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MeerKAT science and specifications
Find out more about the technical specifications for the MeerKAT array, antennae and receivers.

MeerKAT factsheet
Download the latest MeerKAT factsheet.

MeerKAT photographs
Download a selection of MeerKAT visuals and photographs.


The South African MeerKAT radio telescope, currently being built some 90 km outside the small Northern Cape town of Carnarvon, is a precursor to the Square Kilometre Array (SKA) telescope and will be integrated into the mid-frequency component of SKA Phase 1. The SKA Project is an international enterprise to build the largest and most sensitive radio telescope in the world, and will be located in Africa and Australia.

Who is manufacturing the MeerKAT antennas

Stratosat Datacom (Pty) Ltd, the primary industry partner on the manufacturing of the MeerKAT antennas, leads a technology consortium including international partners General Dynamics Satcom (GDSatcom, USA) and Vertex Antennentechnik (Germany). At least 75% of the components making up the MeerKAT dish will be manufactured in South Africa by several sub-contractors. Key local suppliers include Efficient Engineering (pedestals and yokes); Titanus Slew Rings (azimuth bearings) and Tricom Structures (back-up structure), all based in Gauteng.

In some cases foreign companies will manufacture components for the first antenna - such as the first set of reflector panels, first receiver indexer and first sub-reflector - but the rest will be made locally. Suppliers from abroad include the National Research Council of Canada, through the Herzberg, Programs in Astronomy and Astrophysics (low-noise amplifiers and first sub-reflector); Oxford Cryosystems Ltd. (cryogenic coldheads) and Vertex Antennentechnik (control systems).

MeerKAT Schedule

  • Array Release 1 (6 receptors) Engineering Verification completed by 5 April 2016
    • 16 receptors and correlator available
  • Array Release 1 Science Commissioning completed 31 May 2016
    • once 6 done, the additional antennas gets added on a rolling basis (i.e. array commissioning significantly simplified)
  • 16 Antenna Array Science capable by 30 June 2016 (Commissioning done and science capability, but science on PI projects not scheduled to start by then)
  • Array Release 2 (32 receptors) Engineering Verification completed Dec 2016 (additional single receptors Engineering Verification completed)
  • Array Release 2 (32 receptors) Science commissioning completed 31 March 2017
    • Early Science (PI projects) starts
    • WB Imaging
    • Pulsar Timing
    • additional science modes to follow
  • Array Release 3 (64 antennas) Engineering Verification completed mid 2017
  • Array Release 3 (64 antennas) Science Commissioning completed in 2017
    • WB Imaging
    • Pulsar Timing
    • additional science modes to follow

MeerKAT's make-up

  • The MeerKAT telescope will be an array of 64 interlinked receptors (a receptor is the complete antenna structure, with the main reflector, sub-reflector and all receivers, digitisers and other electronics installed).

  • The configuration (placement) of the receptors is determined by the science objectives of the telescope.

  • 48 of the receptors are concentrated in the core area which is approximately 1 km in diameter.

  • The longest distance between any two receptors (the so-called maximum baseline) is 8 km.

  • Each MeerKAT receptor consists of three main components:
    1. The antenna positioner, which is a steerable dish on a pedestal;
    2. A set of radio receivers;
    3. A set of associated digitisers.

  • The antenna positioner is made up of the 13.5 m effective diameter main reflector, and a 3.8 m diameter sub-reflector. In this design, referred to as an 'Offset Gregorian' optical layout, there are no struts in the way to block or interrupt incoming electromagnetic signals. This ensures excellent optical performance, sensitivity and imaging quality, as well as good rejection of unwanted radio frequency interference from orbiting satellites and terrestrial radio transmitters. It also enables the installation of multiple receiver systems in the primary and secondary focal areas, and provides a number of other operational advantages.

  • The combined surface accuracy of the two reflectors is extremely high with a deviation from the ideal shape being no more than 0.6 mm RMS (root mean square). The main reflector surface is made up of 40 aluminium panels mounted on a steel support framework.

  • This framework is mounted on top of a yoke, which is in turn mounted on top of a pedestal. The combined height of the pedestal and yoke is just over 8 m. The height of the total structure is 19.5 m, and it weighs 42 tons.

  • The pedestal houses the antenna's pointing control system.

  • Mounted at the top of the pedestal, beneath the yoke, are an azimuth drive and a geared azimuth bearing, which allow the main and sub-reflectors, together with the receiver indexer, to be rotated horizontally. The yoke houses the azimuth wrap, which guides all the cables when the antenna is rotated, and prevents them from becoming entangled or damaged. The structure allows an observation elevation range from 15 to 88 degrees, and an azimuth range from -185 degrees to +275 degrees, where north is at zero degrees.

  • The steerable antenna positioner can point the main reflector very accurately, to within 5 arcseconds (1.4 thousandths of a degree) under low-wind and night-time observing conditions, and to within 25 arcseconds (7 thousandths of a degree) during normal operational conditions.

About MeerKAT - how it works

  • Electromagnetic waves from cosmic radio sources bounce off the main reflector, then off the sub-reflector, and are then focused in the feed horn, which is part of the receiver.

  • Each receptor can accommodate up to four receivers and digitisers mounted on the receiver indexer. The indexer is a rotating support structure that allows the appropriate receiver to be automatically moved into the antenna focus position, depending on the desired observation frequency.

  • The main function of the receiver is to capture the electromagnetic radiation and convert it to an voltage signal that is then amplified by cryogenic receivers that add very little noise to the signal. The first two receivers will be the L-Band and UHFBand Receivers.

  • Four digitisers will be mounted on the receiver indexer, close to the associated receivers. The function of the four digitisers is to convert the radio frequency (RF) voltage signal from the receiver into digital signals. This conversion is done by using an electronic component called an analogue to digital converter (ADC). The L-band digitiser samples at a rate of 1 712 million samples every second. (The amount of data that is generated by the digitiser for a receiver is equivalent to approximately 73 000 DVDs every day or almost 1 DVD per sec.)

  • Once the signal is converted to digital data, the digitiser sends this data via buried fibre optic cables to the correlator, which is situated inside the Karoo Array Processor Building (KAPB) at the Losberg site complex.

  • A total of 170 km of buried fi bre cables connect the receptors to the KAPB, with the maximum length between the KAPB and a single antenna being 12 km.

  • Thefi bre cables run inside conduits buried 1 m below the ground for thermal stability.

  • At the KAPB, the signals undergo various stages of digital processing, such as correlation - which combines all the signals from all the receptors to form an image of the area of the sky to which the antennas are pointing - and beam-forming, which coherently adds the signals from all the receptors to form a number of narrow, high sensitivity beams used for pulsar science. The science data products are also archived at the KAPB with a portion of the science archive data moved off site via fi bre connection and stored in Cape Town (with possibilities of reprocessing the data).

  • Time and frequency reference signals are distributed, via buried optical fi bres, to every digitiser on every receptor, so that they are all synchronised to the same clock. This is important to properly align the signals from all receptors.

  • The control and monitoring system is responsible for monitoring the health of the telescope and for controlling it to do what the operators want it to do. A large number of internal sensors (more than 150 000) monitor everything from electronic component temperatures to weather conditions and power consumption.

Why MeerKAT?

The telescope was originally known as the Karoo Array Telescope (KAT) that would consist of 20 receptors. When the South African government increased the budget to allow the building of 64 receptors, the team re-named it "MeerKAT" - ie "more of KAT". The MeerKAT (scientific name Suricata suricatta) is also a muchbeloved small mammal that lives in the Karoo region.

The KAT-7 precursor array has been constructed and is being used as an engineering and science prototype.