SKA staged delivery, array assemblies and subarrays

SKAO has adopted a staged approach to construction where the Low and Mid telescopes are constructed and verified in stages called array assemblies (AA). Interferometers lend themselves to easy expansion as new antennas can be added to existing arrays, provided sufficient compute and network resources are available to accommodate the increased data rates. Such an approach ensures that the full functionality of all the software and hardware can be tested and verified at the earliest possible stage during construction.

To clarify the staged delivery of the SKAO telescopes, we have published a memo (linked below) that provides the astronomy community with a single point of reference that describes the array assemblies, the list of antennas and their coordinates in the array assemblies that will be available to the scientific community from the start of Science Verification through to the full design baseline. 

The content presented in this document is complemented by a Python package (called ska_ost_array_config) that allows astronomers to simulate interferometric observations using both the entirety of the dishes or stations available during a particular AA, or a subset of those available (i.e. a “subarray”). Both Low and Mid telescopes are capable of providing up to 16 concurrent subarrays, offering a lot of flexibility to both operations and science observing. 

The memo and the software package can be accessed using the links below:

We encourage feedback from the SKA users community, ideally addressed to

Last modified on 20 June 2024