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The number of independent components (ICs) (chemical constituents) in each peak cluster was estimated using morphological score method.
While the black hole discovered in 2011 in the galaxy NGC 4889 in the Coma Cluster was estimated to have an upper limit of 21 billion solar masses, its range of possible masses was large: between 3 billion and 21 billion suns.
The location of each AE cluster was estimated accordingly.
In the subsubtype A3 analysis, the tMRCA of the Guinea-Bissau cluster was estimated to 1979 (95% HPD 1960 1988).
The significance P of an original cluster was estimated according to the proportion of the randomization null distribution exceeding the observed maximum/minimum t-sum test-statistics.
The physical length of a marker cluster was estimated by summation of the lengths of the scaffolds or scaffold regions with markers on it that mapped in the marker cluster (see also Table S7 and Table S12).
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For the stable configurations, the frequency of oscillation of cluster is estimated O(10−3) of the frequency of operation.
The sensor nodes do not have an attached GPS device but their positions within a cluster are estimated based on internode distances.
The combined mass of the cluster is estimated to be (0.15 1.5) × 1015 solar masses.
The total mass contained in the cluster is estimated to be about 800 solar masses.
The cluster is estimated to dissipate in another 250 million years.
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