Table 1.
Number of sources in the chosen sample within log LIR or logSFR bins.
| Bin | H-ATLAS sample |
SFG 5σ subsample |
SFG 3σ subsample |
||||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| log LIR | Total | Detections | In 5σ stack | In 3σ stack | FIRST subsample | NVSS subsample | FIRST subsample | NVSS subsample | |||||||
| FIRST | NVSS | FIRST | NVSS | FIRST | NVSS | Total (detections) | In stack | Total (detections) | In stack | Total (detections) | In stack | Total (detections) | In stack | ||
| ⟨7.5, 8.0] | 6 | 0 | 0 | N | N | N | N | 4 (0) | N | 0 (0) | N | 4 (0) | N | 0 (0) | N |
| ⟨8.0, 8.5] | 16 | 0 | 0 | N | N | N | Y | 8 (0) | N | 2 (0) | N | 8 (0) | N | 2 (0) | N |
| ⟨8.5, 8.8] | 27 | 0 | 1 | N | N | N | N | 17 (0) | N | 8 (1) | N | 17 (0) | Y | 8 (1) | N |
| ⟨8.8, 9.0] | 37 | 1 | 1 | N | N | N | N | 24 (1) | Y | 5 (1) | N | 24 (1) | Y | 5 (1) | N |
| ⟨9.0, 9.2] | 54 | 1 | 0 | N | N | N | Y | 33 (0) | N | 5 (0) | N | 34 (0) | N | 5 (0) | N |
| ⟨9.2, 9.4] | 111 | 0 | 0 | N | Y | Y | Y | 69 (0) | Y | 13 (0) | Y | 69 (0) | Y | 13 (0) | Y |
| ⟨9.4, 9.6] | 189 | 1 | 4 | N | Y | Y | Y | 101 (1) | N | 24 (2) | N | 101 (1) | Y | 24 (2) | Y |
| ⟨9.6, 9.8] | 280 | 1 | 2 | N | N | Y | Y | 155 (1) | Y | 28 (1) | N | 155 (1) | Y | 28 (1) | Y |
| ⟨9.8, 9.9] | 219 | 0 | 3 | N | N | Y | N | 103 (0) | Y | 12 (1) | N | 103 (0) | Y | 12 (1) | Y |
| ⟨9.9, 10.0] | 267 | 0 | 1 | N | Y | Y | Y | 150 (0) | Y | 25 (1) | N | 150 (0) | Y | 26 (1) | Y |
| ⟨10.0, 10.1] | 291 | 3 | 4 | Y | Y | Y | Y | 166 (2) | Y | 18 (1) | Y | 167 (2) | Y | 21 (2) | Y |
| ⟨10.1, 10.2] | 295 | 3 | 9 | Y | Y | Y | Y | 193 (2) | Y | 30 (4) | Y | 194 (2) | Y | 35 (6) | Y |
| ⟨10.2, 10.3] | 317 | 5 | 7 | Y | Y | Y | Y | 238 (5) | Y | 26 (6) | Y | 238 (5) | Y | 28 (6) | Y |
| ⟨10.3, 10.4] | 317 | 9 | 12 | Y | Y | Y | Y | 264 (9) | Y | 44 (11) | Y | 264 (9) | Y | 45 (11) | Y |
| ⟨10.4, 10.5] | 256 | 5 | 6 | Y | Y | Y | Y | 226 (5) | Y | 40 (1) | Y | 226 (5) | Y | 42 (1) | Y |
| ⟨10.5, 11.5] | 628 | 53 | 79 | Y | Y | Y | Y | 599 (53) | Y | 257 (65) | Y | 595 (51) | Y | 262 (64) | Y |
| ⟨11.5, 12.0] | 15 | 2 | 9 | Y | Y | Y | Y | 15 (2) | Y | 13 (9) | Y | 15 (2) | Y | 14 (9) | Y |
| ⟨12.0, 13.0] | 3 | 0 | 0 | N | N | N | N | 3 (0) | N | 3 (0) | N | 3 (0) | N | 3 (0) | N |
| Total | 3328 | 84 | 138 | 7 | 10 | 12 | 13 | 2368 ( 81) | 12 | 553 (104) | 8 | 2367 ( 79) | 14 | 573 (106) | 12 |
| logSFR | |||||||||||||||
| ⟨ − 3.7, −2.5] | 22 | 1 | 0 | N | N | N | Y | 0 (0) | N | 0 (0) | N | 0 (0) | N | 0 (0) | N |
| ⟨ − 2.5, −2.0] | 33 | 1 | 1 | N | N | N | N | 2 (0) | N | 0 (0) | N | 2 (0) | N | 0 (0) | N |
| ⟨ − 2.0, −1.5] | 45 | 0 | 1 | N | Y | N | Y | 4 (0) | N | 0 (0) | N | 5 (0) | N | 0 (0) | N |
| ⟨ − 1.5, −1.0] | 108 | 0 | 3 | Y | N | Y | N | 22 (0) | N | 8 (0) | N | 23 (0) | Y | 10 (1) | N |
| ⟨ − 1.0, −0.6] | 191 | 1 | 2 | Y | Y | Y | Y | 70 (1) | Y | 11 (2) | Y | 71 (1) | Y | 11 (2) | Y |
| ⟨ − 0.6, −0.2] | 478 | 5 | 7 | Y | Y | Y | Y | 224 (5) | Y | 38 (3) | Y | 225 (5) | Y | 42 (4) | Y |
| ⟨ − 0.2, −0.1] | 252 | 2 | 4 | Y | Y | Y | Y | 149 (2) | Y | 24 (2) | Y | 149 (2) | Y | 26 (2) | Y |
| ⟨ − 0.1, 0.1] | 524 | 0 | 6 | Y | Y | Y | Y | 303 (0) | Y | 42 (3) | Y | 303 (0) | Y | 44 (4) | Y |
| ⟨0.1, 0.2] | 303 | 5 | 6 | Y | Y | Y | Y | 243 (4) | Y | 35 (5) | Y | 242 (4) | Y | 35 (5) | Y |
| ⟨0.2, 0.3] | 353 | 9 | 9 | Y | Y | Y | Y | 339 (9) | Y | 40 (6) | Y | 339 (9) | Y | 42 (6) | Y |
| ⟨0.3, 0.4] | 245 | 6 | 9 | Y | Y | Y | Y | 242 (6) | Y | 40 (6) | Y | 240 (5) | Y | 44 (6) | Y |
| ⟨0.4, 0.6] | 406 | 18 | 24 | Y | Y | Y | Y | 403 (18) | Y | 81 (16) | Y | 402 (17) | Y | 83 (16) | Y |
| ⟨0.6, 2.5] | 368 | 36 | 66 | Y | Y | Y | Y | 367 (36) | Y | 234 (61) | Y | 366 (36) | Y | 236 (60) | Y |
| Total | 3328 | 84 | 138 | 10 | 10 | 10 | 11 | 2368 ( 81) | 9 | 553 (104) | 9 | 2367 ( 79) | 10 | 573 (106) | 9 |
Notes. The numbers in parentheses indicate sources individually detected by the FIRST and NVSS surveys. The SFG subsamples contain sources satisfying the Smolčić et al. (2017) criterion applied using FIRST and NVSS derived radio luminosities or their 5σ or 3σ upper limits. The ‘Total’ columns show the total number of sources in each (sub)sample, the ‘in stack’ columns show whether a particular bin was processed as a detection (Y) or an upper limit (N) in a particular radio map, out to the detection limit of either 5 or 3σ. In the ‘Total’ rows, the number of Ys is shown for the appropriate columns.
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