Table 2
Characteristics of the observations of the CDFS field, covering 19 IFRS from our sample.
| Frequency | Telescope | Angular resolution | Sensitivity | # det | # undet | # outside | Reference |
| [MHz] | [arcsec2] | [μJy beam-1] | |||||
|
|
|||||||
| 150 | GMRT | 25.2 × 14.7 | 2000 | 12 | 7 | ... | (1) |
| 200 | MWA | 135 × 125 | 5900 | 10 | 9 | ... | (2) |
| 325 | GMRT | 11 × 7 | 100 | 18 | 1 | ... | (1) |
| 610 | GMRT | 7.7 × 3.7 | 100 | 10 | ... | 9 | (3) |
| 843 | MOST | 95 × 43 | 1700 | 8 | 9 | 2 | |
| 844 | ASKAP-BETA | 91 × 56 | 450 | 18 | 1 | ... | (4) |
| 1400 | ATCA | 16 × 7 | 14 | 19 | ... | ... | (5) |
| 2300 | ATCA | 57.15 × 22.68 | 70 | 19 | ... | ... | (6) |
| 4800 | ATCA | 4.6 × 1.7 | 100 | 5 | 3 | 11 | (7) |
| 5500 | ATCA | 4.9 × 2.0 | 12 | 2 | ... | 17 | (8) |
| 8640 | ATCA | 4.6 × 1.7 | 90 | 5 | 3 | 11 | (7) |
| 20 000 | ATCA | 29.1 × 21.9 | 40 | 2a | 10 | 7 | (9) |
| 34 000 | ATCA | 8.2 × 5.1 | 30 | 3 | ... | 16 | (10) |
Notes. Columns 5–7 list the number of detected IFRS, undetected IFRS, and IFRS outside the field, respectively.
These two IFRS were also detected in the follow-up observations by Franzen et al. (2014) at 5.5 GHz, 9 GHz, and 18 GHz.
Reference. (1) Based on the map from Sirothia et al. (in prep.); (2) Hurley-Walker et al. (2016); (3) based on the map from Intema et al. (in prep.); (4) based on the map from Marvil et al. (in prep.); (5) Franzen et al. (2015); (6) based on the map from Zinn et al. (2012); (7) Middelberg et al. (2011); (8) Huynh et al. (2012); (9) Franzen et al. (2014); (10) Emonts et al. (in prep.).
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