“…It is well known that the presence of H 2 O in the lanthanide first coordination sphere contributes to nonradiative deexcitation of luminescence and, as a consequence, reduces the quantum yield of the lanthanide luminescence. In order to determine if polynuclear complexes are formed in considerable amount, the Stern-Volmer K SV quenching constants, which are defined by Equations (8) and (9): (8) (9) were determined. K SV Φ and K SV τ are the Stern-Volmer quenching constants that were determined from the luminescence intensity (I) or the luminescence lifetime (τ), and I Tb , I Tb,Eu , I Eu , τ Tb , τ Tb,Eu , τ Tb are the appropriate luminescence quantities in the presence or absence of the quencher (Eu 3+ ).…”