Table 4
Radio continuum properties extracted from the FIRST catalogue.
| Source | Dist. |
|
μ 1.4 L 1.4 | q |
|
|
||||
| [arcsec] | [mJy] | [1025 W Hz-1] | ||
|
|
||||
| PLCK_G045.1+61.1 | <0.135 | <3.2 | >2.4 | |
| PLCK_G080.2+49.8 | <0.135 | <1.8 | >2.4 | |
| PLCK_G092.5+42.9 | 0.9 | 1.50 ± 0.16 | 11.2 | 2.35 ± 0.11 |
| PLCK_G102.1+53.6 | <0.149 | <2.5 | >2.5 | |
| PLCK_G113.7+61.0 | 3.0 | 1.9 ± 0.14 | 6.9 | 2.2 ± 0.08 |
| PLCK_G138.6+62.0 | 2.7 | 2.01 ± 0.16 | 7.3 | 2.1 ± 0.08 |
| PLCK_G145.2+50.9 | <0.144 | <3.9 | >2.8 | |
| PLCK_G165.7+67.0 | 4.1 | 3.41 ± 0.15 | 10.1 | 2.0 ± 0.04 |
| PLCK_G200.6+46.1 | 1.1 | 1.23 ± 0.14 | 6.9 | 1.9 ± 0.11 |
| PLCK_G231.3+72.2 | <0.151 | <2.5 | >2.5 | |
| PLCK_G244.8+54.9 | 3.2 | 2.26 ± 0.14 | 13.6 | 2.3 ± 0.06 |
Notes. The columns are: source name; relative distance between the SPIRE position at 250 μm and the position of the FIRST counterpart, if detected within 5′′; integrated flux density at 1.4 GHz from the FIRST catalogue and gravitational magnification factor of the radio component, μ1.4; radio luminosity at 1.4 GHz in the rest-frame and gravitational magnification factor of that component, μ1.4, for sources without 1.4 GHz detections, the luminosities are derived from 3× the rms given in column 3; the Ratio between radio and FIR luminosity (see Sect. 8), i.e. the q-parameter.
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