Table 9.
Summary of the results.
| Source | Morphology | Components | Jets | Large-scale environment |
Notes |
|---|---|---|---|---|---|
| J091313.73+365817.2 | Spiral | PB, bar, disk | Intermediate | Enhanced SF | |
| J111934.01+533518.7 | Spiral | PB | Supercluster | Interacting, RL | |
| J122749.14+321458.9 | Unclear | Yes | Intermediate | Enhanced SF | |
| J123220.11+495721.8 | Unclear | Yes | Supercluster | ||
| J125635.89+500852.4 | Unclear | Yes | Intermediate | ||
| J133345.47+414127.7 | Unclear | Yes | Supercluster | Starburst | |
| J151020.06+554722.0 | Spiral | Bar, disk | Yes | Intermediate | |
| J152205.41+393441.3 | Spiral | PB, bar, disk | Yes | Void | Interacting |
| J161259.83+421940.3 | Spiral | PB, bar | Yes | Intermediate | Disturbed, starburst |
Notes. Column 1 gives the source name and Col. 2 the seeing during the observations. Column 3 lists the probable morphology of the host galaxy and Col. 4 gives the components of the model; PB denotes pseudo-bulge. In Col. 5 a source is marked if it has been detected at 37 GHz. The large-scale environment parameters in Col. 6 are from Järvelä et al. (2017). Column 7 gives additional notes of the source; SF denotes star formation.
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