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