"The beamformer improves the SNR of the weak signal by factor sqrt(S). For most very weak astronimical signals this is not enough to make them appear above the system noise, so then additional beamforming is needed or integration in time using a correlator."
The beamformer improves the SNR of the weak signal by factor sqrt(S). For most very weak astronimical signals this is not enough to make them appear above the system noise, so then additional beamforming is needed or integration in time using a correlator.