Table 1
Sources observed, sorted by right ascension.
| Source name | RA (J2000) | Dec (J2000) | S74 (Jy) | Host type | Largest angular size (arcsec) |
|---|---|---|---|---|---|
| 3C 196 | 08:13:36.22 | +48:13:02.5 | 130.8 | Q(1) | 10(4) |
| 3C 225 | 09:42:15.30 | +13:45:49.3 | 32.5 | R(1) | 6(5) |
| 3C 273 | 12:29:05.89 | +02:02:55.7 | 161.7 | Q(2) | 22(6) |
| 3C 295 | 14:11:20.24 | +52:12:06.6 | 128.9 | R(1) | 4.7(7) |
| 3C 298 | 14:19:08.30 | +06:28:33.9 | 95.27 | Q(3) | 1.5(8) |
| 3C 380 | 18:29:32.49 | +48:44:57.5 | 124.7 | Q(1) | 20(4) |
Notes. Coordinates and 74 MHz flux densities were obtained from the VLA Low-Frequency Sky Survey Redux (Lane et al. 2014). The galaxy host types are from Laing et al. (1983) (1), where Q refers to a spectroscopically confirmed quasar and R to a non-quasar galaxy; Schmidt (1963) (2) and Rubin & Ford (1966) (3). The largest angular sizes are from Reid et al. (1995) at 966 MHz (4), Jenkins et al. (1977) at 5 GHz (5), Perley & Meisenheimer (2017) at 1.37 GHz (6), Akujor et al. (1994) at 1.6 GHz (7), and Akujor & Garrington (1995) at 1.6 GHz (8).
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.