International audienceThe observation of known pulsars (pulsar timing) or the search for new pulsars can be limited by radio frequency interference (RFI) generated by Telecommunication activity. In this paper, we propose several RFI mitigation techniques to cope with impulsive and/or narrow band RFI. For pulsar timing, we have implemented, a pulse blanker and a cyclostationary blanker, both in real time. For pulsar search, we propose a new approach which combines a hardware-efficient search method and some RFI mitigation capabilities. This method is based on a 2D FFT and Radon transform
Current and upcoming radio telescopes are being designed with increasing sensitivity to detect new a...
As the use of wireless technology has increased around the world, Radio Frequency Interference (RFI)...
In this paper, we present a framework for assessing the effect of non-stationary Gaussian noise and ...
International audienceThe observation of known pulsars (pulsar timing) or the search for new pulsars...
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...
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...
Abstract. Radio astronomy has protected frequency bands for free observations. However, it is often ...
Radio astronomy has protected frequency bands for free observations. However, it is often necessary ...
National audienceRadio astronomical pulsar observations require specific instrumentation and dedicat...
International audienceAs the use of wireless technology has increased around the world, RadioFrequen...
International audienceRadio Frequency Interference (RFI) is a profound obstacle for radio astronomy,...
Les travaux présentés dans ce mémoire s’inscrivent dans le cadre de la détection d’évènements impuls...
The work presented in this thesis is in the context of the intermittent impulsive event detection at...
Current and upcoming radio telescopes are being designed with increasing sensitivity to detect new a...
As the use of wireless technology has increased around the world, Radio Frequency Interference (RFI)...
In this paper, we present a framework for assessing the effect of non-stationary Gaussian noise and ...
International audienceThe observation of known pulsars (pulsar timing) or the search for new pulsars...
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...
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...
Abstract. Radio astronomy has protected frequency bands for free observations. However, it is often ...
Radio astronomy has protected frequency bands for free observations. However, it is often necessary ...
National audienceRadio astronomical pulsar observations require specific instrumentation and dedicat...
International audienceAs the use of wireless technology has increased around the world, RadioFrequen...
International audienceRadio Frequency Interference (RFI) is a profound obstacle for radio astronomy,...
Les travaux présentés dans ce mémoire s’inscrivent dans le cadre de la détection d’évènements impuls...
The work presented in this thesis is in the context of the intermittent impulsive event detection at...
Current and upcoming radio telescopes are being designed with increasing sensitivity to detect new a...
As the use of wireless technology has increased around the world, Radio Frequency Interference (RFI)...
In this paper, we present a framework for assessing the effect of non-stationary Gaussian noise and ...