We present results from the first all-sky radio survey in circular polarization. The survey uses the Murchison Widefield Array (MWA) to cover 30 900 sq deg, over declinations south of +30° and north of -86° centred at 200MHz (over a 169-231MHz band).We achieve a spatial resolution of ~3 arcmin and a typical sensitivity of 3.0mJy PSF-1over most of the survey region. We demonstrate a new leakage mitigation technique that reduces the leakage from total intensity into circular polarization by an order of magnitude. In a blind survey of the imaged region, we detect 14 pulsars in circular polarization above a 6s threshold. We also detect six transient sources associated with artificial satellites. A targeted survey of 2376 pulsars within the surv...
We report the results of a 154 MHz survey to search for emission from exoplanets located in the Upp...
We present polarization measurements at 8.4, 22, and 43 GHz made with the Very Large Array (VLA) of ...
We present deep polarimetric observations at 154 MHz with the Murchison Widefield Array (MWA), cover...
Callingham JR, Shimwell TW, Vedantham HK, et al. V-LoTSS: The circularly polarised LOFAR Two-metre S...
International audienceWe present the detection of 68 sources from the most sensitive radio survey in...
The low-frequency linearly polarised radio source population is largely unexplored. However, a renai...
© 2014 The Authors. We present the results of a survey for low-frequency radio emission from 17 know...
The low-frequency polarisation properties of radio sources are poorly studied, particularly in stati...
Polarization profiles are presented for 20 millisecond pulsars that are being observed as part of th...
We analyse the circular polarization data accumulated in the first 7 years of the Polarimetric Monit...
International audienceContext: While there is evidence for considerable circular polarization of OH ...
We report on measurements of the polarization of extragalactic sources at.148 GHz made during the fi...
We report the first detections of circularly polarized emission at submillimeter wavelengths from th...
Context: Linear polarization of Galactic synchrotron emission provides valuable information on the G...
The Sun is an active star that often produces numerous bursts of electromagnetic radiation at radio ...
We report the results of a 154 MHz survey to search for emission from exoplanets located in the Upp...
We present polarization measurements at 8.4, 22, and 43 GHz made with the Very Large Array (VLA) of ...
We present deep polarimetric observations at 154 MHz with the Murchison Widefield Array (MWA), cover...
Callingham JR, Shimwell TW, Vedantham HK, et al. V-LoTSS: The circularly polarised LOFAR Two-metre S...
International audienceWe present the detection of 68 sources from the most sensitive radio survey in...
The low-frequency linearly polarised radio source population is largely unexplored. However, a renai...
© 2014 The Authors. We present the results of a survey for low-frequency radio emission from 17 know...
The low-frequency polarisation properties of radio sources are poorly studied, particularly in stati...
Polarization profiles are presented for 20 millisecond pulsars that are being observed as part of th...
We analyse the circular polarization data accumulated in the first 7 years of the Polarimetric Monit...
International audienceContext: While there is evidence for considerable circular polarization of OH ...
We report on measurements of the polarization of extragalactic sources at.148 GHz made during the fi...
We report the first detections of circularly polarized emission at submillimeter wavelengths from th...
Context: Linear polarization of Galactic synchrotron emission provides valuable information on the G...
The Sun is an active star that often produces numerous bursts of electromagnetic radiation at radio ...
We report the results of a 154 MHz survey to search for emission from exoplanets located in the Upp...
We present polarization measurements at 8.4, 22, and 43 GHz made with the Very Large Array (VLA) of ...
We present deep polarimetric observations at 154 MHz with the Murchison Widefield Array (MWA), cover...