We present the wide-field imaging and polarimetry at ? = 20 GHz of seven most extended, bright (Stotal = 0.50 Jy), high-frequency selected radio sources in the southern sky with declinations d < -30°. Accompanying the data are brief reviews of the literature for each source. The results presented here aid in the statistical completeness of the Australia Telescope 20-GHz Survey: the Bright Source Sample. The data are of crucial interest for future cosmic microwave background missions as a collection of information about candidate calibrator sources. We were able to obtain data for seven of the nine sources identified by our selection criteria. We report that Pictor A is thus far the best extragalactic calibrator candidate for the Low Freq...
We present polarization measurements at 8.4, 22, and 43 GHz made with the Very Large Array (VLA) of ...
We have observed 250 of the 258 southern sources in the complete 5 GHz 1 Jy sample by Kühr et al. (...
We present techniques developed to calibrate and correct Murchison Widefield Array low-frequency (72...
Sky at 20 GHz. The survey began in 2004 and we will complete observations of the whole Southern Sky ...
Pictor A is one of the brightest and most extended radio sources of the Southern Hemisphere. Its dis...
We present polarization data for 180 extragalactic sources extracted from the Australia Telescope 20...
© 2017 The Author(s). We present high sensitivity (s P ~- 0.6mJy) polarimetric observations in seven...
The Australia Telescope 20-GHz (AT20G) Survey is a blind survey of the whole southern sky at 20 GHz ...
We present high sensitivity (~0.6 mJy) polarimetric observations in seven bands, from 2.1 to 38 GHz,...
The Australia Telescope 20-GHz (AT20G) Survey is a blind survey of the whole southern sky at 20 GHz ...
We present some first results on the variability, polarization and general properties of radio sourc...
The low-frequency polarisation properties of radio sources are poorly studied, particularly in stati...
Basu A, Schwarz D, Kloeckner H-R, et al. CMB foreground measurements through broad-band radio spectr...
Restricted Access. An open-access version is available at arXiv.org (one of the alternative location...
Restricted Access. An open-access version is available at arXiv.org (one of the alternative location...
We present polarization measurements at 8.4, 22, and 43 GHz made with the Very Large Array (VLA) of ...
We have observed 250 of the 258 southern sources in the complete 5 GHz 1 Jy sample by Kühr et al. (...
We present techniques developed to calibrate and correct Murchison Widefield Array low-frequency (72...
Sky at 20 GHz. The survey began in 2004 and we will complete observations of the whole Southern Sky ...
Pictor A is one of the brightest and most extended radio sources of the Southern Hemisphere. Its dis...
We present polarization data for 180 extragalactic sources extracted from the Australia Telescope 20...
© 2017 The Author(s). We present high sensitivity (s P ~- 0.6mJy) polarimetric observations in seven...
The Australia Telescope 20-GHz (AT20G) Survey is a blind survey of the whole southern sky at 20 GHz ...
We present high sensitivity (~0.6 mJy) polarimetric observations in seven bands, from 2.1 to 38 GHz,...
The Australia Telescope 20-GHz (AT20G) Survey is a blind survey of the whole southern sky at 20 GHz ...
We present some first results on the variability, polarization and general properties of radio sourc...
The low-frequency polarisation properties of radio sources are poorly studied, particularly in stati...
Basu A, Schwarz D, Kloeckner H-R, et al. CMB foreground measurements through broad-band radio spectr...
Restricted Access. An open-access version is available at arXiv.org (one of the alternative location...
Restricted Access. An open-access version is available at arXiv.org (one of the alternative location...
We present polarization measurements at 8.4, 22, and 43 GHz made with the Very Large Array (VLA) of ...
We have observed 250 of the 258 southern sources in the complete 5 GHz 1 Jy sample by Kühr et al. (...
We present techniques developed to calibrate and correct Murchison Widefield Array low-frequency (72...