  At highest energy edges Ultra High Energy Cosmic Ray, (UHECR) and PeVs
neutrino (UHE neutrino), should soon offer new exciting astronomy. The fast and
somehow contradictory growth of hundred of antagonist models shows the
explosive vitality of those new astronomy frontiers. No conclusive
understanding on the UHECR and UHE neutrino source are at hand. The earliest
expectation of GRBs (as a one shoot Fireball model) as the main (UHE neutrino)
sources has been rejected. The source of UHECR as the expected GZK ones within
our Super-Galactic Plane (within few tens Mpc) it has been quite disproved.
However alternative models on GRB (as the long life precessing Jets) and the
new updated records by AUGER, TA, ICECUBE are offering nevertheless partial
understanding and early hint for point source correlations along our galaxy and
toward Cen A, the nearest extragalactic AGN.
