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The major (2x) and minor (2y) orthogonal axes of each cluster were measured, and the cluster diameter, D calculated from D = 2√ xy).
The expression levels of genes from each cluster were measured by RT-qPCR in the indicated KDs and expressed as Log2 (fold change) values relative to control (GFP ) KD ESCs after normalization.
The proximities of any two residues in each cluster were measured by their relative 'contact frequency', which is defined by how often the two residues contact each other in the cluster; a pair of residues are in contact when the distance between the surface of the fine resolution beads is less than 10 Å.
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At runtime, the workload for cluster is measured and based on this measurement, future workload is predicted.
The total luminosity of the Coma cluster is measured to be about 3 × 1013 solar luminosities; therefore, the mass-to-light ratio in solar units required to explain Coma as a bound system exceeds by an order of magnitude what can be reasonably ascribed to the known stellar populations.
To evaluate the hierarchical structure, the in-degree inequality of each cluster is measured with the Gini coefficient.
The temperature-dependent CL spectra of the GaN nanorod cluster are measured at temperature T = 20 K to 300 K as shown in Figure 2a.
The length of the cluster is measured as the number of genes in this cluster.
Experimentally, this corresponds to a positive, negative, or no change, respectively, in mRNA levels for each gene (or gene cluster) being measured.
To identify significant and highly present GO categories, the most prevalent GO within each cluster was measured for overrepresentation by a standard hypergeometric test.
Further, the transcription of several representative genes of the maltose-maltodextrin utilization cluster was measured in an InshprK/P-mutant of L. monocytogenes [45].
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