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TRANSCRIPT
MWA Project:
Site: Murchison Radio Observatory Australia’s proposed SKA Site
Strategy: 512 Antenna “Tiles”• Explore “Large N / Small D” regime• Correlate all pairs• Instantaneous complete UV coverage• confront issues with Wide-Field Imaging, Foregrounds, Dynamic Range, …
MWA Project:
Science goals: Epoch of Re-ionization Transients, Sun, …
Implications… Compact, Dense Array Diameter ~ 1.5 km Frequency coverage 80-320 MHz
MWA Project: Consortium:• MIT Haystack Observatory• MIT Kavli Institute• Harvard-Smithsonian Center for Astrophyics• Australian universities (Curtin, ANU, Melbourne, Swinburne, Sydney, Tasmania, Western Australia, …)
• Raman Research Institute • CSIRO/ATNF
Antenna tile (~4m diam.)
clusters
Array (~1.5km diam.)tile
Cluster (50-100m diam.)
node
Coax outTile beamformer Fiber out
Central Processing
Hierarhical groupings
Receiver Node Housing• 64 Nodes• Coax RF input from 8 Tiles• Fiber digital output
Derek Caroll - PSI
Correlator:
• FPGA based “hardware correlator” and fine Filter Bank (10KHz channels)
• Correlate all pairs => 130,816 Interferometer Baselines
• (Prototyping & Testing … baseband recorders, software filter banks and correlators, …)