Table 1.
Properties of the sample.
| SDSS name | Alias | RA | Dec. | z | Sample | RL | Host |
|---|---|---|---|---|---|---|---|
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) |
| J102906.69+555625.2 | J1029 | 10 29 06.69 | +55 56 25.25 | 0.4511 | D-env | – | – |
| J122844.81+501751.2 | J1228 | 12 28 44.82 | +50 17 51.24 | 0.2627 | D-env | 2.4 | D(3) |
| J123220.11+495721.8 | J1232 | 12 32 20.12 | +49 57 21.82 | 0.2625 | D-env | 0.1 | D(3) |
| J150916.18+613716.7 | J1509 | 15 09 16.17 | +61 37 16.80 | 0.2012 | SED | – | D(3) |
| J151020.06+554722.0 | J1510 | 15 10 20.05 | +55 47 22.11 | 0.1497 | SED | 0.5 | D,b(1) |
| J152205.41+393441.3 | J1522 | 15 22 05.50 | +39 34 40.45 | 0.0769 | SED | 1.7 | D,b,PB(1),merger |
| J164100.10+345452.7 | J1641 | 16 41 00.10 | +34 54 52.67 | 0.1640 | SED | 8.0 | D(2) |
Notes. Columns: (1) SDSS source name; (2) short name; (3) right ascension [hh mm ss.s] (J2000); (4) declination [dd mm ss.s] (J2000); (5) spectroscopic redshift; (6) sample of origin of the source. D-env: very dense Mpc-scale environment sample, SED: SED sample; (7) radio-loudness parameter (Kellermann et al. 1989); (8) host galaxy morphology, composed by: D = disk, b = bar, PB = pseudo-bulge ((1)Järvelä et al. 2018, (2)Olguín-Iglesias et al. 2020, and (3)Varglund et al. 2022).
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