Scientific Timeline

Construction Schedule - Array Assemblies

Array Assemblies (AAs) are milestones in the construction, providing an end-to-end telescope system with pre-defined functionality.  The roll-out of dishes and antennas continues after each AA release, so that construction is continuous.  As full funding for AA4 is not yet committed, we are following the Staged Delivery program below with a planned pause at AA*.  If full funding is secured before then, the roll-out will continue after AA*.

Below is the schedule of AAs; the expected functionality of each AA is given further down this page.  

Updated November 2024.  Note that the construction schedule is updated each month at present, and the dates in this table reflect that schedule.  If the "updated" date is significantly different from today's date (i.e., > 3 months), then you may wish to request an updated schedule from us.   Q1=Jan-Mar; Q2=Apr-Jun; Q3=Jul-Sep; Q4=Oct-Dec.  

Science commissioning will start as soon as the first dish/station is available on site.  

AA0.5 is the first test array for interferometry, using prototype dishes and receivers for Mid.  This is an engineering array, used to discover system level issues early and develop procedures (e.g., pointing, tracking, holography).

AA2 is the start of science verification.  The performance of SKA at AA2 is at least as good as existing facilities in many aspects, and usually better (primarily in sensitivity).   Observations with AA2 will be used to ensure the system meets the needs of science users (verification of science requirements, testing of observing modes).  The observatory will undertake some observations of known objects, and make the data available to the community (similar to the model for ALMA science verification)

The planning for scientific observations involving the science community consists of four science milestones:

1. Science Verification (SV) is to demonstrate the science performance of SKA to the astronomical community, and will start once a sufficiently capable array of dishes or stations has been deployed and tested, with “Call for Suggestions” from the community (similar to the ALMA SV model).   Targets that have been observed in a similar manner with existing arrays for comparison are preferred.  The first scientifically interesting data will be publicly released to the community as part of SV.
2. As a transition between Science Verification and normal PI observing, it’s foreseen that there will be at least one Cycle of “shared risk” PI science, which means that, should a scheduled observation be unsuccessful, there would be no guarantee that the proposal would be rescheduled. This is anticipated to happen just after testing of the AA* components and the readiness review is complete.
3. Once the specific observation modes being offered in each time allocation cycle are fully commissioned, PI science will commence. This is anticipated to happen some months after testing of the AA* components is complete.
4. Key Science Projects (KSP) observations are the most ambitious SKA proposals. They will typically require significantly more observing time than PI proposals, and be carried out over more than one observing cycle. This mode of observation requires a very good understanding of the telescope and maturity of the data analysis pipeline, which should be achieved two years after AA* (and then AA4) testing is complete. The process to apply for telescope time in this mode will happen however much earlier, to ensure the KSP teams are notified well in advance of their observations, and can secure the necessary resources.

With these assumptions, the broad science timeline is as follows:

Summary Timeline

Mid AA2 layout | Low AA2 layout

Mid AA* layout| Low AA* layout