  A clear gamma polarization in the gamma signals from GRB021206 probes the
presence of a very thin collimated jet (opening angle Delta\theta < 0.6^o,
(Delta\Omega)\Omega< 2.5 10^-5) in Gamma Ray Burst, GRBs. The last and well
proved GRB030329/SN2003dh time and space coincidence confirms definitively the
earliest GRB980425/SN1998bw connection among GRB and Supernova. The apparent
extreme GRBs luminosity is just the extreme beamed blazing gamma Jet observed
in axis during a Supernova birth. The late relic GRBs sources may be found in
compact SNRs core, as NS or BH jets; at much later epoch, their lower power
gamma jets may be within detectability only from nearby galactic distances, as
Soft Gamma Repeaters (SGRs) or anomalous X-ray Pulsars, AXPs. This common Jet
nature explain some connection between GRBs and SGRs spectra. The geometrical
multi-precessing beaming and their reappearance to the observer may explain the
puzzling presence of X-Ray precursors in GRBs as well as in SGRs. A mysterious
re-brightening afterglows observed in early and late GRB 030329 optical
transient, like in the 27 August 1998 and 18 April 2001 SGR 1900+14 events,
might be understood as the damped oscillatory imprint left by such a
multi-precessing gamma-X-Optical and Radio Jet.
