Table 1.
Observational parameters.
| Source | z | νobs | Δν | Beam | PA | σcont | σline | Notes/Refs | |
|---|---|---|---|---|---|---|---|---|---|
| (GHz) | (km s−1) | (″× ″) | (°) | (mJy beam−1) | (mJy beam−1) | ||||
| PKS 0159–11 | Q | 0.669 | 851.05 | 11.7 | 9.3 × 8.6 | 0.9 | 0.08 | 0.64 | 1,5 |
| PKS 0252–71 | G | 0.56443 ± 0.00003a | 907.02 | 11.0 | 13.3 × 6.3 | 144.1 | 0.14 | 1.74 | 2,3,5 |
| PKS 0403–13 | Q | 0.571 | 904.14 | 11.0 | 8.9 × 7.6 | 166.3 | 0.30 | 0.85 | 4,5 |
| PKS 0405–12 | Q | 0.574 | 902.41 | 11.0 | 9.3 × 8.3 | 40.2 | 0.37 | 0.68 | 5,4 |
| PKS 0637–75 | Q | 0.651 | 860.33 | 11.0 | 17.4 × 6.2 | 103.9 | 0.11 | 1.07 | 6 |
| PKS 0842–75 | Q | 0.524 | 932.02 | – | – | – | – | – | 6 (RFI) |
| PKS 0859–25 | G | 0.305 | 1088.43 | – | 7.8 × 6.0 | 171.1 | 0.17 | – | 5 (RFI) |
| PKS 1136–13 | Q | 0.544 | 914.03 | 10.9 | 9.6 × 7.2 | 150.9 | 0.35 | 0.91 | 5,7 |
| PKS 1151–34 | Q | 0.2579 ± 0.0001a | 1129.09 | 6.9 | 9.5 × 5.8 | 141.2 | 0.57 | 1.86 | 2,3,5 |
| PKS 1306–09 | G | 0.46692 ± 0.00007a | 970.22 | 10.2 | 12.2 × 6.9 | 159.7 | 0.60 | 1.14 | 2,3,5 |
| PKS 1355–41 | Q | 0.313 | 1081.80 | 14.5 | 9.8 × 6.2 | 132.2 | 0.08 | 0.66 | 6 |
| PKS 1510–08 | Q | 0.361 | 1043.64 | 7.5 | 10.5 × 6.7 | 131.3 | 0.09 | 0.69 | 5,8 |
| PKS 1602+01 | BLG | 0.462 | 971.55 | 10.2 | 11.5 × 8.3 | 116.4 | 0.10 | 0.97 | 5,9,10 |
| PKS 1954–388 | Q | 0.63 | 871.41 | 11.4 | 10.2 × 7.1 | 20.4 | 0.05 | 0.55 | 5 |
| PKS 2203–18 | Q | 0.618 | 877.87 | 11.3 | 9.2 × 7.5 | 170.2 | 0.24 | 1.19 | 5 |
| PKS 2243–123 | Q | 0.63 | 871.41 | 11.4 | 9.1 × 8.3 | 176.4 | 0.07 | 0.59 | 4,5,11 |
| PKS 2345–16 | Q | 0.576 | 901.27 | 11.0 | 10.1 × 8.1 | 48.1 | 0.14 | 0.77 | 4,5 |
Notes. The redshifts of most of the observed galaxies are taken from Tadhunter et al. (1993). (a)Redshifts are taken from Santoro et al. (2020) and are based on the measurement of the stellar absorption lines associated with the host galaxy starlight. Note that Santoro et al. (2020) did not correct the redshifts to heliocentric. For PKS 1151–34 this correction for the redshift is +0.000083, while for PKS 1306–09 it is +0.000096. The beam sizes are those of the continuum images. References: (1) Reid et al. (1999); (2) Tzioumis et al. (2002); (3) Santoro et al. (2020); (4) Cheng et al. (2020); (5) Morganti et al. (1993); (6) Burgess & Hunstead (2006); (7) Fernini (2014); (8) Lister et al. (2009); (9) Morganti et al. (1999); (10) Tadhunter et al. (2002); (11) Cheng et al. (2023)
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