Current and upcoming radio telescopes are being designed with increasing sensitivity to detect new and mysterious radio sources of astrophysical origin. While this increased sensitivity improves the likelihood of discoveries, it also makes these instruments more susceptible to the deleterious effects of Radio Frequency Interference (RFI). The challenge posed by RFI is exacerbated by the high data-rates achieved by modern radio telescopes, which require real-time processing to keep up with the data. Furthermore, the high data-rates do not allow for permanent storage of observations at high resolution. Offline RFI mitigation is therefore not possible anymore. The real-time requirement makes RFI mitigation even more challenging because, on one...
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...
International audienceThe observation of known pulsars (pulsar timing) or the search for new pulsars...
Radio Frequency Interference (RFI) mitigation is extremely important to take advantage of the vastly...
International audienceRadio Frequency Interference (RFI) is a profound obstacle for radio astronomy,...
As the use of wireless technology has increased around the world, Radio Frequency Interference (RFI)...
National audienceRadio astronomical pulsar observations require specific instrumentation and dedicat...
Context. Apertif is a multi-beam receiver system for the Westerbork Synthesis Radio Telescope that o...
International audienceAs the use of wireless technology has increased around the world, RadioFrequen...
National audienceRadio astronomy is a passive service and is equipped to observe extremely weak sign...
From the Washington University Senior Honors Thesis Abstracts (WUSHTA), Spring 2018. Published by th...
Radio transient discovery using next generation radio telescopes will pose several digital signal pr...
Fast Radio Bursts must be powered by uniquely energetic emission mechanisms. This requirement has el...
The observation of known pulsars (pulsar timing) or the search for new pulsars can be limited by rad...
In this paper we present an interference detection toolbox consisting of a high dynamic range Digita...
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...
International audienceThe observation of known pulsars (pulsar timing) or the search for new pulsars...
Radio Frequency Interference (RFI) mitigation is extremely important to take advantage of the vastly...
International audienceRadio Frequency Interference (RFI) is a profound obstacle for radio astronomy,...
As the use of wireless technology has increased around the world, Radio Frequency Interference (RFI)...
National audienceRadio astronomical pulsar observations require specific instrumentation and dedicat...
Context. Apertif is a multi-beam receiver system for the Westerbork Synthesis Radio Telescope that o...
International audienceAs the use of wireless technology has increased around the world, RadioFrequen...
National audienceRadio astronomy is a passive service and is equipped to observe extremely weak sign...
From the Washington University Senior Honors Thesis Abstracts (WUSHTA), Spring 2018. Published by th...
Radio transient discovery using next generation radio telescopes will pose several digital signal pr...
Fast Radio Bursts must be powered by uniquely energetic emission mechanisms. This requirement has el...
The observation of known pulsars (pulsar timing) or the search for new pulsars can be limited by rad...
In this paper we present an interference detection toolbox consisting of a high dynamic range Digita...
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...
International audienceThe observation of known pulsars (pulsar timing) or the search for new pulsars...