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The Molonglo Telescope is an EW synthesis array which can image about 5 square degrees in 12 hours, with an average sensitivity of 1.5 mJy/beam and sub arcmin angular resolution. The SKA Molonglo Prototype (SKAMP) project will provide a redevelopment of this telescope to produce a new low frequency spectral line capability, initially with a bandwidth of ∼30 MHz centred on 843 MHz. We will measure the neutral gas in galaxies at a time when the Universe was half its present age using HI absorption measurements against distant radio sources. The results will allow direct tests of theories of galaxy formation at a poorly understood epoch, when most of the stars were being formed. A status report on progress and prospects is presented.

HI absorption studies of galaxies and the SKA Molonglo Prototype (SKAMP) Project