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Table 2

Integrated properties and statistics of the AV distributions.

Object AV,nuclear AV,nuclear A V, R eff AV,FoV AV,median AV,mean AV (P5) AV (P95) Nspaxel
(1) (2) (3) (5) (6) (7) (8) (9) (10) (11)

IRASF 12115-4656 ···  ···  7.7 ± 0.1 5.2 ± 0.1 4.9 6.3 ± 8.1 –3.65 21.5 1533
IC 5179 10.4 ± 0.4 ···  4.2 ±0.1 4.2 ±0.1 4.4 5.2 ±6.3 –3.00 17.3 2099
NGC 2369 16.8 ± 0.2 ···  17.3 ±0.1 15.0 ±0.1 15.5 13.5 ±6.6 3.75 26.0 603
NGC 5135 2.8 ± 0.2 ···  3.8 ±0.1 3.7 ±0.1 4.2 4.7 ±4.5 –1.72 11.7 1100
NGC 3110 ···  ···  7.4 ± 0.1 7.4 ± 0.1 7.9 7.9 ± 5.8 –3.02 16.6 400
NGC 7130 12.3 ± 0.3 ···  11.8 ±0.2 8.7 ±0.1 6.2 5.9 ±6.5 –2.45 18.6 687
ESO 320-G030 ···  ···  7.8 ± 0.1 7.0 ± 0.1 7.8 8.0 ± 7.1 –2.82 20.1 1383
IRASF 17138-1017 15.2 ± 0.4 ···  11.1 ±0.1 7.0 ±0.1 7.6 6.1 ±5.6 –0.91 17.2 806
IC 4687 10.6 ± 0.1 ···  3.9 ±0.1 3.7 ±0.1 4.2 4.5 ±5.1 –1.74 13.1 3401
NGC 3256 ···  12.2 ±0.2 5.0 ±0.1 4.1 ±0.1 5.0 6.6 ±6.1 –2.73 16.8 4522
IRAS 23128-5919 8.7 ± 0.3 6.7 ± 0.2 7.1 ± 0.1 6.8 ± 0.1 6.2 7.0 ± 4.7 –1.60 13.4 1182
IRAS 21130-4446 4.3 ± 0.4 3.2 ± 0.2 4.7 ± 0.3 4.4 ± 0.1 5.4 5.0 ± 5.9 –1.80 15.5 214
IRAS 22491-1808 4.1 ± 0.3 4.5 ± 0.2 5.5 ± 0.1 5.3 ± 0.1 6.4 6.5 ± 5.1 –1.79 16.0 299
IRAS 06206-6315 7.5 ± 0.3 11.3 ± 0.4 7.6 ± 0.2 8.5 ± 0.2 10.7 9.5 ± 7.7 –3.05 22.7 114
IRAS 12112+0305 8.9 ± 0.3 8.4 ± 0.2 9.2 ± 0.2 8.5 ± 0.1 8.2 9.0 ± 6.2 –0.52 20.9 466
IRAS 14348-1447 5.5 ± 0.2 8.1 ± 0.3 6.2 ± 0.2 7.1 ± 0.1 8.6 7.9 ± 6.9 –1.04 20.6 301
IRAS 17208-0014 8.0 ± 0.2 ···  6.8 ±0.1 5.8 ±0.1 4.8 6.3 ±4.0 –1.61 10.8 485

Notes.Columns (2) and (3): Nuclear extinction measured at the main (2) and secondary (3) nucleus within an aperture radius of 063. Columns (4) and (5): Measurements of the AV within the Hα effective radius from Arribas et al. (2012), and the integrated measurement over the whole FoV, respectively. Columns (6) to (9): Median, weighted mean, and 5th and 95th percentiles of the AV distributions. Column (10): Number of valid spaxels in the AV maps and distributions.

(†)

Since the main nucleus of NGC 3256 was not observed, we centred the aperture for AV,Reff on the centre of the FoV, so the measurement might be inaccurate.

(‡)

Due to the limited FoV of the observations, in these objects the Hα effective radius is greater than our FoV, and the AV,Reff measurements are equivalent to AV,FoV.

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