Table 7.
CLASC source comparison with cross-matched SBHW catalogue sources from Setia Gunawan et al. (2003).
| CLASC | SBHW | |||||
|---|---|---|---|---|---|---|
| ID |
 |
 |
ID | S21 cm | S86 cm | α |
| mJy | mJy | mJy | mJy | |||
| 11 | 1.90 ± 0.24 | 4.35 ± 0.44 | 81 | 3.6 ± 0.5 | – | – |
| 12 | 1.78 ± 0.72 | 6.31 ± 0.48 | 83 | 8.4 ± 0.5 | 62 ± 3 | −1.60 |
| 22 | 13.5 ± 1.37 | 15.9 ± 1.6 | 90 | 14.7 ± 0.8 | 54 ± 4 | −0.89 |
| 47 | 0.32 ± 0.08 | 3.69 ± 0.17 | 109 | 3.0 ± 0.6 | – | – |
| 50 | 3.86 ± 0.42 | 3.83 ± 0.39 | 110 | 2.2 ± 0.2 | – | – |
| 52 | 2.43 ± 0.28 | 3.18 ± 0.33 | 112 | 2.2 ± 0.3 | – | > 0.37 |
Notes. Where sources have been detected with multiple components (11, 12, and 47), a combined flux density is included. The spectral index is that calculated between the S86 cm flux density and the COBRaS April 26 S21 cm flux density, except for CLASC #52 which lists the upper limit from Setia Gunawan et al. (2003).
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