| Reference . | ν . | Telescope . | Resolution . | Sensitivity (5σ) . | N(Total) . | N(KSRs) . | Detection fraction . |
|---|---|---|---|---|---|---|---|
| . | (GHz) . | configuration . | (arcsec) . | (mJy) . | . | . | . |
| Thean et al. (2000) | 8.4 | VLA A | ∼0.25 | ∼0.28 | 60 | 4 | ∼6.7 per cent |
| Kukula et al. (1995) | 8.4 | VLA A | ∼0.25 | ∼0.35 | 18 | 0 | 0.0 per cent |
| Ulvestad & Wilson (1989) | 1.4 | VLA A/B | ∼2.0 | ∼0.40 | 57 | 13 | ∼23 per cent |
| Gallimore et al. (2006) | 5.0 | VLA D | ∼15–20 | ∼0.25 | 43 | 19 | ∼44 per cent |
| Our work | |||||||
| FIRST sample | 1.4 | VLA B | ∼5 | ∼1.0 | 2651 | 794 | ∼30.0 per cent |
| FIRST–NVSS sample | 1.4 | VLA D | ∼45 | ∼2.5 | 1737 | 738 | ∼42.3 per cent |
| Reference . | ν . | Telescope . | Resolution . | Sensitivity (5σ) . | N(Total) . | N(KSRs) . | Detection fraction . |
|---|---|---|---|---|---|---|---|
| . | (GHz) . | configuration . | (arcsec) . | (mJy) . | . | . | . |
| Thean et al. (2000) | 8.4 | VLA A | ∼0.25 | ∼0.28 | 60 | 4 | ∼6.7 per cent |
| Kukula et al. (1995) | 8.4 | VLA A | ∼0.25 | ∼0.35 | 18 | 0 | 0.0 per cent |
| Ulvestad & Wilson (1989) | 1.4 | VLA A/B | ∼2.0 | ∼0.40 | 57 | 13 | ∼23 per cent |
| Gallimore et al. (2006) | 5.0 | VLA D | ∼15–20 | ∼0.25 | 43 | 19 | ∼44 per cent |
| Our work | |||||||
| FIRST sample | 1.4 | VLA B | ∼5 | ∼1.0 | 2651 | 794 | ∼30.0 per cent |
| FIRST–NVSS sample | 1.4 | VLA D | ∼45 | ∼2.5 | 1737 | 738 | ∼42.3 per cent |
| Reference . | ν . | Telescope . | Resolution . | Sensitivity (5σ) . | N(Total) . | N(KSRs) . | Detection fraction . |
|---|---|---|---|---|---|---|---|
| . | (GHz) . | configuration . | (arcsec) . | (mJy) . | . | . | . |
| Thean et al. (2000) | 8.4 | VLA A | ∼0.25 | ∼0.28 | 60 | 4 | ∼6.7 per cent |
| Kukula et al. (1995) | 8.4 | VLA A | ∼0.25 | ∼0.35 | 18 | 0 | 0.0 per cent |
| Ulvestad & Wilson (1989) | 1.4 | VLA A/B | ∼2.0 | ∼0.40 | 57 | 13 | ∼23 per cent |
| Gallimore et al. (2006) | 5.0 | VLA D | ∼15–20 | ∼0.25 | 43 | 19 | ∼44 per cent |
| Our work | |||||||
| FIRST sample | 1.4 | VLA B | ∼5 | ∼1.0 | 2651 | 794 | ∼30.0 per cent |
| FIRST–NVSS sample | 1.4 | VLA D | ∼45 | ∼2.5 | 1737 | 738 | ∼42.3 per cent |
| Reference . | ν . | Telescope . | Resolution . | Sensitivity (5σ) . | N(Total) . | N(KSRs) . | Detection fraction . |
|---|---|---|---|---|---|---|---|
| . | (GHz) . | configuration . | (arcsec) . | (mJy) . | . | . | . |
| Thean et al. (2000) | 8.4 | VLA A | ∼0.25 | ∼0.28 | 60 | 4 | ∼6.7 per cent |
| Kukula et al. (1995) | 8.4 | VLA A | ∼0.25 | ∼0.35 | 18 | 0 | 0.0 per cent |
| Ulvestad & Wilson (1989) | 1.4 | VLA A/B | ∼2.0 | ∼0.40 | 57 | 13 | ∼23 per cent |
| Gallimore et al. (2006) | 5.0 | VLA D | ∼15–20 | ∼0.25 | 43 | 19 | ∼44 per cent |
| Our work | |||||||
| FIRST sample | 1.4 | VLA B | ∼5 | ∼1.0 | 2651 | 794 | ∼30.0 per cent |
| FIRST–NVSS sample | 1.4 | VLA D | ∼45 | ∼2.5 | 1737 | 738 | ∼42.3 per cent |
This PDF is available to Subscribers Only
View Article Abstract & Purchase OptionsFor full access to this pdf, sign in to an existing account, or purchase an annual subscription.
