1 Identification on basis of RRE position (Adgie, Crowther, Gent, private
 1 communication).
 2 Identification, or classification of field also by Wall et al.
 2 (1971AuJPS..19....1W).
 3 5-GHz flux density taken from Pauliny-Toth and Kellermann
 3 (1968AJ.....73..953P) and refers to two orthogonal planes of polarization.
 4 Published identification.
 5 Corresponds to 0038-020 in Parkes 2.7-GHz survey (Wall et al.,
 5 1971AuJPS..19....1W) and is identified with QSS.
 6 Partly resolved with 140-ft beam: quoted flux density is integrated or
 6 corrected for source size.
 7 Corresponds to two sources in Parkes 2.7-GHz survey (Wall et al.,
 7 1971AuJPS..19....1W) both identified with E galaxies.
 8 Identification by Olsen (1970AJ.....75..764O).
 9 Identification on basis of quoted position.
10 Identification by Blake (1970ApL.....6..201B).
11 Blake (1970ApL.....6..201B) finds neutral star at radio position. Possibly
11 QSS?
12 Classed as empty field by Wade and Miley (1971AJ.....76..101W).
13 5-GHz flux density from finding survey only, uncertainty +/-0.1f.u.
14 5-GHz flux density from measurements by Davis (private comm.).  A 300-ft
14 position quoted here refers to measurements at 1.4GHz by Davis (private
14 communication).
15 Position measured by Hoglund (1967ApJS...15...61H) quoted, since only a
15 finding survey position was available. Optical field confused by bright star.
16 Classed as empty field by Kristian and Sandage (1970ApJ...162..391K)