KAT-7
Radio telescope in South Africa
From Wikipedia, the free encyclopedia
KAT-7 is a radio telescope situated in the Meerkat National Park, in the Northern Cape of South Africa. Developed as the precursor engineering test bed to the larger MeerKAT telescope, previously known as Karoo Array Telescope (KAT), it has become a science instrument in its own right. The construction was completed in 2011 and commissioning in 2012. It also served as a technology demonstrator for South Africa's bid to host the Square Kilometre Array.[1] KAT-7 is 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.[2]
Five antennas of KAT-7 in 2014 | |
| Location(s) | South Africa |
|---|---|
| Coordinates | 30°43′16″S 21°24′40″E |
| Altitude | 1,100 m (3,600 ft) |
| Wavelength | 3 cm (10.0 GHz)–30 cm (1,000 MHz) |
| Diameter | 12 m (39 ft 4 in) |
| Collecting area | 2,000 m2 (22,000 sq ft) |
| Website | www |
  Location of KAT-7 | |
 Related media on Commons | |
Technical specifications
KAT-7 consist of 7 dishes of 12 metres in diameter, each a prime focus reflecting telescope.[3]
| 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° |
| 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 |
Performance
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.[4]
