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Old and recent puzzles of GRBs and SGRs find a solution with a model based onthe fast blazing of very collimated thin gamma Jets. Damped oscillatingafterglows in GRB030329 find a natural explanation assuming a very thin Jetwhose persistent activity and different angle of view maybe combined at oncewith the Supernovae power and the apparent huge GRBs output. The same thinbeaming offer an understanding of the apparent SGR-Pulsar power connection. Athin collimated precessing Gamma Jet model for both GRBs and SGRs, at theirdifferent scaled luminosity (10^{44} - 10^{38}erg s^-1), explains the existenceof few identical energy spectra and time evolution of these sources leading toa unified model. Their similarity with the huge precessing Jets in AGN, QSRsand Radio-Galaxies inspires this smaller scale SGR-GRB model. Thespinning-precessing Jet explains the rare mysterious X-Ray precursors in GRBsand SGRs events. Any large Gamma Jet off-axis beaming to the observer mightlead to the X-Flash events without any GRB signals, as the most recentXRF030723. Its possible re-brightening would confirm the evidence of thevariable pointing of the jet in or off line towards the observer.  Indeed a multi-precessing Jet at peak activity in all bands may explain thepuzzling X or optical re-brightening bumps found in the GRB 021004, GRB030329and the SGR 1900+ 14 on 27 August 1998 and once again on the 18 April 2001.Rarest micro-quasars neutron star in our galaxy as SS433, and Herbig Haroobjects and Cir-X-1 describe these thin precessing Jet imprints in thespectacular shapes of their relic nebulae.Comment: 10 pages, 10 figures, Vulcano Conference May 200

GRBs-SN and SGR-X-Pulsar as Blazing Jets