A powerful real time Radio-frequency interference (RFI) mitigation back-end system is presented in this work. The interfering signals are estimated by using the wavelet transform to utilize its effective denoising capability. The estimated RFI signals are then subtracted from the total received signal, and ultimately the RFI-mitigated signal is obtained. Here, the hardware implementation and the system tests are demonstrated, showing sinusoid, chirp, and PRN interference mitigation under different Interference to Noise Ratios (INRs).Peer Reviewe
International audienceThe observation of known pulsars (pulsar timing) or the search for new pulsars...
The observation of known pulsars (pulsar timing) or the search for new pulsars can be limited by rad...
Current and upcoming radio telescopes are being designed with increasing sensitivity to detect new a...
A powerful real time Radio-frequency interference (RFI) mitigation back-end system is presented in t...
Radio-frequency interference (RFI) is a serious problem in microwave radiometry. In order to process...
Microwave radiometers are very sensitive passive sensors that measure the power of the thermal noise...
Radio-Frequency Interference (RFI) is a growing problem specially for those systems that work with ...
Radio Frequency Interference (RFI) is the most common problem for electronic measuring systems. The ...
The performance of microwave radiometers can be seriously degraded by the presence of radio-frequenc...
The performance of microwave radiometers can be seriously degraded by the presence of radio-frequenc...
International audienceThe observation of known pulsars (pulsar timing) or the search for new pulsars...
The research work described in this paper is focused on the topic of the Radio Frequency Interferenc...
National audienceRadio astronomical pulsar observations require specific instrumentation and dedicat...
International audienceRadio Frequency Interference (RFI) is a profound obstacle for radio astronomy,...
The observation of known pulsars (pulsar timing) or the search for new pulsars can be limited by rad...
International audienceThe observation of known pulsars (pulsar timing) or the search for new pulsars...
The observation of known pulsars (pulsar timing) or the search for new pulsars can be limited by rad...
Current and upcoming radio telescopes are being designed with increasing sensitivity to detect new a...
A powerful real time Radio-frequency interference (RFI) mitigation back-end system is presented in t...
Radio-frequency interference (RFI) is a serious problem in microwave radiometry. In order to process...
Microwave radiometers are very sensitive passive sensors that measure the power of the thermal noise...
Radio-Frequency Interference (RFI) is a growing problem specially for those systems that work with ...
Radio Frequency Interference (RFI) is the most common problem for electronic measuring systems. The ...
The performance of microwave radiometers can be seriously degraded by the presence of radio-frequenc...
The performance of microwave radiometers can be seriously degraded by the presence of radio-frequenc...
International audienceThe observation of known pulsars (pulsar timing) or the search for new pulsars...
The research work described in this paper is focused on the topic of the Radio Frequency Interferenc...
National audienceRadio astronomical pulsar observations require specific instrumentation and dedicat...
International audienceRadio Frequency Interference (RFI) is a profound obstacle for radio astronomy,...
The observation of known pulsars (pulsar timing) or the search for new pulsars can be limited by rad...
International audienceThe observation of known pulsars (pulsar timing) or the search for new pulsars...
The observation of known pulsars (pulsar timing) or the search for new pulsars can be limited by rad...
Current and upcoming radio telescopes are being designed with increasing sensitivity to detect new a...