Towards completing an EPIC collection of LMC supernova remnants

We propose a Fulfil Programme to observe known supernova remnants (SNRs) in theLarge Magellanic Cloud (LMC). Out of a large sample of 60, these sources are thelast having insufficient Xray observations available. By filling this gap, wewill have the largest and most complete fluxlimited set of SNRs in a galaxyobserved with a single mission/instrument. This will provide an excellentbenchmark for the comparison of SNR populations of galaxies in the Local Groupand beyond. In addition, it will reveal the physical properties of each target,such as age, abundances, and progenitor type. truncated!, Please see actual data for full text [truncated!, Please see actual data for full text]