A practical strategy is presented and successfully implemented to determine
form factors in the time-like but unphysical (below threshold) region usin
g dispersion relations, in a model independent way without any bias towards
expected resonances. Space and timelike data have been employed along with
a regularization scheme to unfold and solve the integral equations. Remark
ably, resonance structures with peaks for the rho(770), rho'(1600) and a st
ructure near the N (N) over bar threshold are automatically generated. The
Phi peak is invisible thus refuting suggestions about any sizeable s (s) ov
er bar content; in the nucleon.