Data from: Microsatellite analysis of genetic diversity and population structure of Arabian horse populations

Khanshour et al_SupMat_Figure S1Comparisons among 15 microsatellite markers and the number of populations out of 14 for which any pair of markers shows significant LD at p<0.05Khanshour et al_SupMat_Figure S2Hardy-Weinberg equilibrium status in 14 populations and 15 loci. For the total markers together in each population, the Fisher’s method was used after Bonferroni correction to determine the significant deviation of a population from H-W equation. Population abbreviations could be seen in Table 1Khanshour et al_SupMat_Figure S3The FCA among all populations except the PZ (as generated by GENETIX). Each population was represented by its center of gravity point into 3D plot. Axis 1 accounts for 24.20% of the variation. Population abbreviations are found Table 1. The percentage of variance explained by each axis is found in the axes labels.Khanshour et al_SupMat_Figure S4ΔK distribution along of different values of clusters (K) for 11 populations depending on Evanno’s method (Evanno 2005) using Structure Harvester application.Khanshour et al_SupMat_Figure S5ΔK distribution along of different values of clusters (K) for ten populations depending on Evanno’s method (Evanno 2005) using Structure Harvester application.