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Brown, Andrew
in Cooperation with on an Cooperation-Score of 37%
Topics
Publications (6/6 displayed)
- 2023Macromolecular crowding Is surprisingly unable to deform the structure of a model biomolecular condensatecitations
- 2022Impact of gene expression profile testing for lymph node positive (LN+) , hormone receptor positive (HR+), HER2 negative (HER2-) breast cancer (BC) patients on the use of adjuvant chemotherapy in a large community cancer center
- 2021(Hydroxy)apatite on cementcitations
- 2015ASKAP Mk II Phased-Array Feed: from the Laboratory to the Observatorycitations
- 2012ASKAP Beamformercitations
- 2007Microfluidic system for cell transfection using sonoporation and ultrasonic particle manipulation
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document
ASKAP Beamformer
Abstract
The SKA will be the mainstay of centimeter astronomy much ofthis century.It will have a sensitivity that is more than an order of magnitude greater than current radio telescopes.A second area for improved performance is field of view.For frequencies above 1GHz this may be achieved by placing a Phased Array Feed (PAF) at the focus of the SKA dishes.The design of the signal processing chain to convert the signal from a PAF to multiple independent beams on the sky is a major challenge.This paper describes the approach used by the Australian SKA Pathfinder (ASKAP) to achieve this.The approach leads to a telescope that has a 30 square degree field of view at 1.45GHz.