Table A.1.
Best-fit parameters of the spectral deconvolution.
| Target | zfit | E(B − V) | GP, fit | GS, fit | Star type | V* | |
|---|---|---|---|---|---|---|---|
| [km/s] | |||||||
| J0732+3533 | 3.0529 | 0.0698 | |||||
| J0812-0040 | 1.9147 | 0.0004 | 20.36 | 20.39 | G0 | +286 | |
| J0812+2007 | 1.4865 | 0.0358 | 20.16 | 21.46 | G2 | +57 | |
| J0927+33512 | 1.1605 | 0.0000 | |||||
| J0950+4329 | 1.7700 | 0.1389 | |||||
| J1048+4541 | 1.4432 | 0.0449 | |||||
| J1103+2348 | 1.4384 | 0.1003 | |||||
| J1318-0136 | 1.4881 | 0.1498 | |||||
| J1510+5959 | 2.0212 | 0.0039 | 20.34 | 20.99 | G3 | -210 | |
Notes. Best-fit parameters for the deconvolved sources. From left to right: Target ID, spectroscopic redshift (zfit), and extinction (E(B − V)) of the best-fitting QSO template. When an object is reproduced by an AGN plus a star, we report the G-band magnitude of the primary and secondary objects ((GP, fit) and GS, fit, respectively), the spectral type of the best-fitting star, and its radial velocity (V*).
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