Table 1
Characteristics of the observations of the ELAIS-S1 field, covering 15 IFRS from our sample.
| Frequency | Telescope | Angular resolution | Sensitivity | # det | # undet | # outside | Reference |
| [MHz] | [arcsec2] | [μJy beam-1] | |||||
|
|
|||||||
| 200 | MWA | 140 × 125 | 7000 | 13 | 2 | ... | (1) |
| 610 | GMRT | 11 × 11 | 100 | 14 | ... | 1 | (2) |
| 843 | MOST | 62 × 43 | 600 | 15 | ... | ... | (3) |
| 1400 | ATCA | 12 × 8 | 17 | 15 | ... | ... | (4) |
| 2300 | ATCA | 33.56 × 19.90 | 70 | 15 | ... | ... | (5) |
| 4800 | ATCA | 4.6 × 1.7 | 130 | 5 | 1 | 9 | (6) |
| 8640 | ATCA | 4.6 × 1.7 | 130 | 3 | 3 | 9 | (6) |
| 34 000 | ATCA | 7 × 7 | 110 | 2 | 1 | 12 | (7) |
Notes. Columns 5–7 list the number of detected IFRS, undetected IFRS, and IFRS outside the field, respectively.
Reference. (1) Hurley-Walker et al. (2016); (2) based on the map from Intema et al. (in prep.); (3) based on the map from Randall et al. (2012); (4) Franzen et al. (2015); (5) based on the map from Zinn et al. (2012); (6) Middelberg et al. (2011); (7) Emonts et al. (in prep.).
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