Antenna Array Characterization via Radio Interferometry Observation of Astronomical Sources
We present an in-situ antenna characterization method and results for a “low-frequency” radio astronomy engineering prototype array, characterized over the 75–300 MHz frequency range. The presence of multiple cosmic radio sources, particularly the dominant Galactic noise, makes in-situ characterizat...
| Main Authors: | , , , , , , , , , , , , , , |
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| Other Authors: | |
| Format: | Conference Paper |
| Published: |
IEEE Explore
2014
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| Online Access: | http://hdl.handle.net/20.500.11937/25205 |