Table 5.
Integrated AGN and SF luminosities.
| Name | Redshift |
 |
 |
SFR | LAS | size* | Stellar mass | Temp. |
 /  ** |
|---|---|---|---|---|---|---|---|---|---|
| (1012 L⊙) | (1012 L⊙)1 | (M⊙ yr−1) | (arcsec) | (kpc) | (log(M*/M⊙)) | (K) | |||
| MRC 0037−258 | 1.100 |
 |
< 2.17 | < 249 | 27.6a | 231.7 | 11.56g | uncons. | ... |
| MRC 0114−211 | 1.410 |
 |
 |
126 | < 2a | < 17 | 11.39g |
 |
0.47 |
| TN J0121+1320 | 3.516 | < 2.67 |
 |
626 | 0.3b | 2.2 | 11.02g |
 |
0.72 |
| MRC 0152−209 (H) | 1.920 |
 |
 |
1817 | 2.2c | 19.0 | 11.76g |
 |
0.89 |
| MRC 0152−209 (C) | 1.920 | ... |
 |
108 | ... | ... | ... |
 |
... |
| MRC 0156−252 | 2.016 |
 |
< 1.99 | < 228 | 8.3d | 71.2 | 12.05g | uncons. | ... |
| TN J0205+2242 | 3.506 | < 2.70 | < 0.74 | < 84 | 2.7b | 20.2 | 10.82g | uncons. | ... |
| MRC 0211−256 | 1.300 |
 |
 |
117 | 2.4a | 20.6 | < 11.54g |
 |
0.57 |
| TXS 0211−122 | 2.340 |
 |
 |
81 | 17.0d | 142.5 | < 11.16g |
 |
> 0.16 |
| MRC 0251−273 | 3.160 |
 |
 |
79 | 3.9a | 30.3 | 10.96g |
 |
> 0.11 |
| MRC 0324−228 | 1.894 |
 |
< 0.86 | < 98 | 9.6a | 81.1 | 10.7(8)f | uncons. | < 0.15 |
| MRC 0350−279 | 1.900 |
 |
< 0.77 | < 88 | 1.2a | 10.4 | < 11.00g | uncons. | ... |
| MRC 0406−244 | 2.427 |
 |
< 1.63 | < 186 | 10.0d | 83.2 | 11.1(3)f | uncons. | < 0.22 |
| PKS 0529−549 | 2.575 |
 |
 |
1018 | 3h | 24.7 | 11.46g |
 |
0.84 |
| TN J0924−2201 | 5.195 | < 14.98 |
 |
142 | 1.2b | 7.6 | 11.10g | uncons. | > 0.23 |
| MRC 0943−242 (H) | 2.923 |
 |
 |
41 | 3.9d | 31.0 | 11.3(4)f |
 |
0.03 |
| MRC 0943−242 (C) | 2.923 | ... |
 |
747 | ... | ... | ... |
 |
... |
| MRC 1017−220 | 1.768 |
 |
< 1.75 | < 201 | < 0.2c | < 1.7 | < 11.70g | uncons. | ... |
| 4C 03.24 | 3.570 |
 |
 |
142 | 6.0e | 44.7 | < 11.27g |
 |
0.26 |
| TN J1338+1942 | 4.110 |
 |
 |
461 | 5.2c | 36.6 | 11.04g |
 |
0.59 |
| TN J2007−1316 | 3.840 |
 |
 |
251 | 3.5b | 25.3 | 11.9(0)f |
 |
0.35 |
| MRC 2025−218 | 2.630 |
 |
< 0.36 | < 41 | 5.1d | 41.7 | < 11.62g | uncons. | ... |
| MRC 2048−272 | 2.060 | < 0.18 | < 0.65 | < 74 | 6.8c | 58.2 | 11.47g | uncons. | ... |
| MRC 2104−242 | 2.491 |
 |
< 0.38 | < 43 | 23.7c | 196.2 | 11.0(0.6)f | uncons. | < 0.07 |
| 4C 23.56 | 2.483 |
 |
< 0.49 | < 56 | 53.0d | 439.1 | < 11.59g | uncons. | ... |
| 4C 19.71 | 3.592 |
 |
 |
84 | 23.3d | 172.0 | < 11.13g |
 |
0.17 |
| MRC 2224−273 | 1.679 |
 |
 |
138 | < 0.2a | < 1.7 | 11.41g |
 |
0.55 |
Notes.
is the integrated AGN luminosity. 
is the integrated SF luminosity over the wavelengths 8–1000 μm in the rest-frame assuming β = 2.5 (Sect. 4.1). Upper-limits in 
were estimated assuming β = 2.5 and T = 50 K (Sect. 4.1). The star-formation rates, SFR, are calculated from the 
via the conversion given in Kennicutt (1998) but we scaled these values from the original Salpeter IMF assumed in Kennicutt (1998) to a Kroupa IMF by dividing by a factor of 1.5. LAS is the largest angular size of the radio source as given in the references indicated by the superscript:
( * )The physical size of radio source at 1.4 GHz (LAS) at the given redshift. The stellar masses are taken from the studies indicated by the superscript:
Drouart et al. (2016). Both of these studies use a Kroupa 2001 IMF. Some values of the stellar mass have two estimates. The value in the parentheses replaces the last digits to give the alternative value (see Sect. 4.5). For example, the possible stellar masses for MRC 2104−242 are log(M*/M⊙)=11.0 or 10.6.
( * *)The difference between the total luminosity of heated dust by star-formation, 
(this paper) and the total luminosity of dust heated by starbursts 
(Drouart et al. 2014). Two of sources contain additional sources in the ALMA images and for these two sources, we indicate the host galaxy and companions as “H” and “C”, respectively.
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