Basic properties of the sample of radio galaxies. Columns are as follows. (1) Name of the active galaxy. (2) Active galaxy redshift. (3) Rest-frame wavelength, in the unit of 
m, corresponding to 1.1 mm in the observer frame. (4) and (5) are the RA and Dec. of the active galaxy. (6) The wavelength regime from which the position of the active galaxy was determined, where R = radio, I = mid-IR (3.6 and 4.5 
m), O = optical (R band) and K = near-IR (K band). (7) 1.1-mm flux density of the millimetre counterpart to the active galaxy. Errors in S1.1 are 1σ, and upper limits are 3σ. (8) The observed offset of the millimetre counterpart relative to the position of the active galaxy. In the absence of a probable counterpart we show in parentheses the offset to the closest millimetre detection. (9) P-statistic of the probable millimetre counterpart. Again, in the absence of a probable counterpart we show in parentheses the P-statistic of the nearest millimetre detection. (10) Log of the far-IR luminosity of millimetre counterparts. For non-detections, we give 3σ upper limits. (11) The star formation rate implied by the far-IR luminosity. Included at the bottom of the table is the radio-quiet quasar SDSS J1030+0524.
| Source name | z |  ( m) | RA (J2000) (hh:mm:ss.ss) | Dec. (J2000) (dd:mm:ss.s) | ID | S1.1 (mJy) | r (arcsec) | P | Log  | SFR (M⊙ yr−1) |
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) |
| MRC 2201−555 | 0.51 | 730 | 22:05:04.83 | −55:17:44.0 | I | 6.1±0.8 | 2.5 | 8×10−6 | 12.86 | 720 |
| MRC 2008−068 | 0.55 | 710 | 20:11:14.22 | −06:44:03.6 | R | 8.6±0.9 | 3.5 | 4×10−6 | 13.04 | 1100 |
| MRC 2322−052 | 1.19 | 500 | 23:25:19.62 | −04:57:36.6 | I | <2.1 | (20.7) | (0.049) | <12.60 | <400 |
| TXS 2322−040 | 1.51 | 440 | 23:25:10.23 | −03:44:46.7 | R | 2.3±0.6 | 2.3 | 0.0006 | 12.68 | 480 |
| MRC 2048−272 | 2.06 | 360 | 20:51:03.49 | −27:03:03.7 | I | 2.3±0.8 | 11.4 | 0.02 | 12.68 | 480 |
| MRC 0355−037 | 2.15 | 350 | 03:57:48.06 | −03:34:09.5 | I | 3.5±0.7 | 6.6 | 0.002 | 13.02 | 1040 |
| PKS 1138−262 | 2.16 | 350 | 11:40:48.35 | −26:29:08.6 | R | <3.6 | (14.3) | (0.007) | <12.85 | <710 |
| 4C +23.56 | 2.48 | 320 | 21:07:14.82 | +23:31:45.1 | R | <1.5 | (21.4) | (0.005) | <12.46 | <290 |
| MRC 2104−242 | 2.49 | 320 | 21:06:58.27 | −24:05:09.1 | R | 3.7±0.9 | 6.9 | 0.002 | 12.87 | 740 |
| PKS 0529−549 | 2.58 | 310 | 05:30:25.43 | −54:54:23.3 | I | 6.4±0.7 | 3.7 | 2×10−5 | 13.10 | 1270 |
| MRC 0316−257 | 3.13 | 270 | 03:18:12.14 | −25:35:10.2 | I | <2.1 | (17.3) | (0.009) | <12.55 | <350 |
| TN J2009−3040 | 3.16 | 260 | 20:09:48.08 | −30:40:07.4 | K | 3.3±0.9 | 12.9 | 0.005 | 12.79 | 610 |
| 4C +41.17 | 3.79 | 230 | 06:50:52.35 | +41:30:31.4 | O | 3.5±1.0 | 6.6 | 0.001 | 12.78 | 610 |
| TN J2007−1316 | 3.83 | 230 | 20:07:53.22 | −13:16:43.4 | R | 2.8±0.9 | 4.0 | 0.002 | 12.68 | 480 |
| TN J1338−1942 | 4.10 | 220 | 13:38:26.23 | −19:42:33.6 | R | <5.0 | (15.7) | (0.0008) | <12.90 | <790 |
| TN J0924−2201 | 5.19 | 180 | 09:24:19.91 | −22:01:41.5 | I | 3.6±0.9 | 13.9 | 0.006 | 12.74 | 560 |
| SDSS J1030+0524 | 6.28 | 150 | 10:30:27.10 | +05:24:55.0 | I | <1.4 | (22.7) | (0.02) | <12.30 | <200 |
| Source name | z | (m) | RA (J2000) (hh:mm:ss.ss) | Dec. (J2000) (dd:mm:ss.s) | ID | S1.1 (mJy) | r (arcsec) | P | Log | SFR (M⊙ yr−1) |
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) |
| MRC 2201−555 | 0.51 | 730 | 22:05:04.83 | −55:17:44.0 | I | 6.1±0.8 | 2.5 | 8×10−6 | 12.86 | 720 |
| MRC 2008−068 | 0.55 | 710 | 20:11:14.22 | −06:44:03.6 | R | 8.6±0.9 | 3.5 | 4×10−6 | 13.04 | 1100 |
| MRC 2322−052 | 1.19 | 500 | 23:25:19.62 | −04:57:36.6 | I | <2.1 | (20.7) | (0.049) | <12.60 | <400 |
| TXS 2322−040 | 1.51 | 440 | 23:25:10.23 | −03:44:46.7 | R | 2.3±0.6 | 2.3 | 0.0006 | 12.68 | 480 |
| MRC 2048−272 | 2.06 | 360 | 20:51:03.49 | −27:03:03.7 | I | 2.3±0.8 | 11.4 | 0.02 | 12.68 | 480 |
| MRC 0355−037 | 2.15 | 350 | 03:57:48.06 | −03:34:09.5 | I | 3.5±0.7 | 6.6 | 0.002 | 13.02 | 1040 |
| PKS 1138−262 | 2.16 | 350 | 11:40:48.35 | −26:29:08.6 | R | <3.6 | (14.3) | (0.007) | <12.85 | <710 |
| 4C +23.56 | 2.48 | 320 | 21:07:14.82 | +23:31:45.1 | R | <1.5 | (21.4) | (0.005) | <12.46 | <290 |
| MRC 2104−242 | 2.49 | 320 | 21:06:58.27 | −24:05:09.1 | R | 3.7±0.9 | 6.9 | 0.002 | 12.87 | 740 |
| PKS 0529−549 | 2.58 | 310 | 05:30:25.43 | −54:54:23.3 | I | 6.4±0.7 | 3.7 | 2×10−5 | 13.10 | 1270 |
| MRC 0316−257 | 3.13 | 270 | 03:18:12.14 | −25:35:10.2 | I | <2.1 | (17.3) | (0.009) | <12.55 | <350 |
| TN J2009−3040 | 3.16 | 260 | 20:09:48.08 | −30:40:07.4 | K | 3.3±0.9 | 12.9 | 0.005 | 12.79 | 610 |
| 4C +41.17 | 3.79 | 230 | 06:50:52.35 | +41:30:31.4 | O | 3.5±1.0 | 6.6 | 0.001 | 12.78 | 610 |
| TN J2007−1316 | 3.83 | 230 | 20:07:53.22 | −13:16:43.4 | R | 2.8±0.9 | 4.0 | 0.002 | 12.68 | 480 |
| TN J1338−1942 | 4.10 | 220 | 13:38:26.23 | −19:42:33.6 | R | <5.0 | (15.7) | (0.0008) | <12.90 | <790 |
| TN J0924−2201 | 5.19 | 180 | 09:24:19.91 | −22:01:41.5 | I | 3.6±0.9 | 13.9 | 0.006 | 12.74 | 560 |
| SDSS J1030+0524 | 6.28 | 150 | 10:30:27.10 | +05:24:55.0 | I | <1.4 | (22.7) | (0.02) | <12.30 | <200 |
Basic properties of the sample of radio galaxies. Columns are as follows. (1) Name of the active galaxy. (2) Active galaxy redshift. (3) Rest-frame wavelength, in the unit of m, corresponding to 1.1 mm in the observer frame. (4) and (5) are the RA and Dec. of the active galaxy. (6) The wavelength regime from which the position of the active galaxy was determined, where R = radio, I = mid-IR (3.6 and 4.5 m), O = optical (R band) and K = near-IR (K band). (7) 1.1-mm flux density of the millimetre counterpart to the active galaxy. Errors in S1.1 are 1σ, and upper limits are 3σ. (8) The observed offset of the millimetre counterpart relative to the position of the active galaxy. In the absence of a probable counterpart we show in parentheses the offset to the closest millimetre detection. (9) P-statistic of the probable millimetre counterpart. Again, in the absence of a probable counterpart we show in parentheses the P-statistic of the nearest millimetre detection. (10) Log of the far-IR luminosity of millimetre counterparts. For non-detections, we give 3σ upper limits. (11) The star formation rate implied by the far-IR luminosity. Included at the bottom of the table is the radio-quiet quasar SDSS J1030+0524.
| Source name | z | (m) | RA (J2000) (hh:mm:ss.ss) | Dec. (J2000) (dd:mm:ss.s) | ID | S1.1 (mJy) | r (arcsec) | P | Log | SFR (M⊙ yr−1) |
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) |
| MRC 2201−555 | 0.51 | 730 | 22:05:04.83 | −55:17:44.0 | I | 6.1±0.8 | 2.5 | 8×10−6 | 12.86 | 720 |
| MRC 2008−068 | 0.55 | 710 | 20:11:14.22 | −06:44:03.6 | R | 8.6±0.9 | 3.5 | 4×10−6 | 13.04 | 1100 |
| MRC 2322−052 | 1.19 | 500 | 23:25:19.62 | −04:57:36.6 | I | <2.1 | (20.7) | (0.049) | <12.60 | <400 |
| TXS 2322−040 | 1.51 | 440 | 23:25:10.23 | −03:44:46.7 | R | 2.3±0.6 | 2.3 | 0.0006 | 12.68 | 480 |
| MRC 2048−272 | 2.06 | 360 | 20:51:03.49 | −27:03:03.7 | I | 2.3±0.8 | 11.4 | 0.02 | 12.68 | 480 |
| MRC 0355−037 | 2.15 | 350 | 03:57:48.06 | −03:34:09.5 | I | 3.5±0.7 | 6.6 | 0.002 | 13.02 | 1040 |
| PKS 1138−262 | 2.16 | 350 | 11:40:48.35 | −26:29:08.6 | R | <3.6 | (14.3) | (0.007) | <12.85 | <710 |
| 4C +23.56 | 2.48 | 320 | 21:07:14.82 | +23:31:45.1 | R | <1.5 | (21.4) | (0.005) | <12.46 | <290 |
| MRC 2104−242 | 2.49 | 320 | 21:06:58.27 | −24:05:09.1 | R | 3.7±0.9 | 6.9 | 0.002 | 12.87 | 740 |
| PKS 0529−549 | 2.58 | 310 | 05:30:25.43 | −54:54:23.3 | I | 6.4±0.7 | 3.7 | 2×10−5 | 13.10 | 1270 |
| MRC 0316−257 | 3.13 | 270 | 03:18:12.14 | −25:35:10.2 | I | <2.1 | (17.3) | (0.009) | <12.55 | <350 |
| TN J2009−3040 | 3.16 | 260 | 20:09:48.08 | −30:40:07.4 | K | 3.3±0.9 | 12.9 | 0.005 | 12.79 | 610 |
| 4C +41.17 | 3.79 | 230 | 06:50:52.35 | +41:30:31.4 | O | 3.5±1.0 | 6.6 | 0.001 | 12.78 | 610 |
| TN J2007−1316 | 3.83 | 230 | 20:07:53.22 | −13:16:43.4 | R | 2.8±0.9 | 4.0 | 0.002 | 12.68 | 480 |
| TN J1338−1942 | 4.10 | 220 | 13:38:26.23 | −19:42:33.6 | R | <5.0 | (15.7) | (0.0008) | <12.90 | <790 |
| TN J0924−2201 | 5.19 | 180 | 09:24:19.91 | −22:01:41.5 | I | 3.6±0.9 | 13.9 | 0.006 | 12.74 | 560 |
| SDSS J1030+0524 | 6.28 | 150 | 10:30:27.10 | +05:24:55.0 | I | <1.4 | (22.7) | (0.02) | <12.30 | <200 |
| Source name | z | (m) | RA (J2000) (hh:mm:ss.ss) | Dec. (J2000) (dd:mm:ss.s) | ID | S1.1 (mJy) | r (arcsec) | P | Log | SFR (M⊙ yr−1) |
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) |
| MRC 2201−555 | 0.51 | 730 | 22:05:04.83 | −55:17:44.0 | I | 6.1±0.8 | 2.5 | 8×10−6 | 12.86 | 720 |
| MRC 2008−068 | 0.55 | 710 | 20:11:14.22 | −06:44:03.6 | R | 8.6±0.9 | 3.5 | 4×10−6 | 13.04 | 1100 |
| MRC 2322−052 | 1.19 | 500 | 23:25:19.62 | −04:57:36.6 | I | <2.1 | (20.7) | (0.049) | <12.60 | <400 |
| TXS 2322−040 | 1.51 | 440 | 23:25:10.23 | −03:44:46.7 | R | 2.3±0.6 | 2.3 | 0.0006 | 12.68 | 480 |
| MRC 2048−272 | 2.06 | 360 | 20:51:03.49 | −27:03:03.7 | I | 2.3±0.8 | 11.4 | 0.02 | 12.68 | 480 |
| MRC 0355−037 | 2.15 | 350 | 03:57:48.06 | −03:34:09.5 | I | 3.5±0.7 | 6.6 | 0.002 | 13.02 | 1040 |
| PKS 1138−262 | 2.16 | 350 | 11:40:48.35 | −26:29:08.6 | R | <3.6 | (14.3) | (0.007) | <12.85 | <710 |
| 4C +23.56 | 2.48 | 320 | 21:07:14.82 | +23:31:45.1 | R | <1.5 | (21.4) | (0.005) | <12.46 | <290 |
| MRC 2104−242 | 2.49 | 320 | 21:06:58.27 | −24:05:09.1 | R | 3.7±0.9 | 6.9 | 0.002 | 12.87 | 740 |
| PKS 0529−549 | 2.58 | 310 | 05:30:25.43 | −54:54:23.3 | I | 6.4±0.7 | 3.7 | 2×10−5 | 13.10 | 1270 |
| MRC 0316−257 | 3.13 | 270 | 03:18:12.14 | −25:35:10.2 | I | <2.1 | (17.3) | (0.009) | <12.55 | <350 |
| TN J2009−3040 | 3.16 | 260 | 20:09:48.08 | −30:40:07.4 | K | 3.3±0.9 | 12.9 | 0.005 | 12.79 | 610 |
| 4C +41.17 | 3.79 | 230 | 06:50:52.35 | +41:30:31.4 | O | 3.5±1.0 | 6.6 | 0.001 | 12.78 | 610 |
| TN J2007−1316 | 3.83 | 230 | 20:07:53.22 | −13:16:43.4 | R | 2.8±0.9 | 4.0 | 0.002 | 12.68 | 480 |
| TN J1338−1942 | 4.10 | 220 | 13:38:26.23 | −19:42:33.6 | R | <5.0 | (15.7) | (0.0008) | <12.90 | <790 |
| TN J0924−2201 | 5.19 | 180 | 09:24:19.91 | −22:01:41.5 | I | 3.6±0.9 | 13.9 | 0.006 | 12.74 | 560 |
| SDSS J1030+0524 | 6.28 | 150 | 10:30:27.10 | +05:24:55.0 | I | <1.4 | (22.7) | (0.02) | <12.30 | <200 |
