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Table 3.

Narrow line region properties from the line fitting of the integrated H-band SINFONI spectra of the SUPER sample.

Target λrange(a) Dext(b) z[O III](c)log L[O III](d)
 v[O III](e)
 log LHβ(d)
Narrow Broad FWHMnarrow FWHMbroad v10 w80 vmax Narrow Broad
(Å) (arcsec) (erg s−1) (erg s−1) (km s−1) (km s−1) (km s−1) (km s−1) (km s−1) (erg s−1) (erg s−1)
X_N_160_22 4550–5200 1.0 2.442 43.11 ± 0.04 43.30 ± 0.07 869 ± 50 3035 ± 185 −2333 ± 146 2816 ± 160 3637 ± 222 42.60 ± 0.08 –
X_N_81_44 4500–5420 0.9 2.317 42.68 ± 0.04 42.19 ± 0.13 494 ± 30 1851 ± 130 −336 ± 40 775 ± 108 1682 ± 117 41.43 ± 0.05 43.24 ± 0.05
X_N_66_23 4600–5250 0.7 2.384 – 43.16 ± 0.03 – 900 ± 44 −495 ± 36 1001 ± 51 764 ± 38 42.84 ± 0.05 –
X_N_35_20 4600–5200 0.3 2.260 – 41.87 ± 0.45 – 643 ± 106 −330 ± 78 681 ± 209 546 ± 90 – –
X_N_12_26 4450–5180 0.8 2.471 – 42.41 ± 0.07 – 933 ± 184 −680 ± 57 1044 ± 89 792 ± 156 – 42.06 ± 0.07
X_N_4_48 4500–5250 0.5 2.314 – 42.24 ± 0.07 – 1126 ± 151 −648 ± 84 1198 ± 100 956 ± 129 – 41.50 ± 0.06
X_N_102_35 4620–5400 0.3 2.190 42.51 ± 0.13 42.76 ± 0.13 550 ± 112 1473 ± 261 −1076 ± 140 1501 ± 170 1761 ± 295 41.18 ± 0.10 42.14 ± 0.09
X_N_115_23 4550–5280 0.7 2.340 43.27 ± 0.03 43.18 ± 0.02 471 ± 24 1495 ± 62 −623 ± 57 1015 ± 67 1437 ± 56 42.38 ± 0.06 42.13 ± 0.28
cid_166 4430–5185 0.6 2.460 42.60 ± 0.11 43.17 ± 0.07 503 ± 91 1703 ± 150 −1502 ± 41 1755 ± 109 2136 ± 155 41.77 ± 0.04 42.89 ± 0.10
cid_1605 4650–5200 0.4 2.117 – 42.43 ± 0.43 – 1095 ± 244 −573 ± 98 1153 ± 142 929 ± 208 – –
cid_346 4550–5450 0.7 2.216 – 42.97 ± 0.04 – 1989 ± 212 −1343 ± 166 2142 ± 231 1689 ± 181 – 42.74 ± 0.14
cid_1205 4700–5200 0.3 2.256 – 42.66 ± 0.04 – 636 ± 72 −223 ± 36 717 ± 48 540 ± 61 – –
cid_467 4600–5200 0.4 2.284 – 42.87 ± 0.43 – 1256 ± 132 −702 ± 112 1368 ± 154 1067 ± 112 – –
J1333+1649 4750–5350 1.1 2.098 44.00 ± 0.02 44.58 ± 0.04 602 ± 22 2700 ± 80 −2271 ± 78 2714 ± 96 3248 ± 87 – 44.08 ± 0.12
J1441+0454( * ) 4730–5350 1.0 2.053 – 43.41 ± 0.03 – 1956 ± 96 -3698 ± 70 2161 ± 102 1661 ± 82 42.29 ± 0.13 42.79 ± 0.19
J1549+1245 4450–5250 1.0 2.367 43.15 ± 0.10 44.49 ± 0.05 327 ± 49 1362 ± 25 −613 ± 27 1457 ± 38 1413 ± 32 41.40 ± 0.10 43.47 ± 0.06
S82X1905 4550–5450 0.8 2.272 – 42.82 ± 0.04 – 607 ± 59 -304 ± 34 678 ± 55 515 ± 54 42.18 ± 0.15 –
S82X1940 4550–5400 0.6 2.349 42.28 ± 0.03 42.54 ± 0.03 354 ± 20 1336 ± 71 −820 ± 51 1186 ± 39 1373 ± 71 41.30 ± 0.17 42.09 ± 0.09
S82X2058 4600–5400 0.6 2.314 42.44 ± 0.08 42.61 ± 0.08 539 ± 61 1442 ± 109 −972 ± 88 1340 ± 95 1701 ± 234 42.01 ± 0.09 41.67 ± 0.40

Notes.

(a)

The wavelength range used for the emission line fitting.

(b)

The diameter (in arcsec) of the circular aperture centred on the target used to extract the spectrum.

(c)

Redshift of the target determined from the peak location of the [O III] λ5007 in the integrated spectrum.

(d)

The luminosity of the individual Gaussian components in erg s−1, not corrected for reddening. The emission lines were modelled using multiple Gaussian components and the terms “narrow” and “broad” refer to these individual Gaussian components parameters. In case of single Gaussian fits, the Gaussian component is classified as broad if the width (FWHM) > 600 km s−1. – means that there was no detection of the corresponding component. The errors indicate 1σ uncertainty.

(e)

Line widths (FWHM) of the individual Gaussian components. v10 and w80 are the non-parametric velocities and vmax the maximum velocity as defined in Sect. 5.1.

( * )The fit does not constrain the NLR properties due to contamination from telluric absorption and strong contribution from FeII emission. The reported [O III] emission is highly blue-shifted (∼−3000 km s−1) and the [O III] redshift corresponds to this component.

There is no detection of lines in X_N_53_3 and X_N_44_64.

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