“…The Ln 3+ environment is similar to that of the unsubstituted M 2+ ions, except that the Ln 3+ ions collapse slightly toward the vacancy, lowering the site symmetry to C 3 v . The Ln 3+ ions investigated optically in one or more of the CsMX 3 hosts include singly doped Pr 3+ , − Nd 3+ , − Tb 3+ , , Ho 3+ , , Eu 3+ , , Er 3+ , − Tm 3+ , and Ce 3+ 26 systems, and codoped Tm 3+ −Pr 3+ , Tm 3+ −Ho 3+ , Yb 3+ −Er 3+ , Gd 3+ −Er 3+ 30 and Ce 3+ −Tm 3+ 31 systems. By far, the majority of these spectroscopic investigations of lanthanide pairs in these hosts have centered on upconversion processes, especially in Er 3+ :CsCdBr 3 , wherein pair luminescence can be obtained at wavelengths shorter than the excitation wavelength(s).…”