Abstract / truncated to 115 words (read the full abstract)

The radio astronomical community is currently developing and building several new radio telescopes based on phased array technology. These telescopes provide a large field-of-view, that may in principle span a full hemisphere. This makes calibration and imaging very challenging tasks due to the complex source structures and direction dependent radio wave propagation effects. In this thesis, calibration and imaging methods are developed based on least squares estimation of instrument and source parameters. Monte Carlo simulations and actual observations with several prototypes show that this model based approach provides statistically and computationally efficient solutions. The error analysis provides a rigorous mathematical framework to assess the imaging performance of current and future radio telescopes in terms of ... toggle 4 keywords

calibration imaging radio astronomy array processing

Information

Author
Wijnholds, Stefan J.
Institution
Delft University of Technology
Supervisor
Publication Year
2010
Upload Date
April 8, 2010

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