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Based on data on elastic $\rho^0$ photoproduction from the H1, Omega and ZEUScollaborations, a fit has been performed to extract the value $\alpha_P (t)$ ofthe pomeron trajectory at fixed values of t from the W dependence of thedifferential $\gamma p$ cross section $d \sigma_{\gamma p} (W) / d t$. The dataused in the fit cover the range of $8.3 \le W \le 94 GeV$ in $\gamma p$centre-of-mass energy and $0.01 \le |t| \le 0.95 GeV^2$ in momentum transfer.  A linear fit to the resulting values of $\alpha_P (t)$ yields $\alpha_{P,0}=1.0871 \pm 0.0026 (stat.) \pm 0.0030 (syst.)$ for the intercept and $\alpha'_P= 0.126 \pm 0.013 (stat.) \pm 0.012 (syst.) GeV^{-2}$ for the slope of thepomeron trajectory. The data are also compatible with the Donnachie-Landshofftrajectory $\alpha_P (t) = 1.0808 + 0.25 GeV^{-2}\cdot t$ at low values $|t|\lesssim 0.3 GeV^2$ and with a constant value of $\alpha_P (t)$ at largervalues of $|t|$.

Extraction of the Pomeron Trajectory from a Global Fit to Exclusive $\rho^0$ Meson Photoproduction Data