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We propose EPIC observations to obtain a complete view of the Magellanic bridgestellar population in X-rays for the first time. These comprise of LMXBssupersoft sources and other possible serendipitous objects. The targets are acarefully chosen high-purity sample associated with the MCB obtained bycorrelating the deepest eROSITA data with multi-wavelength information to removeforeground and background contaminants. Our systematic survey of selected MCBregions will create a unique data set to understand the tidal interactionsbetween the Large Magellanic Cloud and the Small Magellanic Cloud and trace thehistory of the Local Galaxy group. [truncated! Please see actual data for full text]