KAT-7

It also served as a technology demonstrator for South Africa's bid to host the Square Kilometre Array. The first Radio telescope to be built with a composite reflector and uses a stirling pump for 75 K cryogenic cooling. The telescope was built to test various systems for the MeerKAT array, from the ROACH correlators designed and manufactured in Cape Town, now used by various telescopes internationally, to composite construction techniques.

KAT-7 consist of 7 dishes of 12 metres in diameter, each a prime focus reflecting telescope. Key performance parameters • Parameter || Value • Number of antennae — 7 • Dish diameter — 12 m • Minimum baseline — 26 m • Maximum baseline — 185 m • Frequency Range — 1200...1950 MHz • Instantaneous Bandwidth — 256 MHz • Polarisation — Linear (H + V) • Tsys — for all elevation angles above 30°: < 35 K across the entire frequency band ~ 30 K average • Elevation — 2...95° Correlator Modes: • Mode || # Bands || Band Bandwidth || Channel Bandwidth || available? • Wideband — 1 — 256 MHz — 390.625 kHz — Yes • 8k Wideband — 1 — 256 MHz — 48.8 kHz — Yes • HI Spectral Line — 1 — ≥ 33.4 MHz — ≤ 4.8 kHz — ~ Oct 2012 • OH Spectral Line — 1 — 400/32 = 12.5 MHz — 1.5 kHz — ~ Jun 2012 • OH Spectral Line — 1 — 400/128 = 3.1 MHz — 0,381 kHz — ~ Jun 2012

In April 2010 four of the seven dishes were linked together as an integrated system to produce its first interferometric image of an astronomical object. In Dec 2010, there was a successful detection of very long baseline interferometry (VLBI) fringes between the Hartebeesthoek Radio Astronomy Observatory's 26 m dish and one of the KAT-7 dishes.