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Our current understanding of radio-loud AGN comes predominantly from studies at frequencies of 5 GHz and below. With the recent completion of the Australia Telescope 20 GHz (AT20G) survey, we can now ...
We have analyzed the properties of the Na D doublet lines in a large sample of 691 radio galaxies using the Sloan Digital Sky Survey (SDSS). These radio galaxies are resolved in the FIRST survey, have...
VLA radio continuum observations of WR ring nebulae。
Radio Continuum and H I Observations of the Remarkable Planetary Nebula KJPN 8
We have made observations of the associated HI absorption of a high redshift radio galaxy 0902C34 at z D 3:395 with the Giant Meterwave Radio Telescope in the 3231MHz band.We find a narrowabsorptio...
We present the 100 strongest 1.4 GHz point sources from a new mosaic image in the direction of the Large Magellanic Cloud (LMC). The observations making up the mosaic were made using Australia Telesco...

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