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Table 2.

Spectroscopic best-fit results.

Name f[O III] f[O III]/ fHβ fHα f[N II]/ fHα W80[O III] W80Hα V10[O III] V10Hα V90[O III] V90Hα Vpeak
J0143 725 ± 25 3.1 ± 0.4 680 ± 26 0.10 ± 0.04 169 ± 3 143 ± 7 −29 ± 2 −49 ± 3 140 ± 3 94 ± 7 0 ± 2
J1343 69 ± 7 0.08 ± 0.07 119 ± 10 −57 ± 6 62 ± 6 0 ± 4
J1038 485 ± 13 5.34 ± 0.35 350 ± 5 0.06 ± 0.02 182 ± 3 190 ± 6 −148 ± 7 −132 ± 6 57 ± 4 57 ± 3 0 ± 1
–A1 23.4 ± 0.8 3.9 ± 0.7 22.5 ± 0.6 0.07 ± 0.03 202 ± 5 211 ± 9 −121 ± 5 −123 ± 5 91 ± 4 87 ± 5 −60 ± 25
–A2 94.2 ± 1.4 6.2 ± 0.6 63.8 ± 1.7 0.06 ± 0.01 154 ± 4 171 ± 6 −103 ± 3 −121 ± 3 50 ± 3 51 ± 6 2 ± 1
–A3 165.1 ± 1.6 6.2 ± 0.4 116.9 ± 3.2 0.05 ± 0.01 152 ± 3 163 ± 9 −103 ± 2 −113 ± 8 51 ± 2 50 ± 4 −1 ± 3
–A4 87.2 ± 1.2 6.0 ± 0.5 58.1 ± 1.3 0.03 ± 0.01 165 ± 4 175 ± 5 −116 ± 1 −126 ± 3 49 ± 3 46 ± 5 −8 ± 1
J1958 14400 ± 300 4.6 ± 0.4 12 400 ± 500 0.10 ± 0.05 282 ± 7 269 ± 8 −66 ± 4 −73 ± 4 213 ± 6 191 ± 9 4 ± 4
–A1 3500 ± 100 5.3 ± 0.7 3600 ± 200 0.13 ± 0.06 179 ± 9 182 ± 11 −71 ± 6 −77 ± 7 101 ± 9 105 ± 11 −5 ± 5
–A2 5100 ± 100 3.4 ± 0.2 4300 ± 200 0.20 ± 0.08 224 ± 12 188 ± 7 −82 ± 3 −90 ± 5 145 ± 13 98 ± 7 −3 ± 2
–B 2000 ± 200 4.5 ± 1.5 1700 ± 240 <0.3b 184 ± 35 158 ± 24 75 ± 30 99 ± 24 257 ± 7 257 ± 7 191 ± 13
J1110 178 ± 5 <0.16b 113 ± 4 −57 ± 2 55 ± 2 0 ± 1
–A1 49 ± 2 105 ± 5 −52 ± 3 53 ± 3 −1 ± 2
–A2 39 ± 2 112 ± 6 −71 ± 4 41 ± 4 −15 ± 2
–A3 6 ± 1 94 ± 28 −56 ± 5 38 ± 5 −8 ± 2
J0022a 140 ± 3 0.27 ± 0.01 313 ± 12 −230 ± 9 82 ± 9 −62 ± 12
–A1 9 ± 2 0.26 ± 0.07 297 ± 78 −197 ± 77 100 ± 38 −22 ± 16
–A2 53 ± 2 0.26 ± 0.02 286 ± 15 −218 ± 17 68 ± 11 −40 ± 29
–A3 36 ± 2 0.25 ± 0.02 266 ± 17 −187 ± 19 78 ± 10 −34 ± 16

Notes. Column (1): target name and relative images in the arc-structure; Cols. (2) to (5): non-lensing-corrected fluxes (in 10−17 erg s−1 cm2) and flux ratios. Columns (6) to (11): non-parametric velocity measurements from [O III]5007 and Hα. Column (12): Vpeak measurements.

(a)

For J0022, non-parametric estimates are derived from the[N II] line instead of Hα (see text). All velocities are not corrected for the instrument spectral resolution; by subtracting the instrumental resolution in quadrature we would obtain a difference of 20 km s−1 for velocities as low as 70 km s−1 and even smaller corrections for highest velocities (i.e. <10 km s−1 at ν > 100 km s−1).

(b)

From a 3σ upper limit on the undetected [N II] line.

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