TITLE: GCN GRB OBSERVATION REPORT NUMBER: 4819 SUBJECT: GRB 060218: rebrightening DATE: 06/02/23 17:24:47 GMT FROM: Daniele Fargion at Phys.Dept, Rome Univ1,It The very recent GRB 060218 long burst, brightening, decline and rebrightening are puzzling, but consistent with a model for GRB (and later on for SGR), made by precessing spinning and blazing gamma collimated Jets (solid angle about 10^-8 sr). See ref. below. The GRB is associated to a blazing Jet whose peak power is like a Supernova one (but apparent as GRB power). In a very small near-by cosmic volumes as GRB 060218 at z=0.0331 or GRB980425 at z=0.008, it is quite off-axis (a few degree). The off-axis geometry increase the probability to be found and reduce its apparent luminosity (underluminous GRB). The spinning-precessing jet lead to inner fast variability, rebrightenings and while shining away, the smooth GRB decay. In analogy, but at much lower power and therefore at nearer distances later on, comparable and longeve X-Jet-pulsars are blazing as SGR. The persistent precessing jet offer multi optical rebrightening and-or permits un-correlation with earlier SN. Hadron material around the SN make the GRB event a possible TeV source observable by Milagro or ARGO,Hess and MAGIC, an UHECR source in Auger and Hires,a UHE neutrino source for AMANDA and Baikal (see DF and M.G. Nuovo Cim. 28 C.N 4-5.p.813-816. astro-ph/0505150). The GRB maybe obsevable by its PeVs Glashow neutrino while inducing air-showers at horizons or EeV Tau air-showers below the MAGIC horizons (see astro-ph/0511597). In conclusion: The presence (but even the already absence) in near days of a complete SN rise combined with multi-bumps (optical and-or radio rebrightening) will stand for a definitive long live (but decaying) precessing Jet, blazing within an earlier SN shell. Its possible late Jet blaze has been and it maybe observed in future X flare again (if shining online to us). On the contrary the rise of an unique dramatic SN bump a few days later the observed brightening and rebrightening of the GRB, will be the clear hint that GRB-SN explosion maybe preceeded by a persistent SGR Jet activity whose culmination ends into a the catastrophic SN-GRB most powerfull beamed event. This scenario may be still marginally coexisting with previous one , if a Jet activity may trigger the star collapse and survive the SN explosion. see D.F. ATEL # 31; by DF, 15 Jul 1998; "On the nature of GRB-SGRs blazing jets" in Astron. Astrophys. Suppl. Ser. 138, 507-508; and or more recent astro-ph/0501403 in D.F. Chin.J.Astron.Astrophys.3,3 (2003) 472-482. This message may be cited Daniele Fargion E_mail: daniele.fargion@roma1.infn.it Phone: +390649914287 Fax: +39064957697 ----------------------------------------------