1. Measured aperture-array noise temperature of the Mark II phased array feed for ASKAP
- Author
-
Aaron Chippendale, Brown, A. J., Beresford, R. J., Hampson, G. A., Shaw, R. D., Hayman, D. B., Macleod, A., Forsyth, A. R., Hay, S. G., Leach, M., Cantrall, C., Brothers, M. L., and Hotan, A. W.
- Subjects
Astrophysics::Instrumentation and Methods for Astrophysics ,FOS: Physical sciences ,Astrophysics::Cosmology and Extragalactic Astrophysics ,Astrophysics - Instrumentation and Methods for Astrophysics ,Instrumentation and Methods for Astrophysics (astro-ph.IM) - Abstract
We have measured the aperture-array noise temperature of the first Mk. II phased array feed that CSIRO has built for the Australian Square Kilometre Array Pathfinder telescope. As an aperture array, the Mk. II phased array feed achieves a beam equivalent noise temperature less than 40 K from 0.78 GHz to 1.7 GHz and less than 50 K from 0.7 GHz to 1.8 GHz for a boresight beam directed at the zenith. We believe these are the lowest reported noise temperatures over these frequency ranges for ambient-temperature phased arrays. The measured noise temperature includes receiver electronics noise, ohmic losses in the array, and stray radiation from sidelobes illuminating the sky and ground away from the desired field of view. This phased array feed was designed for the Australian Square Kilometre Array Pathfinder to demonstrate fast astronomical surveys with a wide field of view for the Square Kilometre Array., Comment: 5 pages, 4 figures, accepted for publication in Antennas and Propagation (ISAP), 2015 International Symposium on