Abstract
We report characterization results for an engineering prototype of a next-generation low-frequency radio astronomy array. This prototype, which we refer to as the Aperture Array Verification System 0.5 (AAVS0.5), is a sparse pseudo-random array of 16 log-periodic antennas designed for 70–450 MHz. It is co-located with the Murchison Widefield Array (MWA) at the Murchison Radioastronomy Observatory (MRO) near the Australian Square Kilometre Array (SKA) core site. We characterize the AAVS0.5 using two methods: in-situ radio interferometry with astronomical sources and an engineering approach based on detailed full-wave simulation. Insitu measurement of the small prototype array is challenging due to the dominance of the Galactic noise and the relatively weaker calibration sources easily accessible in the southern sky. The MWA, with its 128 “tiles” and up to 3 km baselines, enabled in-situ measurement via radio interferometry.We present array sensitivity and beam pattern characterization results and compare to detailed full-wave simulation. We discuss areas where differences between the two methods exist and offer possibilities for improvement. Our work demonstrates the value of the dual astronomy–simulation approach in upcoming SKA design work.
Author
Sutinjo, A., Colegate, T. ; Wayth, R. ; Hall, P. ; de Lera Acedo, E. ; Booler, T. ; Faulkner, A. ; Feng, L. ; Hurley-Walker, N. ; Juswardy, B. ; Padhi, S. ; Razavi-Ghods, N. ; Sokolowski, M. ; Tingay, S. ; Vaate, J.
Journal
IEEE Transactions on Antennas and Propagation
Paper Publication Date
October 2015
Paper Type
Astroinformatics