\begin{document}$\gamma$\end{document}-ray spectra of PG 1553+113 and PKS 2155−304 measured by Fermi-LAT and H.E.S.S. The choice of extragalactic background light (EBL) model, which induces the attenuation effect in observed \begin{document}$\gamma$\end{document}-ray spectra, affects the ALP implications. For the ordinary EBL model that prefers a null hypothesis, we set constraints on the ALP-photon coupling constant at 95% C.L. as \begin{document}$g_{a\gamma}\lesssim 5\times 10^{-11} ~{\rm{GeV}}^{-1}$\end{document} for the ALP mass \begin{document}$\sim 10$\end{document} neV. We also consider the CIBER observation of the cosmic infrared radiation, which shows an excess at wavelengths of \begin{document}$\sim 1~\mu$\end{document}m after the substraction of foregrounds. High-energy gamma-rays from extragalactic sources at high redshifts would suffer from a more significant attenuation effect caused by this excess. In this case, we find that the ALP-photon oscillation would improve the fit to the observed spectra of PKS 2155−304 and PG 1553+113 and find a favored parameter region at 95% C.L.."> Implications of axion-like particles from the Fermi-LAT and H.E.S.S. observations of PG 1553+113 and PKS 2155−304 -
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