086495

We propose a Fulfil Programme to observe six known supernova remnants openParSNRsclosePar in the Large Magellanic Cloud openParLMCclosePar. Out of a large sample of 60 comma these sources are the last having insufficient X-ray observations available. By filling this gap comma we will have the largest and most complete flux-limited set of SNRs in a galaxy observed with a single mission-instrument. This will provide an excellent benchmark for the comparison of SNR populations of galaxies in the Local Group and beyond. In addition comma it will reveal the physical properties of each target comma such as age comma abundances comma and progenitor type.