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Table 3.

Core-D sources with VLBA observations from literature (see Sect. 3.4 for details) and the parameters derived.

Source St, 4300 MHz Sun, 4300 MHz St, 7600 MHz Sun, 7600 MHz αc/x, t αc/x, un Type Sep VLBI
[Jy] [Jy] [Jy] [Jy] [″] morph
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10)
J105922.02+523902.1( † ) 0.046 0.026 0.045 0.025 −0.04 −0.07 F 1.36 Core-jet
J110833.89+483202.9( † ) 0.018 0.016 0.017 0.016 −0.10 0.0 F 0.96 Core
J111300.30+494230.0 0.013 0.011 0.015 0.014 +0.25 +0.42 F/I 8.06 Core
J114312.36+505016.3( ⋆ )(†) 0.037 0.032 0.025 0.015 −0.69 −1.33 S 0.97 Core
J144841.08+465638.2 0.038 0.018 0.027 0.029 −0.60 +0.84 I 0.24 Core

Notes. Columns: 1 – Source; 2 – C-band total flux density integrated over entire map in Jy; 3 – C-band unresolved flux density at long VLBA baselines in Jy; 4 – X-band total flux density integrated over the entire map in Jy; 5 – X-band unresolved flux density at long VLBA baselines in Jy; 6 – spectral index estimated using total flux at C and X bands from columns 2 and 4; 7 – spectral index estimated using VLBI flux at C and X bands from columns 3 and 5; 8 – core spectrum type (F: flat spectrum, I: inverted spectrum, S: steep spectrum, I: inverted spectrum); 9 – angular separation between radio positions in the LoTSS DR2 catalog and RFC in arcsec; and 10 – VLBI morphology. The source names marked with ( † ) are the ones identified with broad lines in their SDSS spectra as discussed in Sect. 3.4, and ( ⋆ ) are the sources identified with USS in Sect. 3.3.

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