We present polarization measurements at 8.4, 22, and 43 GHz made with the Very Large Array (VLA) of a complete sample of extragalactic sources stronger than 1 Jy in the 5 yr Wilkinson Microwave Anisotropy Probe (WMAP) catalogue and with declinations north of -34 degrees. The observations were motivated by the need to know the polarization properties of radio sources at frequencies of tens of GHz in order to subtract polarized foregrounds for future sensitive cosmic microwave background (CMB) experiments. The total intensity and polarization measurements are generally consistent with comparable VLA calibration measurements for less-variable sources, and within a similar range to WMAP fluxes for unresolved sources. A further paper will presen...
We present the largest ever sample of radio polarization properties for z > 4 sources, with 14 sourc...
Article first published online: 1 AUG 2006We present some first results on the variability, polariza...
Galactic synchrotron emission represents the most relevant foreground contamination in cosmic microw...
We present polarization measurements at 8.4, 22, and 43 GHz made with the VLA of a complete sample o...
We present polarization measurements of extragalactic radio sources observed during the cosmic micro...
A sample of 129 unresolved radio sources with ultrahigh linear polarization (> 30 per cent) has been...
We investigate the statistical properties of the polarized emission of extragalactic radio sources a...
We investigate the statistical properties of the polarized emission of extragalactic radio sources a...
We report on measurements of the polarization of extragalactic sources at.148 GHz made during the fi...
We have observed 250 of the 258 southern sources in the complete 5 GHz 1 Jy sample by Kühr et al. (...
The high-frequency (> 20 GHz), bright flux density (> 200 mJy) radio population is dominated by blaz...
The Wilkinson Microwave Anisotropy Probe (WMAP) has mapped the entire sky in five frequency bands be...
We have used the very large JVAS/CLASS 8.4-GHz surveys of flat-spectrum radio sources to obtain a la...
© 2017 The Author(s). We present high sensitivity (s P ~- 0.6mJy) polarimetric observations in seven...
We present polarization data for 180 extragalactic sources extracted from the Australia Telescope 20...
We present the largest ever sample of radio polarization properties for z > 4 sources, with 14 sourc...
Article first published online: 1 AUG 2006We present some first results on the variability, polariza...
Galactic synchrotron emission represents the most relevant foreground contamination in cosmic microw...
We present polarization measurements at 8.4, 22, and 43 GHz made with the VLA of a complete sample o...
We present polarization measurements of extragalactic radio sources observed during the cosmic micro...
A sample of 129 unresolved radio sources with ultrahigh linear polarization (> 30 per cent) has been...
We investigate the statistical properties of the polarized emission of extragalactic radio sources a...
We investigate the statistical properties of the polarized emission of extragalactic radio sources a...
We report on measurements of the polarization of extragalactic sources at.148 GHz made during the fi...
We have observed 250 of the 258 southern sources in the complete 5 GHz 1 Jy sample by Kühr et al. (...
The high-frequency (> 20 GHz), bright flux density (> 200 mJy) radio population is dominated by blaz...
The Wilkinson Microwave Anisotropy Probe (WMAP) has mapped the entire sky in five frequency bands be...
We have used the very large JVAS/CLASS 8.4-GHz surveys of flat-spectrum radio sources to obtain a la...
© 2017 The Author(s). We present high sensitivity (s P ~- 0.6mJy) polarimetric observations in seven...
We present polarization data for 180 extragalactic sources extracted from the Australia Telescope 20...
We present the largest ever sample of radio polarization properties for z > 4 sources, with 14 sourc...
Article first published online: 1 AUG 2006We present some first results on the variability, polariza...
Galactic synchrotron emission represents the most relevant foreground contamination in cosmic microw...