----- Submission 1 (Tue Apr 05 12:58:39 GMT 2005) ----- Phase II Proposal 10467 (sgr1806_2) successfully submitted. ----- Submission 2 (Wed Apr 06 15:40:16 GMT 2005) ----- Phase II Proposal 10467 (sgr1806_2b) successfully submitted. ----- Submission 3 (Fri Apr 08 08:48:31 GMT 2005) ----- Assigned ID: 733 ----- Submission 1 (Thu Feb 10 18:42:00 GMT 2005) ----- Phase I Proposal 733 (sgr1806) successfully submitted. ----- Submission 3 (Thu Feb 10 18:59:23 GMT 2005) ----- Phase I Proposal 733 (sgr1806) successfully submitted. ----- Submission 4 (Thu Feb 10 18:59:49 GMT 2005) ----- Phase I Proposal 733 (sgr1806) successfully submitted. On 2004 December 27, the ``magnetar'' candidate SGR1806-20 experienced a giant flare, the third detected from Soft Gamma-ray Repeaters since 1979 (GCN Circulars #2920, #2922). This was by far the most luminous flare ever observed from a Galactic high energy source (more than 10^46 erg/s). Following this event, SGR1806-20 was observed and detected in the radio band (GCN # 2928, #2930) and resolved into two parts: a point-like and a diffuse component. Our team, based on the radio position, detected the probable IR counterpart , the first IR counterpart ever for a SGR, by using the VLT NACO observations carried out in 2004 (ATel #278). This DDT proposal is aimed at (a) studying, in the IR band, the afterglow diffuse component (linked to the giant flare event), its shape and expansion rate as a function of time, (b) tracing back the flux at the onset of the flare through the detection and study of its scattered-light echoes, (c) searching for jet--like structures.

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