0870004

This observation targets SN2011fe which occurred on 23 August 2011 in the nearby galaxy M101 at 6.4 Mpc distance aiming at high energy emission from 56Co decay gamma-ray lines and its associated Compton-scattered continuum. The prospected emission maximum from the 56Co lines should be ~early November. These ToO observations target the rise of such emission towards this maximum which is expected to show characteristic differences for different progenitor and explosion models. Observations are in standard dither mode for broader usage of these public data andcomplement another proprietary ToO on SN2011fe as was proposed for AO-8 and is scheduled in the first weeks after explosion and at expected gamma-ray maximum. [truncated! Please see actual data for full text]