Recent investigations into Titan's orbital migration have produced divergent findings for Saturn's tidal dissipation, as characterized by its quality factor (Q). Lainey et al. (2020) presented evidence for a low Q value consistent with resonance locking, based on separate analyses of radio science and astrometric data. However, a subsequent study integrating data from multiple missions derived a substantially higher Q, in direct conflict with the radio science results of Lainey et al. (2020). To address this discrepancy, our study re-evaluates Titan's migration by combining Cassini radio science data, reduced to normal points, with more than a century of astrometric observations. This combined dataset was processed within a unified dynamical framework using the NOE software. Our joint analysis confirms the rapid migration rate and low Q reported by Lainey et al. (2020), thereby supporting the hypothesis of non-classical dissipation mechanisms.