We present the first results of a project called SAGAN, which is dedicated solely to the
studies of relatively rare megaparsec-scale radio galaxies in the Universe, called giant radio …

A subsample of the Wall & Peacock 2-Jy sample of radio sources, with redshift z< 0.7 or
unknown and declination δ<+ 10°, has been selected and observed in the radio at 6 cm (or …

We have made a sensitive radio continuum survey of 114 nearby E and S0 galaxies to
search for weak sources. The radio detection rate is 42 per cent, with a flux limit of 0.8 mJy at …

Active galactic nuclei (AGNs) with jets seen at small viewing angles are the most luminous
and abundant objects in the γ-ray sky. AGNs with jets misaligned along the line of sight …

The Fermi gamma-ray satellite has recently detected gamma-ray emissions from radio
galaxy cores. From these samples, we first examine the correlation between the luminosities …

We have imaged with milliarcsecond resolution at 5 GHz 374 strong flat-spectrum radio
sources north of declination-44 using the VLBA in 1996 June. The source sample was …

This is the first paper of a series exploring the multifrequency properties of a sample of 11
nearby low-excitation radio galaxies (LERGs) in the southern sky. We are conducting an …

Unlike blazars, radio galaxies have jets that are misaligned relative to our line-of-sight. This
misaligned geometry provides us with a unique view of both the jet and super massive black …

We present radio images with the Australia Telescope of a sample of powerful radio
galaxies. The observations were designed to be sensitive to the largest-scale structures in …

Abstract We find compact (< 0.03 arcsec) radio-continuum cores in about 70 per cent of
radio-emitting elliptical and S0 galaxies over a wide range in total radio power (1021–1026 …