ASKAP is designed to be a high speed survey instrument with high dynamic range. This requires an extremely wide field-of-view interferometer with Phased Array Feeds (PAFs). The PAF has a total of 188 elements, 94 in each of two polarizations.
The specification for ASKAP is:
A total collecting area of approximately 4,000 square metres, from 36 antennas each 12 metres in diameter
System temperature less than 50 K
Frequency range from 700 MHz to 1.8 GHz
300 MHz instantaneous bandwidth
36 independent beams, each of about 1 square degree, yield overlapping to a 30 square degree field-of-view at 1.4 GHz
Maximum baseline of approximately 6 km
Full cross-correlation of all antennas
Possible remote array station capability located in NSW, approximately 3,000 km from the core site.
ASKAP user community workshops ideas October 2014: Members of the ASKAP Science Survey Teams and other potential ASKAP users met this week at the Marsfield headquarters of CSIRO Astronomy and Space Science in a one-day workshop to discuss the next steps for ASKAP.
"The sun never sets on the SKA" October 2014: In what has been called “the largest ever gathering of people working on the international SKA project”, some 300 engineers and scientists recently gathered in Fremantle, WA, to progress the development of the international SKA telescope.