5 Notes on individual sources

Apart from the information in Table 5 we note that:

• 0627+532, 0652+577, 1107+485, 1256+546 and 1311+552 are 6C sources (Hales et al. 1993 and references therein).
• 1107+485 is a member of the DRAO 408 MHz survey (Green & Riley 1995).
• 1745+670 and 1753+648 are members of the NEP survey (Kollgaard et al. 1994).
• 1607+563, 1755+578 and 1815+614 are members of the 7C survey (Visser et al. 1995).
• 0514+474 was observed by Leahy & Roger (1996).
• 0102+480 and 2253+417 are members of the CJ1 survey (Polatidis et al. 1995).
• 1245+676 is a giant radio galaxy with a GPS core (O'Dea priv. comm. 1996).
• 0140+490 has a large scale symmetric structure $2\hbox{$.\mkern-4mu^\prime$}5$ across.
• 1839+548 and 2119+709 are marked as "quasi-point" sources in JVAS. All other sources are pointlike i.e. they are unresolved by the VLA in "A" configuration at 8.4 GHz.
• 1815+614 and 1946+708 are CSOs (Taylor et al. 1996; Taylor & Vermeulen 1997).