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Table 2.

Intensity modelling table for CARS sources.

Object FWHMmax(a) e(b) Scale (c) S[O III](d) r[O III](e) p-value (f) σ[O III]:Hβ(g) Type (h)
(mas) (kpc/″) (pc)
HE 0021−1810 1001 ± 69 0.36 ± 0.10 0.845 40 ± 29 ± 100 1.01 ± 0.01 0.01 1.47 Unresolved
HE 0021−1819 791 ± 7 0.37 ± 0.02 1.051 44 ± 4 ± 11 1.01 ± 0.01 4.1 × 10−3 1.97 Resolved
HE 0040−1105 741 ± 3 0.33 ± 0.01 1.099 92 ± 2 ± 8 0.99 ± 0.01 0.28 1.21 Unresolved
HE 0108−4743 1451 ± 22 0.27 ± 0.05 1.591 67 ± 8 ± 12 0.84 ± 0.02 3.5 × 10−7 2.99 Resolved
HE 0114−0015 633 ± 11 0.30 ± 0.04 1.104 70 ± 21 ± 67 0.99 ± 0.03 0.75 0.83 Unresolved
HE 0119−0118 748 ± 11 0.38 ± 0.03 1.026 54 ± 7 ± 8 1.06 ± 0.01 2.1 × 10−8 3.02 Resolved
HE 0212−0059 673 ± 7 0.12 ± 0.04 0.970 186 ± 8 ± 4 1.39 ± 0.08 6.6 × 10−5 2.43 Resolved
HE 0224−2834 1661 ± 7 0.16 ± 0.02 0.951 29 ± 7 ± 10 0.99 ± 0.02 0.23 0.81 Unresolved
HE 0227−0913 1204 ± 3 0.19 ± 0.01 1.005 16 ± 3 ± 14 1.06 ± 0.02 0.01 0.62 Unresolved
HE 0232−0900 1222 ± 2 0.23 ± 0.01 1.994 126 ± 2 ± 4 0.86 ± 0.02 5.2 × 10−11 3.41 Resolved
HE 0253−1641 954 ± 10 0.28 ± 0.02 1.630 22 ± 3 ± 14 1.00 ± 0.01 0.21 1.23 Unresolved
HE 0345+0056 921 ± 3 0.18 ± 0.01 1.015 7 ± 1 ± 8 1.04 ± 0.01 0.49 1.06 Unresolved
HE 0351+0240 794 ± 3 0.29 ± 0.01 1.657 16 ± 5 ± 19 0.89 ± 0.02 3.8 × 10−3 1.68 Resolved
HE 0412−0803 781 ± 1 0.30 ± 0.00 1.087 26 ± 1 ± 4 0.90 ± 0.01 1.4 × 10−5 1.98 Resolved
HE 0429−0247 980 ± 8 0.24 ± 0.02 1.850 42 ± 4 ± 11 1.06 ± 0.01 4.5 × 10−4 1.76 Resolved
HE 0433−1028 606 ± 4 0.12 ± 0.03 1.588 14 ± 1 ± 6 1.00 ± 0.01 0.08 1.42 Unresolved
HE 0853+0102 628 ± 8 0.20 ± 0.04 1.044 12 ± 6 ± 8 1.00 ± 0.01 0.10 1.32 Unresolved
HE 0934+0119 744 ± 6 0.07 ± 0.03 1.011 27 ± 5 ± 13 1.00 ± 0.01 0.27 1.24 Unresolved
HE 1011−0403 820 ± 8 0.17 ± 0.04 1.070 17 ± 6 ± 25 1.02 ± 0.01 0.70 1.10 Unresolved
HE 1017−0305 806 ± 3 0.28 ± 0.01 1.106 14 ± 8 ± 27 0.90 ± 0.02 1.8 × 10−3 0.63 Unresolved
HE 1029−1831 751 ± 10 0.26 ± 0.05 1.080 57 ± 5 ± 12 0.94 ± 0.02 3.3 × 10−6 5.52 Resolved
HE 1107−0813 697 ± 8 0.39 ± 0.02 1.087 40 ± 14 ± 164 0.95 ± 0.03 0.71 0.98 Unresolved
HE 1108−2813 510 ± 2 0.27 ± 0.01 0.981 35 ± 2 ± 8 1.00 ± 0.01 0.61 1.00 Unresolved
HE 1126−0407 811 ± 3 0.29 ± 0.01 1.075 23 ± 4 ± 28 1.02 ± 0.01 0.92 0.96 Unresolved
HE 1237−0504 614 ± 1 0.23 ± 0.01 0.982 5 ± 0 ± 3 0.99 ± 0.01 3.3 × 10−6 0.46 Unresolved
HE 1248−1356 646 ± 9 0.41 ± 0.02 0.960 11 ± 2 ± 5 1.03 ± 0.02 1.8 × 10−8 5.17 Resolved
HE 1310−1051 536 ± 1 0.60 ± 0.00 1.026 4 ± 1 ± 2 1.01 ± 0.01 4.3 × 10−3 0.43 Unresolved
HE 1330−1013 775 ± 12 0.25 ± 0.05 0.817 19 ± 5 ± 17 1.01 ± 0.02 0.09 0.76 Unresolved
HE 1338−1423 398 ± 4 0.68 ± 0.00 1.105 49 ± 1 ± 6 0.74 ± 0.01 2.0 × 10−8 10.67 Resolved
HE 1353−1917 811 ± 9 0.26 ± 0.04 0.853 802 ± 7 ± 17 1.15 ± 0.11 8.6 × 10−11 7.18 Resolved
HE 1417−0909 769 ± 2 0.27 ± 0.01 0.615 33 ± 3 ± 10 0.95 ± 0.01 0.01 0.68 Unresolved
HE 2128−0221 757 ± 6 0.11 ± 0.03 0.899 38 ± 8 ± 25 0.97 ± 0.02 0.12 0.73 Unresolved
HE 2211−3903 529 ± 4 0.32 ± 0.02 0.803 78 ± 9 ± 15 0.93 ± 0.02 0.12 0.69 Unresolved
HE 2222−0026 680 ± 6 0.23 ± 0.03 0.905 45 ± 14 ± 44 0.99 ± 0.02 5.9 × 10−4 0.55 Unresolved
HE 2233+0124 927 ± 15 0.33 ± 0.03 0.575 37 ± 23 ± 39 1.02 ± 0.03 3.3 × 10−3 0.69 Unresolved
HE 2302−0857 729 ± 8 0.17 ± 0.03 1.131 178 ± 6 ± 15 1.24 ± 0.03 3.2 × 10−5 2.14 Resolved

Notes.

(a)

Maximum FWHM estimated from the semi-major axis of the best-fit elliptical Moffat model fitted to the surface brightness map of BLR Hβ,

(b)

ellipticity of the best-fit elliptical Moffat model,

(c)

the kiloparsec per arcsecond scale achievable for individual objects,

(d)

the offset between the Moffat centers of BLR Hβ and [O III] wing. It quantifies how the is the region of the region of maximum [O III] wing emission from the AGN central engine. It further gives an indication of the lower limit of the size of the outflowing region. The size of the outflowing region could be extended far beyond this distance, but this quantifies that the outflow has already traversed at least distance; and hence it is a lower limit of the size of the outflowing region. The first uncertainty denotes the random uncertainty due to measurements; and the second uncertainty denotes the uncertainty in position measurement due to systematics,

(e)

the flux ratio of the integrated surface brightness profile within central 2–3″ (2″ for MUSE and 3″ for VIMOS) and that of the best-fit Moffat model for [O III] wing,

(f)

the p-value estimated from Levene’s test to check the similarity of distributions between the normalized residuals of BLR Hβ and [O III] wing,

(g)

the ratio of standard deviation of the normalized residuals of [O III] wing and BLR Hβ,

(h)

the characterization of the spatial profile of the [O III] wing- if they are unresolved or resolved.

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