Table 2
The 16 compact sources detected above 5σ at 154 MHz.
Name | ΔRA | ΔDec | S P−118 | S I−118 | S P−154 | S I−154 | |
[s] | [′′] | [mJy/beam] | [mJy] | [mJy/beam] | [mJy] | ||
|
|||||||
Uncatalogued | 46.300 | 39.66 | – | – | 0.76±0.16 | 0.94±0.26 | |
Uncatalogued | 46.415 | 64.90 | – | – | 0.74±0.14 | 0.49±0.27 | |
Uncatalogued | 47.644 | 42.17 | – | – | 0.85±0.19 | 1.02±0.30 | |
39.10+57.3abcd | 47.869 | 43.72 | – | – | 1.94±0.26 | 2.98±0.40 | |
39.64+53.4abcd | 48.389 | 39.61 | – | – | 1.42±0.23 | 2.30±0.36 | |
40.32+55.1abcd | 49.060 | 41.47 | 3.80±0.51 | 5.92±0.79 | 5.17±0.54 | 6.75±0.73 | |
Uncatalogued | 50.366 | 64.55 | – | – | 1.05±0.18 | 1.26±0.27 | |
Uncatalogued | 50.820 | 46.60 | 1.68±0.36 | 2.29±0.56 | 1.92±0.26 | 3.15±0.41 | |
42.53+61.9a | 51.258 | 48.12 | – | – | 1.43±0.23 | 3.72±0.44 | |
43.31+59.2abcd | 52.020 | 45.40 | – | – | 4.59±0.49 | 5.01±0.57 | |
45.42+67.4abcd | 54.126 | 53.54 | 10.88±1.15 | 17.02±1.91 | 11.91±1.21 | 15.98±1.63 | |
45.74+65.2abcd | 54.453 | 51.38 | 5.13±0.65 | 8.14±1.01 | 5.42±0.58 | 9.05±0.96 | |
46.52+63.9abcd | 55.208 | 49.99 | 1.70±0.37 | 1.88±0.60 | 2.33±0.30 | 3.08±0.43 | |
46.56+73.8abc | 55.254 | 59.87 | 5.75±0.68 | 7.97±0.98 | 6.76±0.70 | 8.61±0.91 | |
Uncatalogued | 55.824 | 55.68 | – | – | 1.05±0.20 | 1.26±0.31 | |
Uncatalogued | 57.017 | 58.75 | – | – | 1.30±0.20 | 1.78±0.30 |
Notes. Four additional possible extended sources are described in Sect. 4.4. Six of the compact sources listed below are detected also at 118 MHz. Fitted peak brightness values are given as SP and integrated flux densities are given as SI. Uncertainties on flux densities were calculated as i.e. including both a 10% calibration uncertainty and the uncertainty estimated from the fit, σfit. The right ascension and declination are given as offset from
and 69
(J2000). Sources with names (given traditionally as B1950-offset) were detected previously by or Objects not listed in these studies were marked as “Uncatalogued”. All uncatalogued objects except (46.42, 64.9) were clearly detected also by eMERLIN at 1.6 GHz. See Sect. 4.3 for further notes on source detection.
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