  We describe the development of a noise-temperature testing capability for
phased-array antennas operating in receive mode from 0.7 GHz to 1.8 GHz.
Sampled voltages from each array port were recorded digitally as the
zenith-pointing array under test was presented with three scenes: (1) a large
microwave absorber at ambient temperature, (2) the unobstructed radio sky, and
(3) broadband noise transmitted from a reference antenna centred over and
pointed at the array under test. The recorded voltages were processed in
software to calculate the beam equivalent noise temperature for a maximum
signal-to-noise ratio beam steered at the zenith. We introduced the
reference-antenna measurement to make noise measurements with reproducible,
well-defined beams directed at the zenith and thereby at the centre of the
absorber target. We applied a detailed model of cosmic and atmospheric
contributions to the radio sky emission that we used as a noise-temperature
reference. We also present a comprehensive analysis of measurement uncertainty
including random and systematic effects. The key systematic effect was due to
uncertainty in the beamformed antenna pattern and how efficiently it
illuminates the absorber load. We achieved a combined uncertainty as low as 4 K
for a 40 K measurement of beam equivalent noise temperature. The measurement
and analysis techniques described in this paper were pursued to support
noise-performance verification of prototype phased-array feeds for the
Australian Square Kilometre Array Pathfinder telescope.
