The Boolardy Engineering Test Array (BETA) is a 6 antenna interferometer, with each antenna having a 188-element phased array feed at the prime focus. Here we attempt to mitigate the affect of radio frequency interference (RFI) by updating the beam weights using a projection algorithm applied to the measured single-dish array covariance matrix. We observe an astronomical source at 1225 MHz, which contains substantial interference from the GPS L2 band, and compare a number of different projection algorithms by looking at the affect on correlated visibilities, and on the resulting images. The RFI projection algorithms perform remarkably well, yielding a promising future for this technique
The next generation of radio telescopes is expected to be one to two orders of magnitude more sensit...
The Square Kilometre Array (SKA) Phase 1 Mid Correlator Beamformer (Mid.CBF) adopts two novel method...
Microwave radiometry field has been increasing its performance with higher accuracy measurements, le...
Radio Frequency Interference (RFI) is probably one of the most important limiting factors in the acc...
© 2018 IEEE. Radio-frequency interference (RFI) is a critical problem in radio astronomy observation...
National audienceRadio astronomy is a passive service and is equipped to observe extremely weak sign...
International audienceBecause of the denser active use of the spectrum, and because of higher radio ...
Radio interferometers are phased arrays producing high-resolution images from the covariance matrix ...
International audienceRadio interferometers are phased arrays producing high-resolution images from ...
Radio frequency interference (RFI) is a signi¯cant problem for current and future radio telescopes. ...
Spatial Radio Frequency Interference (RFI) filtering offers both RFI rejection and potential signal-...
Radio Frequency Interference (RFI) is a massive problem for radio observatories around the world. Du...
International audienceRadio Frequency Interference (RFI) is a profound obstacle for radio astronomy,...
International audiencePhased array radio telescopes allow for the filtering of Radio Frequency Inter...
International audienceRadio astronomical observations are increasingly corrupted by radio frequency ...
The next generation of radio telescopes is expected to be one to two orders of magnitude more sensit...
The Square Kilometre Array (SKA) Phase 1 Mid Correlator Beamformer (Mid.CBF) adopts two novel method...
Microwave radiometry field has been increasing its performance with higher accuracy measurements, le...
Radio Frequency Interference (RFI) is probably one of the most important limiting factors in the acc...
© 2018 IEEE. Radio-frequency interference (RFI) is a critical problem in radio astronomy observation...
National audienceRadio astronomy is a passive service and is equipped to observe extremely weak sign...
International audienceBecause of the denser active use of the spectrum, and because of higher radio ...
Radio interferometers are phased arrays producing high-resolution images from the covariance matrix ...
International audienceRadio interferometers are phased arrays producing high-resolution images from ...
Radio frequency interference (RFI) is a signi¯cant problem for current and future radio telescopes. ...
Spatial Radio Frequency Interference (RFI) filtering offers both RFI rejection and potential signal-...
Radio Frequency Interference (RFI) is a massive problem for radio observatories around the world. Du...
International audienceRadio Frequency Interference (RFI) is a profound obstacle for radio astronomy,...
International audiencePhased array radio telescopes allow for the filtering of Radio Frequency Inter...
International audienceRadio astronomical observations are increasingly corrupted by radio frequency ...
The next generation of radio telescopes is expected to be one to two orders of magnitude more sensit...
The Square Kilometre Array (SKA) Phase 1 Mid Correlator Beamformer (Mid.CBF) adopts two novel method...
Microwave radiometry field has been increasing its performance with higher accuracy measurements, le...