Details
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Enabler
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Won't have (this time)
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None
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None
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Data Processing
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2
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SPO-1002
Description
Visibility prediction is one of the most time consuming steps in the self-calibration loop, in particular when a complex source model (many source components, diffuse emission) is involved. Prediction using Image Domain Gridding (IDG), IDGpredict, could be a computationally attractive alternative to direct prediction. However, at the moment, experience from LOFAR indicates that the crossover point at which IDGpredict computationally outperforms direct prediction lies at several thousands of source components. As system architect, I want to know where the crossover point will be for the SKA-Low and SKA-Mid arrays is (expressed in number of source components in the source model), so that I can make an informed decision on further development of processing functions for visibility prediction.