The Galactic halo is supposed to form from merging with nearby dwarf galaxies. In order probe different components of the halo, we have applied Gaussian Mixture Models method a selected sample metal poor stars [Fe/H] $< -0.7$ dex in APOGEE DR16 catalogue based on four-parameters, metallicity, [Mg/Fe] ratio and spatial velocity (\textit{$V_R$, $V_\phi$}). Nine groups are identified four (group 1...