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With a fantastic sensitivity improving significantly over the advanced GWdetectors, Einstein Telescope (ET) will be able to observe hundreds of thousandinspiralling double compact objects per year. By virtue of gravitationallensing effect, intrinsically unobservable faint sources can be observed by ETdue to the magnification by intervening galaxies. We explore the possibility ofobserving such faint sources amplified by strong gravitational lensing.Following our previous work, we use the merger rates of DCO (NS-NS,BH-NS,BH-BHsystems) as calculated by Dominik et al.(2013). It turns out that tens tohundreds of such (lensed) extra events will be registered by ET. This willstrongly broaden the ET's distance reach for signals from such coalescences tothe redshift range z=2 - 8. However, with respect to the full inspiral eventcatalog this magnification bias is at the level of 0.001 and should not affectmuch cosmological inferences.

Strongly lensed gravitational waves from intrinsically faint double compact binaries - prediction for the Einstein Telescope