“…As shown in the figures, it is found that the excitation spectrum monitored by 555 nm is mostly composed by the band absorption near 254 nm and two excitation peaks at 375 nm. The former can be attributed to the host absorption [10], and the later belong to the characteristic absorption of Er 3+ [11]. When the excitation spectrum monitored at 675 nm is checked, not only the strong band absorption at 254 nm can be There are some stronger emission peaks at 540, 555 and 675 nm, which are due to the Er 3+ transition of 4 H 11/2 -4 I 15/2 , 4 S 3/2 -4 I 15/2 and 4 F 9/2 -4 I 15/2 [12].…”