“…5 that both the emission intensity of 1.46 m and 1.53 m depend on the temperature, nevertheless, in lower temperature below 100 K, it is almost no change for the emission intensities for both the 3 H 4 → 3 F 4 (1.46 m) and 4 I 13/2 → 4 I 15/2 (1.53 m) transitions. In higher temperature above 100 K, the emission intensities decrease with the increasing of temperature, and it can be noted that the emission intensity of 1.53 m deceases much drastical than that of 1.46 m, and the two intensities become nearly equal to unity at 300 K. The temperature dependence of the emission spectra can be understood by considering the phonon assistant energy transfer (ET) rate, which is given by Miyakawa-Dexter theory [28,29],…”