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About 25% of the optical extragalactic sky is obscured by the dust and starsof our Milky Way. Dynamically important structures might still lie hidden inthis zone. Various approaches are presently being employed to uncover thegalaxy distribution in this Zone of Avoidance (ZOA). Results as well as thedifferent limitations and selection effects from these multi-wavelengthsexplorations are being discussed. Galaxies within the innermost part of theMilky Way - typically at a foreground obscuration in the blue of A_B > 5mag and|b| < 5 deg - remain particularly difficult to uncover except for HI-surveys:the Galaxy is fully transparent at the 21cm line and HI-rich galaxies are easyto trace. We will report here on the first results from the systematic blindHI-search (v < 12700 km/s) in the southern Zone of Avoidance which is currentlybeing conducted with the Parkes Multibeam (MB) Receiver.

Galaxies Behind the Deepest Extinction Layer of the Southern Milky Way