New Candidates for Supernova Remnantsin the Large Magellanic Cloud

We propose observations of new candidates for Xray supernova remnants(SNRs) in the Large Magellanic Cloud (LMC). Building on a successful campaign to observe candidates with ROSAT detections, we now propose observations of the lowest Xray surface brightness SNR candidates whichwere found in multiwavenlength observations and confirmed in the newest eROSITAdata. Owing to the high sensitivity ofXMMNewton we will be able to confirm SNRsat the faintest end of the Xray luminosity function(XLF) and study their plasmaproperties and age, aswell as the ambient interstellar medium. truncated!, Please see actual data for full text [truncated!, Please see actual data for full text]