How Electromagnetic Models can improve astronomical observations in the Square Kilometre Array Radio Telescope

Abstract

The Square Kilometer Array is an ambitious project aiming to tackle some of the most fundamental scientific questions of our time and revolutionize our understanding of the Universe. The SKA is made up of two world-leading complementary radio telescopes on two continents, and will cover a very wide frequency range from 50 MHz up to 15 GHz+. These telescopes represent a game-changer for radio astronomy and, to achieve the science goals, precise prediction and knowledge of the telescopes’ performance and behavior are essential. This contribution provides insights into the importance of electromagnetic models in prediction, support, and verification of astronomical observations with the Square Kilometer Array.