• Title/Summary/Keyword: W.I

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FIMS Observation of Cygnus Loop

  • Seon Kwang-Il;Lee D.-H.;Park J.-H.;Kim I.-J.;Shinn J.-H.;Ryu K.-S.;Jin H.;Yuk I.-S.;Han W.;Nam U.-W.;Min K.-W;Edelstein J.;Korpela E.
    • The Bulletin of The Korean Astronomical Society
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    • v.29 no.2
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    • pp.38.1-38.1
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    • 2004
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Search for star clusters in M33

  • Park W. -K.;Lee M. G.;Kim S. C.;Park H. S.;Park J. -H.;Lee S. -G.;Oh S. J.;Lee Y. -W.;Sohn Y. -J.;Rey S. -C.;Yuk I. -S;Kim H. -I.;Han W.
    • The Bulletin of The Korean Astronomical Society
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    • v.28 no.2
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    • pp.89-89
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    • 2003
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On the Flatness of Semi-Cubically Hyponormal Weighted Shifts

  • Li, Chunji;Ahn, Ji-Hye
    • Kyungpook Mathematical Journal
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    • v.48 no.4
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    • pp.721-727
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    • 2008
  • Let $W_{\alpha}$ be a weighted shift with positive weight sequence ${\alpha}=\{\alpha_i\}_{i=0}^{\infty}$. The semi-cubical hyponormality of $W_{\alpha}$ is introduced and some flatness properties of $W_{\alpha}$ are discussed in this note. In particular, it is proved that if ${\alpha}_n={\alpha}_{n+1}$ for some $n{\geq}1$, ${{\alpha}_{n+k}}={\alpha}_n$ for all $k{\geq}1$.

FIMS Observations of Hot Interstellar Medium

  • Seon Kwang-Il;Kim I. J.;Park J. H.;Shinn J. H.;Lee D. H.;Ryu K. S.;Han W.;Min K. W.;Jin H.;Yuk I. S.;Nam U. W.;Edelstein J.;Nishikida K.
    • Bulletin of the Korean Space Science Society
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    • 2004.10b
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    • pp.49-49
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    • 2004
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The Properties of M33 Star Cluster System

  • Park W -K.;Lee M.S.;Park H.S.;Kim S. C.;Park J. -H.;Lee S. -G.;Oh S.J;Lee Y.-W.;Sohn Y. -J.;Rey S. -C.;Yuk I. -S.;Kim H. -I.;Han W
    • The Bulletin of The Korean Astronomical Society
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    • v.30 no.1
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    • pp.38.2-38.2
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    • 2005
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A Study on Determining of Job Sequence by Work Sampling(I) (W.S법에 의한 JOB SEQUENCE의 결정(I))

  • 강성수;노인규
    • Journal of Korean Society of Industrial and Systems Engineering
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    • v.11 no.18
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    • pp.59-69
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    • 1988
  • This study represents the method of application of W.S(Work Sampling) to determine job sequence. The result shows job sequence which has the came performance measure of optimal job sequence is selected by average number of 199 sampling. In the case, the optimal job sequence is not selected within the sampling number of 921 which satisfy the reliability of 99.5% and precision of 99%, the deviation is very little which 0.73%. This improves the possibility of application of W.S method to select optimal job sequence is very high.

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Observation Planning Software for FIMS

  • Park, J.H.;K.I. Seon;I.S. Yuk;U.W. Nam;W. Han;K.S. Ryu;K.W. Min;J. Seon;J. Edelstein
    • Bulletin of the Korean Space Science Society
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    • 2000.04a
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    • pp.49-49
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    • 2000
  • No Abstract, See Full Text

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