Abstract
It is shown that the excellent Murchison Radio-astronomy Observatory site allows the Murchison
Widefield Array to employ a simple RFI blanking scheme and still calibrate visibilities and form
images in the FM radio band. The techniques described are running autonomously in our calibration
and imaging software, which is currently being used to process an FM-band survey of the
entire southern sky.
| Original language | English |
|---|---|
| Number of pages | 6 |
| Journal | Proceedings of Science |
| Volume | 122 |
| Issue number | 897 |
| Publication status | Published - 2010 |
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