Table B.1
Compilation of z > 4 star-forming galaxies (i.e. excluding known QSO or AGN) with both [CII] and SFR (or IR luminosity) measurements (so excluding upper limits).
| Source name | Redshift | L[CII] | LIR | SFR | Ref | From LFIR to LIR | Lensing | Selection |
| [109 L⊙] | [1012 L⊙] | M⊙ yr-1 | Magnification | |||||
|
|
||||||||
| 4 <z< 5 | ||||||||
| SPT0418-47 | 4.224 | 65 ± 5 | 67.7 ± 4.32 | – | 1 | 1.08 ×L[42.5–500] | 32.7 ± 2.7 | DSFG |
| SPT0113-46 | 4.232 | 46 ± 10 | 22.68 ± 1.08 | – | 1 | 1.08 ×L[42.5–500] | 23.9 ± 0.5 | DSFG |
| ID141 | 4.243 | 61.6 ± 9.8 | 85 ± 3 | – | 2 | – | 10-30 | DSFG |
| ALMAJ081740.86+135138.2 | 4.260 | 3.02 |
1.00 |
3 | – | – | DLA | |
| SPT2311-54 | 4.281 | 24 ± 3 | 35.97 ± 3.27 | – | 1 | 1.09 ×L[42.5–500] | 1.9 ± 0.1 | DSFG |
| SPT0345-47 | 4.296 | 33 ± 4 | 100.28 ± 8.72 | – | 1 | 1.09 ×L[42.5–500] | 7.9 ± 0.5 | DSFG |
| SPT2103-60 | 4.435 | 71 ± 10 | 37.06 ± 2.18 | – | 1 | 1.09 ×L[42.5–500] | 27.8 ± 1.8 | DSFG |
| ALESS61.1 | 4.419 | 1.5 ± 0.3 | 2.1 ± 0.4 | – | 4 | – | – | DSFG |
| SMG1 | 4.424 | 8.3 ± 0.2 | 16 ± 3 | 5 | – | – | DSFG | |
| SMG2 | 4.429 | 2.9 ± 0.2 | 7.9 ± 0.3 | 5 | – | – | DSFG | |
| ALESS65.1 | 4.445 | 3.2 ± 0.4 | 2.0 ± 0.4 | – | 4 | – | – | DSFG |
| SPT0441-46 | 4.477 | 24 ± 6 | 40.33 ± 2.18 | – | 1 | 1.09 ×L[42.5–500] | 12.7 ± 1 | DSFG |
| SPT2146-55 | 4.567 | 22 ± 5 | 29.46 ± 3.27 | – | 1 | 1.09 ×L[42.5–500] | 6.6 ± 0.41 | DSFG |
| BR1202-0725N | 4.691 | 10.0 ± 1.5 | 12.86 ± 2.14 | – | 6 | 1.07 ×L[40–500] | – | DSFG |
| SPT2132-58 | 4.768 | 21 ± 4 | 33.96 ± 3.29 | – | 1 | 1.10 ×L[42.5–500] | 5.7 ± 0.5 | DSFG |
| 5 <z< 6 | ||||||||
| HZ8 | 5.148 | 0.26 |
– | 18 |
7 | – | – | UV |
| HDF850.1 | 5.185 | 11 ± 2.2 | 8.7 ± 1.0 | – | 8 | – | 1.6 ± 0.1 | DSFG |
| HLSJ091828.6+514223 | 5.243 | 85 ± 2 | 160 ± 10 | – | 9 | – | 8.9 ± 1.9 | DSFG |
| HZ7 | 5.250 | 0.32 |
– | 21 |
7 | – | – | UV |
| HZ6 | 5.290 | 1.41 |
0.081 |
49 |
7 | – | – | UV |
| SPT2319-55 | 5.293 | 14 ± 2 | 27.69 ± 2.22 | – | 1 | 1.11 ×L[42.5–500] | 13.9 ± 1.82 | DSFG |
| AzTEC-3 | 5.299 | 6.69 ± 0.23 | 17.34 |
– | 10 | 1.67 ×L[42.5–122.5] | – | DSFG |
| HZ4 | 5.540 | 0.95 |
0.135 |
51 |
7 | – | – | UV |
| HZ3 | 5.546 | 0.47 |
– | 18 |
7 | – | – | UV |
| HZ9 | 5.548 | 1.62 |
0.347 |
67 |
7 | – | – | UV |
| SPT0346-52 | 5.656 | 50 ± 7 | 137.5 ± 5.6 | – | 1 | 1.12 ×L[42.5–500] | 5.6 ± 0.1 | DSFG |
| HZ10 | 5.659 | 1.35 |
0.871 |
169 |
7 | – | – | UV |
| HZ2 | 5.670 | 0.36 |
– | 25 |
7 | – | – | UV |
| HZ1 | 5.690 | 0.25 |
– | 24 |
7 | – | – | UV |
| 6 <z< 7 | ||||||||
| ID52 | 6.018 | 0.40 ± 0.06 | – | 0.1 | 11 | – | – | Blind |
| ID09 | 6.024 | 0.30 ± 0.07 | – | 0.3 | 11 | – | – | Blind |
| A383-5.1 | 6.028 | 0.0083 | – | 3.2 | 12 | – | 11.4 | UV |
| ID49 | 6.051 | 0.24 ± 0.06 | – | 0.1 | 11 | – | – | Blind |
| SDSS J0842+1218 Comp | 6.066 | 1.87 ± 0.24 | 0.9 ± 0.3 | 140 ± 50 | 14 | – | – | Blind |
| WMH5 | 6.070 | 0.66 ± 0.07 | 0.200 ± 0.038 | 43 ± 5 | 15 | 1.60 ×L[42.5–122.5] | – | UV |
| CFHQ J2100-1715 Comp | 6.080 | 2.45 ± 0.42 | 5.4 ± 0.7 | 360 ± 70 | 14 | – | – | Blind |
| CLM1 | 6.166 | 0.24 ± 0.03 | 0.040 ± 0.024 | 37 ± 4 | 15 | 1.59 ×L[42.5–122.5] | – | UV |
| PSO J308-21 Comp EC | 6.249 | 0.66 ± 0.13 | 0.52 ± 0.17 | 77 ± 26 | 14 | – | – | Blind |
Notes. IR luminosities are computed by integrated the SED over rest-frame 8 to 1000 μm. The seventh column gives the multiplicative factors that were used to convert the quoted FIR luminosities (defined for a wavelength range given in brackets) to 8–1000 μm luminosities (based on Béthermin et al. (2015) effective SEDs). When applicable, the lensing magnifications are also given (all luminosities are uncorrected for lensing amplification).
Lensing for SPT sources are from Spilker et al. (2016).
Reference. (1) Gullberg et al. (2015); (2) Cox et al. (2011); (3) Neeleman et al. (2017); (4) Swinbank et al. (2012); (5) Oteo et al. (2016); (6) Wagg et al. (2012); (7) Capak et al. (2015); (8) Walter et al. (2012); (9) Rawle et al. (2014);(10) Riechers et al. (2014); (11) Aravena et al. (2016); (12) Knudsen et al. (2016); (13) Smit et al. (2017); (14) Decarli et al. (2017); (15) Willott et al. (2015); (16) Riechers et al. (2013); (17) Matthee et al. (2017); (18) Pentericci et al. (2016); (19) Bradač et al. (2017); (20) Strandet et al. (2017); (21) Knudsen et al. (2017).
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