\begin{document}$ |\Delta z|<0.005$\end{document}, and most of the available data from the GW measurements is employed to detect cosmic opacity due to improvements in the distribution of the future SNe Ia observations. Results show that the uncertainties of the constraints on cosmic opacity can be reduced to \begin{document}$ \sigma_{\epsilon}\sim 0.0041$\end{document} and 0.0014 at the \begin{document}$ 1\sigma$\end{document} confidence level (CL) for 1000 data points from the ET and DECIGO measurements, respectively. Compared with the allowable limits of intergalactic opacity obtained from quasar continuum observations, these future astronomical observations can be used to verify the cosmic opacity. In this way, GW and SNe Ia measurements can be used as important and effective tools to detect cosmic opacity in the future."> Exploring the potentiality of future standard candles and standard sirens to detect cosmic opacity -
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