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Additionally, the major advantage of the multi-layer clustering algorithm is that no explicit definition of the distance measure among instances (patients) is necessary and that no explicit definition of the number or size of the resulting clusters is expected from the user [12].
Thus, a maximal number of clusters is expected at an intermediate threshold λ t h r m a x.
12. Similarly the number of clusters is expected to decrease and remain throughout the entire simulation less than 5 with probability greater than 0.75.
Through a comparative analysis of closely related species [ 35] and functional experiments, an estimate for the evolutionary forces that shape the pS/pT clusters is expected.
The position of these clusters is expected to vary with the number of non-segregating subgenomes that are targeted in addition to the segregating subgenome.
Note that the relatively low number of statistically significantly SPR-enriched clusters is expected due to incompleteness of SPR (KPR) data set.
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Some clusters are expected to show a gradual transition from solidlike to liquidlike, appearing slushy in the temperature range between their solidlike and liquidlike zones.
Other clusters are expected to show, as seen in computer simulations, distinct solidlike and liquidlike forms that qualitatively resemble bulk solids and liquids in virtually every aspect, even though they may exhibit quantitative differences from the bulk.
These different densities impact negatively the CGP protocol since clusters are expected to be equally balanced throughout the simulation, however the CGP will still present a good performance.
The infrared spectra, Raman spectra, and PES of Ag n V (n = 1 12) clusters are expected to identify the ground states in times to come.
Rogier Windhorst, an astronomer from Arizona State University, called the result "very exciting stuff", principally because such clusters are expected to be incredibly rare in the earliest days of the Universe.
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