Notes. Source S443 has been included here but is shown separately from the other sources to indicate that its detection does not imply the presence of an AGN. Column (1): ID we use in this paper; Col.  (2): the rms of the low-resolution image in mJy/beam; Cols.  (3), (4): the flux density extracted from the low-resolution image and its error in mJy; Cols.  (5), (6): the coordinates of the source in the low-resolution image; Cols.  (7), (8): the fraction of the ATCA flux density recovered in the low-resolution image and its error; Cols. (9), (10): the classification given by Norris et al. (2006) and based on the Szokoly et al. (2004) criteria; Col.  (11): a 1 here indicates that this source had not been previously known to contain an AGN; Col. (12): the value of q₂₄; Cols.  (13)–(15): the soft-band (0.5 keV to 2 keV) and hard-band (2 keV to 8 keV) X-ray counts listed by Luo et al. (2008) and Lehmer et al. (2005), and the derived hardness ratio; Cols.  (16), (17): the spectral index α listed by Kellermann et al. (2008), multiplied with −1 to convert to our convention of S ∝ ν^α, and its error; Cols.  (17), (18): the redshift and its reference: M08 – Mainieri et al. (2008); N06 – Norris et al. (2006); A06 – Afonso et al. (2006); Z04 – Zheng et al. (2004); W04 – Wolf et al. (2004); L04 – Le Fèvre et al. (2004).