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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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