• Title/Summary/Keyword: Spec-catalog

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Development of a System that Translates Spec-catalog Data for Plant Equipment Considering Holes and Nozzles (홀과 노즐을 고려한 플랜트 기기 스펙-카탈로그 데이터 번역 시스템 개발)

  • Lee, Hyunoh;Kwon, Hyeokjun;Lee, Gwang;Mun, Duhwan
    • Journal of the Korean Society of Manufacturing Process Engineers
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    • v.19 no.9
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    • pp.59-70
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    • 2020
  • Three-dimensional (3D) design data is used for various purposes throughout the life cycle of a plant construction project. Plant 3D CAD systems support 3D modeling based on specs-catalogs, which contain data that are used for different purposes such as design, procurement, production, and handover. Therefore, it is important to share the spec-catalog data in the 3D design model with other application systems. Sharing this data thus requires a system that extracts spec-catalog data from plant 3D CAD systems and converts them into neutral model data. In this paper, we analyze equipment spec-catalog data of plant 3D CAD systems and, based on these analyses, define the data structure for neutral spec-catalog data. We subsequently propose a procedure that translates native spec-catalog data to neutral model data and develop a prototype system that performs this operation. The proposed method is then experimentally validated for the test spec-catalog data.

SEARCHING FOR ULIRGS BY USING AKARI AND WISE

  • Koyama, Shuhei;Matsuhara, Hideo
    • Publications of The Korean Astronomical Society
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    • v.32 no.1
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    • pp.309-311
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    • 2017
  • Properties of ULIRGs (Ultra Luminous InfraRed Galaxies) are important to understand the cosmic star formation history. To investigate their properties up to z=0.3, we search for ULIRGs identified by using the AKARI/FIS Bright Source Catalogue and the WISE All-Sky catalog. By matching the AKARI $90{\mu}m$ catalogue with the WISE catalog, we selected 3,452 galaxies. Additionally, combined with the SDSS DR10 spectroscopic data, we selected 952 galaxies with spec-z. We then computed total infrared luminosities using SED fitting technique, and identified 31 ULIRGs, 561 LIRGs and 344 IRGs. For these galaxies, we found an indication that ULIRGs selected by AKARI change the SED shape with redshift (z = 0.1 - 0.3).