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Table 6.

AGN properties from the modeling of the Hβ, [O III] and Fe II spectral region.

Object f(Hβ) (a) f(FeII) (b) f(OIII) (c) FWHMHβ(d) σHβ(e) MBH(f) Lbol(g) λEdd(h)
10−16 erg s−1cm−2 [km s−1] [km s−1] [106 M⊙] [1043 erg s−1]
HE0021−1810 95 ± 5 90 ± 3 185 ± 1 5079 ± 65 2194 ± 28 12.3 ± 3.2 6.6 ± 0.7 0.04 ± 0.01
HE0021−1819 92 ± 0 10 ± 1 289 ± 0 3624 ± 22 1539 ± 9 6.1 ± 1.3 6.4 ± 0.6 0.08 ± 0.02
HE0040−1105 349 ± 1 88 ± 2 501 ± 0 2696 ± 6 1144 ± 2 5.5 ± 0.8 13.4 ± 1.3 0.19 ± 0.04
HE0108−4743 307 ± 2 174 ± 4 283 ± 1 1174 ± 19 934 ± 24 0.5 ± 0.1 4.3 ± 0.4 0.69 ± 0.15
HE0114−0015 83 ± 1 52 ± 2 61 ± 0 2764 ± 39 1174 ± 17 2.8 ± 0.6 4.4 ± 0.4 0.13 ± 0.03
HE0119−0118 863 ± 3 235 ± 4 746 ± 1 2983 ± 31 1861 ± 11 15.9 ± 2.4 48.0 ± 4.8 0.24 ± 0.04
HE0212−0059 1524 ± 83 52 ± 1 560 ± 4 9133 ± 228 4329 ± 120 86.8 ± 17.5 21.3 ± 2.1 0.02 ± 0.00
HE0224−2834 488 ± 2 106 ± 2 386 ± 1 4989 ± 20 2119 ± 9 35.8 ± 3.7 34.6 ± 3.5 0.08 ± 0.01
HE0227−0913 2658 ± 5 1719 ± 4 442 ± 1 1127 ± 5 1025 ± 4 1.0 ± 0.2 14.2 ± 1.4 1.12 ± 0.27
HE0232−0900 3663 ± 5 491 ± 5 2820 ± 2 5017 ± 7 2131 ± 3 79.1 ± 9.8 111.2 ± 11.1 0.11 ± 0.02
HE0253−1641 673 ± 4 632 ± 4 890 ± 2 1707 ± 10 1376 ± 13 2.3 ± 0.3 14.5 ± 1.5 0.49 ± 0.08
HE0345+0056 5929 ± 31 2901 ± 7 2140 ± 7 906 ± 8 1141 ± 8 2.3 ± 0.2 92.5 ± 9.2 3.22 ± 0.31
HE0351+0240 643 ± 1 170 ± 4 576 ± 1 2710 ± 7 1228 ± 4 6.6 ± 1.1 16.9 ± 1.7 0.20 ± 0.05
HE0412−0803 2579 ± 836 523 ± 3 6880 ± 200 4022 ± 1258 1709 ± 36 35.9 ± 16.9 66.2 ± 6.6 0.15 ± 0.15
HE0429−0247 616 ± 2 140 ± 2 331 ± 0 1479 ± 23 1390 ± 7 2.3 ± 0.4 22.3 ± 2.2 0.75 ± 0.15
HE0433−1028 2640 ± 7 883 ± 4 1389 ± 2 2676 ± 14 1667 ± 7 14.6 ± 1.7 58.4 ± 5.8 0.32 ± 0.06
HE0853+0102 154 ± 26 61 ± 2 124 ± 5 3850 ± 1557 1571 ± 493 9.2 ± 4.3 9.8 ± 1.0 0.08 ± 0.10
HE0853−0126 40 ± 1 40 ± 2 15 ± 1 794 ± 32 1079 ± 105 0.2 ± 0.0 3.8 ± 0.4 1.45 ± 0.32
HE0934+0119 985 ± 1 335 ± 2 363 ± 0 1559 ± 6 1053 ± 5 4.3 ± 0.6 47.3 ± 4.7 0.87 ± 0.13
HE0949−0122 582 ± 23 550 ± 5 735 ± 3 1300 ± 22 1959 ± 17 0.7 ± 0.2 5.3 ± 0.5 0.61 ± 0.17
HE1011−0403 1111 ± 2 457 ± 4 325 ± 1 2043 ± 6 1104 ± 6 9.5 ± 1.1 68.3 ± 6.8 0.57 ± 0.11
HE1017−0305 1167 ± 5 457 ± 5 206 ± 1 4525 ± 20 1925 ± 8 38.5 ± 4.1 51.5 ± 5.2 0.11 ± 0.01
HE1029−1831 594 ± 19 225 ± 4 377 ± 1 2538 ± 20 1293 ± 38 6.4 ± 0.8 20.0 ± 2.0 0.25 ± 0.04
HE1107−0813 2273 ± 124 1147 ± 4 108 ± 6 3369 ± 219 1817 ± 26 39.3 ± 7.6 128.6 ± 12.9 0.26 ± 0.05
HE1108−2813 890 ± 2 743 ± 8 480 ± 1 2985 ± 9 1267 ± 4 6.0 ± 1.1 11.1 ± 1.1 0.15 ± 0.03
HE1126−0407 4056 ± 7 3443 ± 5 668 ± 2 2199 ± 8 1404 ± 4 24.4 ± 4.2 225.5 ± 22.6 0.73 ± 0.16
HE1237−0504 2625 ± 4 1694 ± 3 1697 ± 2 3880 ± 7 1651 ± 3 5.4 ± 1.0 4.4 ± 0.4 0.06 ± 0.01
HE1248−1356 136 ± 2 88 ± 4 433 ± 1 3397 ± 54 1443 ± 23 1.4 ± 0.4 0.8 ± 0.1 0.05 ± 0.02
HE1310−1051 1363 ± 3 302 ± 3 1185 ± 1 3540 ± 8 1503 ± 4 16.8 ± 1.6 31.1 ± 3.1 0.15 ± 0.02
HE1330−1013 464 ± 3 286 ± 5 136 ± 1 1858 ± 20 1357 ± 24 1.5 ± 0.4 5.6 ± 0.6 0.30 ± 0.09
HE1338−1423 2583 ± 20 385 ± 2 1535 ± 4 1751 ± 35 1167 ± 11 7.5 ± 1.0 76.2 ± 7.6 0.81 ± 0.15
HE1353−1917 472 ± 22 149 ± 3 392 ± 1 6655 ± 41 2491 ± 106 32.4 ± 4.7 12.6 ± 1.3 0.03 ± 0.01
HE1417−0909 727 ± 29 111 ± 3 611 ± 42 3356 ± 13 1425 ± 5 13.9 ± 2.2 27.4 ± 2.7 0.16 ± 0.03
HE2128−0221 166 ± 1 90 ± 2 194 ± 0 2014 ± 18 856 ± 8 2.6 ± 0.4 10.5 ± 1.0 0.32 ± 0.06
HE2211−3903 659 ± 8 371 ± 6 298 ± 1 5958 ± 59 2533 ± 25 36.7 ± 5.7 21.1 ± 2.1 0.05 ± 0.01
HE2222−0026 372 ± 2 173 ± 2 85 ± 1 3087 ± 20 1542 ± 7 11.2 ± 1.7 25.7 ± 2.6 0.18 ± 0.03
HE2233+0124 470 ± 17 62 ± 3 105 ± 2 8715 ± 152 3975 ± 101 99.7 ± 12.9 30.1 ± 3.0 0.02 ± 0.00
HE2302−0857 2214 ± 35 49 ± 4 2701 ± 134 5963 ± 112 2172 ± 26 92.8 ± 13.0 84.2 ± 8.4 0.07 ± 0.02

Notes.

(a)

Integrated BLR component flux of Hβ excluding the NLR contribution.

(b)

Integrated flux of the Fe II(5100–5550 Å) band.

(c)

Integrated NLR component flux of [O III].

(d)

FWHM of the Hβ BLR component.

(e)

Line dispersion of the Hβ BLR component.

(f)

BH mass estimated from the BLR Hβ luminosity and FWHM following Greene & Ho (2005a), see Eq. (2). Errors are based on the propagation of measurement errors and uncertainties of the scaling relation. A systematic error of 0.3 dex is typically assumed for the precision of single-epoch BH mass estimate for a single object.

(g)

Bolometric luminosity estimated from the Hβ luminosity (see text for details). Errors are dominated by the systematic uncertainty of the absolute flux calibration which is assumed to be 10 per cent.

(h)

Eddington ratio defined as Lbol/LEdd.

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