\begin{document}$z_c$\end{document}. It is shown that the dipole appears at the \begin{document}$2\sigma$\end{document} confidence level only if \begin{document}$z_c\leq 0.1$\end{document}, and in this redshift region, the dipole is very stable, almost independent of the specific value of \begin{document}$z_c$\end{document}. For \begin{document}$z_c=0.1$\end{document}, the dipole amplitude is \begin{document}$D=1.0_{-0.4}^{+0.4}\times 10^{-3}$\end{document}, pointing toward \begin{document}$(l,b)=(334.5_{\ -21.6^{\circ}}^{\circ +25.7^{\circ}},16.0_{\ -16.8^{\circ}}^{\circ +27.1^{\circ}})$\end{document}, which is approximately \begin{document}$65^{\circ}$\end{document} away from the CMB dipole. This implies that the full Pantheon+ sample is consistent with a large-scale isotropic universe, but the low-redshift anisotropy could not be purely explained by the peculiar motion of the local universe."> Consistency of Pantheon+ supernovae with a large-scale isotropic universe -
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