South Africa is shortlisted to host the Square Kilometre Array (SKA), the most powerful radio telescope ever. South Africa is building an SKA technology pathfinder telescope, the Karoo Array Telescope (known as MeerKAT).

MeerKAT specifications and science

Request for proposals
An open invitation to the astronomical community to propose key project science with the South African Square Kilometre Array Precursor - MeerKAT. Closing date: 15 March 2010

MeerKAT specifications

MeerKAT will provide an array in the southern hemisphere that complements the eVLA from L-band to X-band. The array will be optimized for deep and high fidelity imaging of extended low-brightness emissions, the detection of nano-jansky radio sources, the measurement of polarization, and the monitoring of radio transient sources. The MeerKAT reference design is an array of 80 12-metre dishes fitted with wideband single-pixel cryogenic receivers.View MeerKAT specifications

MeerKAT science

MeerKAT will be the most sensitive centimetre- wavelength radio telescope in the southern hemisphere, and will make significant contributions to both galactic and extragalactic astronomical research. MeerKAT will explore phenomena such as cosmic magnetism, the evolution of individual galaxies and clusters of galaxies, the influence of dark matter on galaxies and clusters, and the nature of transient radio sources.

The scientific programme will be a mixture of blind and directed surveys conducted by large project teams, and smaller experiments designed by individual principal investigators or small teams.

These teams and principal investigators will be international in their composition, and will include participants from Africa. The scientific productivity of MeerKAT will be enhanced by combining its results with those obtained by instruments operating at other wavelengths, for instance infrared and X-ray satellite data.

The longer baselines of the MeerKAT will allow it to make full use of its superior sensitivity, providing detailed images of objects discovered by other instruments at different wavelengths, or indeed of objects discovered by the MeerKAT itself. The longer baselines will also allow accurate astrometry of objects discovered by the MeerKAT, which will aid the cross-identification of these objects in surveys at other wavelengths, for instance surveys conducted by infrared and X-ray satellites.