\begin{document}$ \chi^2 $\end{document} function of the distance modulus of data samples, we obtain the constrained values of cosmographic parameters in the parameterization of the dark energy scenario. One condition of the phantom barrier crossing is acquired. Several physical properties of the universe are discussed by considering the anisotropy effect and different observational data points. One should note that the deductions of the cosmological parameter verify recent observational data."> Phantom cosmologies from the simplest parameterization of the DE model using observational data in a BI type universe -
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