• 제목/요약/키워드: Catalog Function

검색결과 66건 처리시간 0.025초

3D CAD 데이터 기반의 제조기업 지원서비스를 위한 소프트웨어 플랫폼 설계 (Design of a Software Platform to Support Manufacturing Enterprises Using 3D CAD Data)

  • 권혁진;윤주성;오요셉;이주연;김보현
    • 한국CDE학회논문집
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    • 제19권4호
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    • pp.434-442
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    • 2014
  • Most manufacturing enterprises create CAD data as a result of the product/part design process; however, the CAD data is being utilized only for production activities. Besides the processes directly related to manufacturing such as design and production, the CAD data is an important resource that can be used in variety of services (e.g., catalog production and production manuals) for manufacturing enterprises. This study proposes a software platform that can support a wide range of services for manufacturing companies in an efficient and productive way. The software platform was designed based on the functions identified by requirement analysis. The platform consists of four layers: data model layer to manage relevant data; library layer and common function layer to configure services; and application layer to install and run the software. Finally, this study evaluates the validity of the proposed platform architecture by applying it to the digital catalog system.

전자 상거래의 이미지 공유를 위한 웹 이미지 서버의 성능 평가 (Performance Evaluation of Web Image Server for sharing e-Commerce System's Image)

  • 김명은;조동섭
    • 정보처리학회논문지B
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    • 제9B권5호
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    • pp.533-540
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    • 2002
  • 인터넷 전자상거래의 발달로 데스크 탑 컴퓨터만이 아니라 냉장고, 달리는 차 안, PDA 휴대 전화 등 생활 영역 곳곳에서도 전자상거래를 할 수 있다. 다양한 기기들에서 전자상거래를 하기 위해 쇼핑몰들은 여러 화질의 이미지를 제공해야 한다. 현재의 전자상거래 시스템을 같은 상품 이미지라도 쇼핑몰들이 각각 저장하고 있다. 웹 이미지 서버는 쇼핑몰이 더 이상 이미지를 저장하지 않도록 이미지를 제공하는 중앙 집중적인 이미지 저장소이다. 따라서, 웹 이미지 서버를 이용하면 여러 쇼핑몰의 저장공간을 간편화할 수 있다. 또한, 이미지를 효율적으로 사용할 수 있고 쇼핑몰의 이미지의 갱신과 관리가 쉽게 이루어질 수 있다. 본 논문에서는 기존에 구현된 웹 이미지 서버를 쇼핑몰 관리 기능, 사용자 로그 기록 기능과 이미지 카탈로그 기능을 추가하여 확장하였고, 웹 서버 성능 평가 툴인 WAS를 이용하여 웹 이미지 서버 시스템의 응답시간을 측정하여 비교하였고, 사용자를 계속 증가시켜 웹 이미지 서버의 안전성을 평가하였다.

CORRELATION FUNCTIONS OF THE ABELL, APM, AND X-RAY CLUSTERS OF GALAXIES

  • LEE SUNGHO;PARK CHANGBOM
    • 천문학회지
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    • 제35권3호
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    • pp.111-121
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    • 2002
  • We have measured the correlation functions of the optically selected clusters of galaxies in the Abell and the APM catalogs, and of the X-ray clusters in the X-ray-Brightest Abell-type Clusters of galaxies (XBACs) catalog and the Brightest Clusters Sample (BCS). The same analysis method and the same method of characterizing the resulting correlation functions are applied to all observational samples. We have found that the amplitude of the correlation function of the APM clusters is much higher than what has been previously claimed, in particular for richer subsamples. The correlation length of the APM clusters with the richness R $\ge$ 70 (as defined by the APM team) is found to be $r_0 = 25.4_{-3.0}^{+3.1}\;h^{-1}$ Mpc. The amplitude of correlation function is about 2.4 times higher than that of Croft et al. (1997). The correlation lengths of the Abell clusters with the richness class RC $\ge$ 0 and 1 are measured to be $r_0 = 17.4_{-1.1}^{+1.2}$ and $21.0_{-2.8}^{+2.8}\;h^{-1}$ Mpc, respectively, which is consistent with our results for the APM sample at the similar level of richness. The richness dependence of cluster correlations is found to be $r_0= 0.40d_c + 3.2$ where $d_c$ is the mean intercluster separation. This is identical in slope with the Bahcall & West (1992)'s estimate, but is inconsistent with the weak dependence of Croft et al. (1997). The X-ray bright Abell clusters in the XBACs catalog and the X-ray selected clusters in the BCS catalog show strong clustering. The correlation length of the XBACs clusters with $L_x {\ge}0.65{\times} 10^{44}\;h^{-2}erg\;s^{-1}$ is $30.3_{-6.5}^{+8.2}\;h^{-1}$ Mpc, and that of the BCS clusters with $L_x {\ge}0.70{\times} 10^{44}\;h^{-2}erg\;s^{-1}$ is $30.2_{-8.9}^{+9.8}\;h^{-1}$ Mpc. The clustering strength of the X-ray clusters is much weaker than what is expected from the optical clusters.

New Galaxy Catalog of the Virgo Cluster

  • Kim, Suk;Rey, Soo-Chang;Jerjen, Helmut;Lisker, Thorsten;Sung, Eon-Chang;Lee, Youngdae;Chung, Jiwon;Pak, Mina;Yi, Wonhyeong;Lee, Woong
    • 천문학회보
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    • 제39권2호
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    • pp.50-50
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    • 2014
  • We present a new catalog of galaxies in the wider region of the Virgo cluster, based on the Sloan Digital Sky Survey (SDSS) Data Release 7. The Extended Virgo Cluster Catalog (EVCC) covers an area of 725 deg2 or 60.1 Mpc2. It is 5.2 times larger than the footprint of the classical Virgo Cluster Catalog (VCC) and reaches out to 3.5 times the virial radius of the Virgo cluster. We selected 1324 spectroscopically targeted galaxies with radial velocities less than 3000 km s-1. In addition, 265 galaxies that have been missed in the SDSS spectroscopic survey but have available redshifts in the NASA Extragalactic Database are also included. Our selection process secured a total of 1589 galaxies of which 676 galaxies are not included in the VCC. The certain and possible cluster members are defined by means of redshift comparison with a cluster infall model. We employed two independent and complementary galaxy classification schemes: the traditional morphological classification based on the visual inspection of optical images and a characterization of galaxies from their spectroscopic features. SDSS u, g, r, i, and z passband photometry of all EVCC galaxies was performed using Source Extractor. We compare the EVCC galaxies with the VCC in terms of morphology, spatial distribution, and luminosity function. The EVCC defines a comprehensive galaxy sample covering a wider range in galaxy density that is significantly different from the inner region of the Virgo cluster. It will be the foundation for forthcoming galaxy evolution studies in the extended Virgo cluster region, complementing ongoing and planned Virgo cluster surveys at various wavelengths.

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Open API를 이용한 서지레코드와 목록 확장에 관한 연구 (A Study on the Bibliographic Records and the Expansion of Library Catalog Using Open API)

  • 구중억;이응봉
    • 한국문헌정보학회지
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    • 제43권2호
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    • pp.299-328
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    • 2009
  • 본 연구에서는 네이버, 다음, 알라딘, Amazon, Google, KERIS, LibraryThing, OCLC 등 8개의 도서용 Open API 현황을 비교 분석하였다. 그리고 C대학교 도서관의 서지레코드에서 '광학'(DDC 535) 분류 167건의 표본 서지레코드를 선정하여 Open API의 활용성을 비교 분석하였다. 이러한 분석결과를 토대로 Open API를 이용한 서지레코드의 접근점 기능 확대와 목록 확장에 유용하다고 판단되는 12개의 Open API 적용 모형을 실험적으로 구현하였다. 또 통합서지용 KORMARC 001, 010, 012, 020, 035, 246, 505, 520, 850, 856 필드들을 대상으로 Open API를 이용하여 서지레코드의 접근점 기능 확대와 목록 확장방안들을 고찰하였다. 마지막으로 표본 서지레코드의 OPAC 검색결과 간략화면과 상세화면을 대상으로 Open API를 이용하여 목록 확장방안들을 예시로 구현하였다.

전자 카탈로그에 대한 효율적인 색인어 통계 정보 관리 방법 (Efficient Management of Statistical Information of Keywords on E-Catalogs)

  • 이동주;황인범;이상구
    • 한국전자거래학회지
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    • 제14권4호
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    • pp.1-17
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    • 2009
  • 전자 카탈로그는 상품이나 서비스 정보를 저장하고 있는 전자 문서로, 전자 상거래에서 가장 중요한 자료 중 하나이다. 전자 카탈로그는 지속적으로 추가, 수정 혹은 삭제되면서 최신의 상태로 유지되게 되는데, 전자 카탈로그의 양이 많아지면서 중복이 발생하고, 부적합한 분류에 할당되는 등, 품질 유지 문제가 발생한다. 검색, 중복확인, 자동분류는 카탈로그 품질 관리를 위해 중요한 기능들인데, 이 기능을 구현하기 위해서 카탈로그에서 추출된 색인어들의 통계 정보를 활용한 확률 모델들이 제시되었다. 그러나 이들은 서로 독립적으로 다루어 졌기에, 카탈로그 관리 시스템이라 는 하나의 시스템에서 구현될 수 있음에도 불구하고, 각 모델들이 공유하는 데이터와 이를 관리하기 위한 데이터 관리 기법에 관한 연구는 미흡하였다. 따라서 본 논문에서는 세 기능을 위한 확률모델을 정리하고, 이를 관계형 데이터베이스 상에서 구현하고, 통계 정보를 효율적으로 관리하는 방법을 제시한다. 특히, 실체화 뷰를 이용하여 불필요한 응용의 개발 비용과 데이터 무결성 저해요인을 제거하였다. 다량의 실제 전자 카탈로그 데이터베이스에 대한 실험을 통해 관계형 데이터 베이스를 이용한 구현이 속도와 정확성에 있어 실용성이 있음을 보였고, 응용을 통한 통계 정보갱신 방법과의 비교를 통해 실체화 뷰를 활용한 통계 정보 관리 기법의 효용성을 보였다.

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The environment dependences of quasar properties in the Sloan Digital Sky Survey

  • Song, Hyunmi;Park, Changbom
    • 천문학회보
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    • 제39권2호
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    • pp.59.2-59.2
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    • 2014
  • We study the environmental dependences of various quasar properties using the Sloan Digital Sky Survey (SDSS). For an environmental indicator, we construct the galaxy number density field from the latest data (Data Release 12) of Constant MASS (CMASS) galaxies of SDSS in the redshift range 0.46<=z<=0.59. The galaxy number density field is determined by searching the 20 nearest galaxies from each grid point. For quasars, we use the fifth edition of the SDSS Quasar Catalog made by Schneider et al. (2010) and the catalog of properties for the quasars by Shen et al. (2011). We find environmental dependences of quasar properties as a function of the galaxy number density. This will help us to understand the evolution of quasars with their environment, which will be useful to improve modeling Active Galactic Nuclei feedback in cosmological hydrodynamic simulations.

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From dark matter to baryons in a simulated universe via machine learning

  • Jo, Yongseok
    • 천문학회보
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    • 제45권1호
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    • pp.50.2-50.2
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    • 2020
  • The dark matter (DM) only simulations have been exploited to study e.g. the large scale structures and properties of a halo. In a baryon side, the high-resolution hydrodynamic simulation such as IllustrisTNG has helped extend the physics of gas along with stars and DM. However, the expansive computational cost of hydrodynamic simulations limits the size of a simulated universe whereas DM-only simulations can generate the universe of the cosmological horizon size approximately. I will introduce a pipeline to estimate baryonic properties of a galaxy inside a dark matter (DM) halo in DM-only simulations using a machine trained on high-resolution hydrodynamic simulations. An extremely randomized tree (ERT) algorithm is used together with multiple novel improvements such as a refined error function in machine training and two-stage learning. By applying our machine to the DM-only simulation of a large volume, I then validate the pipeline that rapidly generates a galaxy catalog from a DM halo catalog using the correlations the machine found in hydrodynamic simulations. I will discuss the benefits that machine-based approaches like this entail, as well as suggestions to raise the scientific potential of such approaches.

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주제목록을 위한 한국용어열색인 시스템의 기능 (Function of the Korean String Indexing System for the Subject Catalog)

  • 윤구호
    • 한국문헌정보학회지
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    • 제15권
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    • pp.225-266
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    • 1988
  • Various theories and techniques for the subject catalog have been developed since Charles Ammi Cutter first tried to formulate rules for the construction of subject headings in 1876. However, they do not seem to be appropriate to Korean language because the syntax and semantics of Korean language are different from those of English and other European languages. This study therefore attempts to develop a new Korean subject indexing system, namely Korean String Indexing System(KOSIS), in order to increase the use of subject catalogs. For this purpose, advantages and disadvantages between the classed subject catalog nd the alphabetical subject catalog, which are typical subject ca-alogs in libraries, are investigated, and most of remarkable subject indexing systems, in particular the PRECIS developed by the British National Bibliography, are reviewed and analysed. KOSIS is a string indexing based on purely the syntax and semantics of Korean language, even though considerable principles of PRECIS are applied to it. The outlines of KOSIS are as follows: 1) KOSIS is based on the fundamentals of natural language and an ingenious conjunction of human indexing skills and computer capabilities. 2) KOSIS is. 3 string indexing based on the 'principle of context-dependency.' A string of terms organized accoding to his principle shows remarkable affinity with certain patterns of words in ordinary discourse. From that point onward, natural language rather than classificatory terms become the basic model for indexing schemes. 3) KOSIS uses 24 role operators. One or more operators should be allocated to the index string, which is organized manually by the indexer's intellectual work, in order to establish the most explicit syntactic relationship of index terms. 4) Traditionally, a single -line entry format is used in which a subject heading or index entry is presented as a single sequence of words, consisting of the entry terms, plus, in some cases, an extra qualifying term or phrase. But KOSIS employs a two-line entry format which contains three basic positions for the production of index entries. The 'lead' serves as the user's access point, the 'display' contains those terms which are themselves context dependent on the lead, 'qualifier' sets the lead term into its wider context. 5) Each of the KOSIS entries is co-extensive with the initial subject statement prepared by the indexer, since it displays all the subject specificities. Compound terms are always presented in their natural language order. Inverted headings are not produced in KOSIS. Consequently, the precision ratio of information retrieval can be increased. 6) KOSIS uses 5 relational codes for the system of references among semantically related terms. Semantically related terms are handled by a different set of routines, leading to the production of 'See' and 'See also' references. 7) KOSIS was riginally developed for a classified catalog system which requires a subject index, that is an index -which 'trans-lates' subject index, that is, an index which 'translates' subjects expressed in natural language into the appropriate classification numbers. However, KOSIS can also be us d for a dictionary catalog system. Accordingly, KOSIS strings can be manipulated to produce either appropriate subject indexes for a classified catalog system, or acceptable subject headings for a dictionary catalog system. 8) KOSIS is able to maintain a constistency of index entries and cross references by means of a routine identification of the established index strings and reference system. For this purpose, an individual Subject Indicator Number and Reference Indicator Number is allocated to each new index strings and new index terms, respectively. can produce all the index entries, cross references, and authority cards by means of either manual or mechanical methods. Thus, detailed algorithms for the machine-production of various outputs are provided for the institutions which can use computer facilities.

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LARGE SDSS QUASAR GROUPS AND THEIR STATISTICAL SIGNIFICANCE

  • Park, Changbom;Song, Hyunmi;Einasto, Maret;Lietzen, Heidi;Heinamaki, Pekka
    • 천문학회지
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    • 제48권1호
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    • pp.75-82
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    • 2015
  • We use a volume-limited sample of quasars in the Sloan Digital Sky Survey (SDSS) DR7 quasar catalog to identify quasar groups and address their statistical significance. This quasar sample has a uniform selection function on the sky and nearly a maximum possible contiguous volume that can be drawn from the DR7 catalog. Quasar groups are identified by using the Friend-of-Friend algorithm with a set of fixed comoving linking lengths. We find that the richness distribution of the richest 100 quasar groups or the size distribution of the largest 100 groups are statistically equivalent with those of randomly-distributed points with the same number density and sky coverage when groups are identified with the linking length of $70h^{-1}Mpc$. It is shown that the large-scale structures like the huge Large Quasar Group (U1.27) reported by Clowes et al. (2013) can be found with high probability even if quasars have no physical clustering, and does not challenge the initially homogeneous cosmological models. Our results are statistically more reliable than those of Nadathur (2013), where the test was made only for the largest quasar group. It is shown that the linking length should be smaller than $50h^{-1}Mpc$ in order for the quasar groups identified in the DR7 catalog not to be dominated by associations of quasars grouped by chance. We present 20 richest quasar groups identified with the linking length of $70h^{-1}Mpc$ for further analyses.