This is true even if observed clusters are complete in themselves rather than being the observed part of larger complete clusters: here methods may describe imaginary complete clusters rather than the observed clusters.
Two types of frequently observed clusters of α variants are found to share either a common <1 1 1>β axis or a common {1 1 0}β plane.
In the Antennae galaxy, for example, the Hubble Space Telescope has observed clusters of clusters, regions in the galaxy that span hundreds of parsecs, where many of the clusters will eventually collide and merge.
Similarly, we observed clusters of bands at ∼10 nt intervals.
Occasionally, we also observed clusters of cells, predominantly clustered through their uropod regions, to be enriched in flotillin staining (unpublished observations), probably due to the flotillin interaction with PSGL-1 [44].
So far we have assumed observed clusters are generated from complete clusters by excluding missing members, but ICS can also arise where observed clusters are complete in themselves.
For a single binary X, they compared the log odds ratios in complete and observed clusters.
Second, we also observed clusters of plaques within the population of new plaques.
By mapping these genes back to the human genome, they observed clusters of adipose tissue specific genes.
We observed clusters of subthreshold-positive activation at z = 2.0 for vigilance scores (Fig 5) in the mPFC and ACC.
However, we also observed clusters mapping outside the typical promoter region 2 kb upstream and 200 bp downstream from TSSs.
