\begin{document}$ V(\phi) $\end{document} in the quintessence field is a double exponential function, whereas \begin{document}$ V(\phi) $\end{document} in the phantom field is a double Gaussian function. This reconstruction can provide an important reference for the scalar field study. The two types of data employed reveal that the tachyon field is disadvantageous for describing the cosmic acceleration."> Observational constraint on the dark energy scalar field -
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