Table 3.
Information about the SINFONI maps.
| ID | H-band PSF | K-band PSF | z[O III] | F([O III])/F(Hβ) | F([N II])/F(Hα) | Re([O III]) | Re(Hα) | Line |
|---|---|---|---|---|---|---|---|---|
| [arcsec2] | [arcsec2] | [kpc] | [kpc] | components | ||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) |
| X_N_81_44 | 0.27 × 0.27 | 0.24 × 0.24 | 2.3180 | > 8.00 | < 0.10 | < 1.11 | 3.48 ± 0.08 | n, b, BLR |
| XID36 | 0.35 × 0.35 | 0.15 × 0.15 | 2.2578 | 10.15 ± 0.63 | 0.69 ± 0.12 | 1.06 ± 0.01 | 1.57 ± 0.01 | n, b |
| XID419 | 0.52 × 0.47 | 0.24 × 0.22 | 2.1430 | > 2.15 | 0.91 ± 0.05 | < 2.07 | 1.42 ± 0.02 | n |
| cid_1057 | 0.32 × 0.30 | 0.46 × 0.43 | 2.2099 | 2.51 ± 0.17 | – | 1.36 ± 0.01 | – | n, b |
| cid_346 | 0.30 × 0.30 | 0.30 × 0.30 | 2.2170 | 1.58 ± 0.20 | 0.43 ± 0.11 | 1.99 ± 0.03 | 2.28 ± 0.05 | n, b, BLR |
| cid_451 | 0.30 × 0.28 | 0.28 × 0.27 | 2.4434 | > 10.59 | 0.61 ± 0.03 | 0.78 ± 0.00 | 0.67 ± 0.01 | n, b |
| cid_1205 | 0.30 × 0.30 | 0.30 × 0.30 | 2.2555 | > 1.66 | – | 0.99 ± 0.02 | 1.33 ± 0.09 | n, BLR |
| cid_1143 | 0.41 × 0.38 | 0.30 × 0.30 | 2.4418 | 6.91 ± 1.97 | 0.75 ± 0.09 | < 1.62 | 0.92 ± 0.02 | n, b |
Notes. PSF of the H and K-band SINFONI images and line fluxes measured from the integrated spectra. If the S/N of a line is smaller than 3, we report a 5σ upper limit. For cid_1057, the S/N of the K-band image is too low to derive any information about the Hα and [N II] emission. (4) Redshift derived from the narrow component of the [O III] line. (5) Ratio of the fluxes of [O III]λ5007 and Hβ narrow emission lines. For Type 1 AGN, this is the flux of the narrow component, i.e. the BLR component is not included. (6) Ratio of the fluxes of [N II]λ6548 and Hα narrow emission lines. For Type 1 AGN, this is the flux of the narrow component, i.e. the BLR component is not included. (7) Half-light radius (Re) of the [O III] systemic emission ([−300, 300] km s−1 range), deconvolved from the PSF. If Re is smaller than the PSF, we give the size of the PSF as an upper limit. (8) Half-light radius (Re) of the Hα systemic emission ([−300, 300] km s−1 range), deconvolved from the PSF. (9) Components used to fit the emission lines. ‘n’: narrow component, ‘b’: broad component (for the outflow), ‘BLR’: broad line region component.
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