을 갱신할 때 활용할 수 있도록 정리하였고, 제안된 시스템이 좀 더 개선되기 위한 방안 세가지를 끝으로 제시하였다.

• 정보보호학회논문지
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• 제30권6호
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• pp.967-973
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• 2020

전략물자관리 제도의 이행 확산에 따라 전략물자 판정의 중요성이 높아지고 있으나 전략물자 제도를 처음 접하는 수출기업은 전략물자의 개념을 이해하기 쉽지 않고, 전략물자를 통제하는 기준이 다양하여 전략물자 판정에 어려움이 따른다. 본 논문에서는 전략물자 제도를 처음 접하는 기업이나 전략물자 판정시스템 이용자에게 진입장벽을 낮추어 판정이라는 과정을 쉽게 접근할 수 있는 방법을 제안한다. 이용자가 전략물자 판정이라는 절차를 매뉴얼이나 카탈로그의 제공만으로 판정결과를 확인할 수 있게 된다면, 전략물자 판정 방법과 절차에 보다 편리하고 쉽게 다가설 수 있을 것이다. 본 연구 목적을 달성하기 위해 이미지 인식 및 분류에서 연구되고 있는 딥러닝과 OCR(광학문자판독) 기술을 활용하고, 전략물자 판정 지원도구에 대한 개발과 연구를 통하여 우리 기업의 전략물자 판정에 도움이 되는 정보를 제공한다.

• 천문학회보
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• 제46권1호
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• pp.57.3-58
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• 2021

We performed three-dimensional Monte Carlo dust scattering radiative transfer simulations for FUV light to obtain dust scattered FUV images and compared them with the observed FUV image obtained by FIMS/SPEAR and GALEX. From this, we find the scattering properties of interstellar dust in our Galaxy and suggest the intensity of extragalactic background light (EBL) at FUV wavelength. The best-fit values of the scattering properties of interstellar dust are albedo = 0.38^-0.04_+0.04, g-factor = 0.55^-0.15_+0.10, and EBL = 138^-23₊₂₁ CU for the allsky which are consistent well with the Milky Way dust model of Draine and direct measurements of Gardner et al., respectively. At the high Galactic latitude of |b|>10°, the observation is well fitted with the model of lower albedo = 0.35^-0.04_+0.06 and g-factor = 0.50^-0.20_+0.15. On the contrary, the scattering properties of interstellar dust show higher albedo = 0.43^-0.02_+0.02 and g-factor = 0.65^-0.15_+0.05 near the Galactic plane of |b|<10°. In the present simulation, recent three-dimensional distribution maps of interstellar dust in our Galaxy, stellar distances in the catalog of GAIA DR2, and FUV fluxes and/or spectral types in the TD-1 and Hipparcos star catalogs were used.