2015/10/12 by Claude Carignan, C. Carignan, Carignan, Claude
Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysics of Galaxies (astro-ph.GA) #FOS: Physical sciences #Radio Astronomy Observations and Technology #Superconducting and THz Device Technology #astro-ph.GA
paper · pdf · doi:10.48550/arxiv.1510.03462
6 pages, 4 figures, to be published in ASP Conf. Ser., Proceedings of the conference "Frontiers in Radio Astronomy and FAST Early Sciences Symposium 2015 (FRA 2015)", held in Guiyang, China, July 29-31 2015 (V2: typos corrected)
openalex publication_date 2015/10/12 · arxiv created 2015/10/15 · arxiv updated 2015/10/16 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
The seven-dish KAT-7 array was built as an engineering test-bed for the 64-dish Karoo Array Telescope, known as MeerKAT, which is the South African precursor of the Square Kilometre Array (SKA). KAT-7 and MeerKAT are located close to the South African SKA core site in the Northern Cape's Karoo desert region. Construction of the KAT-7 array was completed in December 2010. The short baselines (26 to 185 m) and low system temperature (T\rm sys ∼ 26 K) of the telescope make it very sensitive to large-scale, low-surface-brightness emission, which is one of the HI science drivers for MeerKAT and one of the future strengths of FAST. While the main purpose of KAT-7 was to test technical solutions for MeerKAT and the SKA, scientific targets were also observed during commissioning to test the HI line mode and the first results obtained are presented. A description of MeerKAT and an update on its construction is also given. Early science should start in mid-2016 with a partial array and the full array should be completed at the end of 2017. For cosmic-web research (detection of low column density HI), a future combination of data from FAST and MeerKAT should allow to explore the unknown territory of < 1018 cm-2 surface densities and the possible connection between spiral galaxies and the surrounding cosmic web.