Table C.1.
PSS-CSO sample. Only the first six rows of the table are shown here for illustration. Uncertain data are indicated by a colon. The full list is available in electronic form from the VizieR Service of the CDS Strasbourg.
| SDSS name | RA | DEC | z | Ri | Type | SDSS class | log Lr | log LLS | f_L | |
|---|---|---|---|---|---|---|---|---|---|---|
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | |
| 1 | J002225.42+001456.1 | 5.60592 | 0.24892 | 0.306 | 4.20 | GPS | GAL | 26.9 | −0.57 | - |
| 2 | J002833.42+005510.9 | 7.13925 | 0.91969 | 0.104 | 2.52 | CSS | GAL | 24.8 | 0.53 | - |
| 3 | J002914.24+345632.2 | 7.30933 | 34.94228 | 0.517 | 4.41 | CSO | GAL | 27.2 | −0.70 | - |
| 4 | J005905.51+000651.6 | 14.77296 | 0.11433 | 0.719 | 3.84 | CSS | QSO | 27.7 | - | - |
| 5 | J014109.16+135328.3 | 25.28817 | 13.89119 | 0.621 | 4.54 | CSS | QSO | 27.6 | 0.80 | - |
| 6 | J074417.47+375317.2 | 116.07279 | 37.88811 | 1.066 | 3.65 | CSS | QSO | 27.8 | 1.25 | - |
| tWHAN | tSED | tWISE | D4000n | e_D4000n | log SFR | log ℳ* | f_S | tm | SDSS name of ECS | |
| (11) | (12) | (13) | (14) | (15) | (16) | (17) | (18) | (19) | (20) | |
| 1 | wAGN | 3 | inter | 1.686 | 0.783 | - | - | - | - | J005727.88+020934.5 |
| 2 | sAGN | 2 | inter | 1.259 | 0.012 | 0.317 | 10.5 | 1 | 3.00 | J155700.17+413111.1 |
| 3 | - | 5 | inter | 1.518 | 1.418 | - | - | - | - | J113852.21+501602.3 |
| 4 | - | 6 | QSO | - - | - | - | - | - | - | J142456.92+200026.3 |
| 5 | - | 4 | QSO | - - | - | - | - | - | - | J121427.42+595814.8 |
| 6 | - | 6 | QSO | - - | - | - | - | - | - | J093033.53+360125.1 |
Notes. (1) SDSS name; (2) - (3) right ascension and declination (degrees); (4) redshift; (5) radio loudness parameter (Sect. 2); (6) radio type from Liao & Gu (2020); (7) SDSS spectral class; (8) 1.4 GHz radio luminosity (W Hz−1); (9)-(10) largest linear size (kpc) and upper limit flag from Liao & Gu (2020); (11) type based on WHAN diagram; (12) spectral type from MBSED (Table 4); (13) type based on WISE W1 − W2 vs. W2 − W3 diagram (Fig. 12); (14) - (15) 4000 Å break index and uncertainty; (16) - (18) SFR (ℳ⊙ yr−1), stellar mass (ℳ⊙) and uncertainty flag from Chang et al. (2015); (19) merger index based on images from the DESI Legacy Surveys; (20) counterpart in the ECS sample.
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