By Aitken R.J.

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**Extra resources for A Statistical Study of the Visual Double Stars in the Northern Sky (1915)(en)(5s)**

**Sample text**

16. Final IBIS paradigm 24 J. MacGregor Smith and the IBIS which must integrate them and the models necessary to resolve the issues (see Fig. 16). The IBIS is necessary to frame ∆1 and to interrelate the different issues and problems spawned by ∆2 . A systems model Σ is necessary for ∆3 , ∆4 . Generating ideas and evaluating as captured by ∆5 and ∆6 must rely on effective algorithmic tools but these must be tempered with a cognizance of the multiple objectives and criteria involved so that effective tradeoffs can be made.

LLB versus CV for systems (17) with Tdown = 100 Fig. 6. Sensitivity of LLB to the nature of up- and downtime distributions for systems (17) Lean buffering in serial production lines with non-exponential machines 43 Function 1 (CV ) is illustrated in Figure 6. As one can see, in most cases it takes values within 10%. Thus, it is possible to conclude that for all practical purposes kE depends on the coefﬁcients of variation of up- and downtime, rather than on actual distribution of these random variables.

Thus, it is possible to conclude that for all practical purposes kE depends on the coefﬁcients of variation of up- and downtime, rather than on actual distribution of these random variables. 2 System {[D(p, P ), D(r, R)]1 , . . , [D(p, P ), D(r, R)]10 } Figures 7 and 8 present the simulation results for lines (18), while Figure 9 characterizes the sensitivity of kE to up- and downtime distributions. This sensitivity is calculated according to (19) with the only difference that the max is taken over A, B ∈ {(18)}.