Table 4.
Properties of the ionised gas obtained from the analysis of the COG, spectroastrometry, and the flux and velocity maps.
| Target |
 |
 |
vo | Ro | D600 |
 |
Ṁcone | Ṁthin-shell | fesc |
|---|---|---|---|---|---|---|---|---|---|
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | |
| (kpc ) | (kpc) | (km s−1) | (kpc) | (kpc) | (erg s−1) | (M⊙ yr−1) | (M⊙ yr−1) | (%) | |
| X_N_160_22 | 1.54 ± 0.02 | 1.52 ± 0.02 | −1700 | 0.4 | – | 43.36 | 4–79 | 5–105 | 38 |
| X_N_81_44 | 1.84 ± 0.16 | 1.61 ± 0.05 | +500 | 0.9 | 2.4 | 42.26 | 0.1–1 | 0.1–2 | 6 |
| X_N_66_23 | 1.29 ± 0.12 | 1.03 ± 0.02 | 600 | 0.4 | 2.4 | 42.88 | 0.4–7 | 0.5–10 | 4 |
| X_N_35_20 ( * *) | – | – | 681 | < 2.2 | – | 41.31 | 0.01–0.2 | 0.01–0.2 | 0 |
| X_N_12_26 | 1.08 ± 0.07 | 1.14 ± 0.01 | −400 | 0.3 | – | 42.06 | 0.1–1 | 0.1–2 | 2 |
| X_N_4_48 ( * ) | – | – | 1198 | < 2.9 | – | 41.97 | 0.1–1 | 0.1–2 | 5 |
| X_N_102_35( * ) | – | – | 1501 | < 7.6 | – | 42.68 | 0.4–9 | 0.6–12 | 16 |
| X_N_115_23 | 1.67 ± 0.04 | 1.49 ± 0.04 | +900 | 0.9 | 4.0 | 43.09 | 0.3–6 | 0.4–8 | 7 |
| cid_166 | 1.42 ± 0.03 | 1.42 ± 0.02 | −2100 | 0.7 | – | 43.10 | 1–27 | 2–36 | 30 |
| cid_1605( * ) | – | – | 1153 | < 5.8 | – | 42.15 | 0.1–2 | 0.1–3 | 4 |
| cid_346 | 2.12 ± 0.07 | 1.90 ± 0.05 | +600 | 2.8 | 5.6 | 42.83 | 0.6–11 | 0.8–15 | 27 |
| cid_1205( † ) | – | – | 717 | < 2.5 | – | 42.08 | 0.05–1 | 0.1–1 | 0 |
| cid_467( * ) | – | – | 1368 | < 9.0 | – | 42.63 | 0.4–7 | 0.5–10 | 8 |
| J1333+1649 | 1.76 ± 0.03 | 1.74 ± 0.05 | −2900 | 0.3 | 6.5 | 44.54 | 51–1021 | 68–1361 | 43 |
| J1441+0454( * *) | – | – | 2161 | < 2.8 | – | 43.41 | 3–68 | 4–91 | 97 |
| J1549+1245 | 1.35 ± 0.03 | 1.25 ± 0.03 | +1300 | 0.2 | 4.0 | 44.29 | 16–326 | 22–435 | 12 |
| S82X1905 | 1.86 ± 0.04 | 1.73 ± 0.01 | +300 | 2.7 | 1.6 | 42.21 | 0.04–0.8 | 0.1–1 | 0 |
| S82X1940 | 1.23 ± 0.03 | 1.29 ± 0.04 | −600 | 0.6 | – | 42.35 | 0.2–3 | 0.2–4 | 8 |
| S82X2058( † ) | – | – | 1340 | < 2.2 | – | 42.54 | 0.3–6 | 0.4–8 | 13 |
Notes. (1) and (2): 
and 
are the half-light radius of the BLR PSF and [O III] emission, respectively, derived from the COG analysis for 11 targets with S/N > 5 in the integrated spectrum of [O III], as described in Sect. 5.2. 
is not computed for X_N_35_20 and J1441+0454 as the [O III] S/N is low. Targets marked by ( * ) were observed without AO and are not resolved. H-band data cubes of cid_1205 and S82X1058 (marked by ( † )) have a bright stripe that interferes in the spatially resolved analysis, and therefore the half-light radii are not reported (see Sect. 5.1). (3) and (4): vo is the outflow velocity of the bulk of the ionised gas, which is at the maximum distance, Ro, from the AGN. vo and Ro are derived from the spectroastrometry analysis of the 11 targets with S/N > 5 in the integrated spectrum of [O III], as described in Sect. 5.4. For targets marked by ( * ), ( * *), or ( † ), we report the w80 value of the integrated spectrum and the PSF value as a proxy for vo and Ro. (5): D600 is the maximum projected spatial extent of w80 > 600 km s−1 from the maps in Figs. 7 and 8. D600 is calculated for seven targets that show extended ionised gas emission from COG and PSF-subtraction methods. (6): 
is the outflow luminosity computed from [O III] λ5007 emission line for channels with |v| > 300 km s−1 (Sect. 5.5). (7) and (8): Ṁcone and Ṁthin-shell are the masss outflow rates assuming a biconical and a thin-shell geometry described in Sect. 5.5. The two values in each column correspond to the outflow rates assuming an electron density of 104 cm−3 and 500 cm−3. (9): fesc is the fraction of the outflowing gas which has the capability to escape the gravitational potential of the host galaxy (Sect. 6).
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