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Table 2:

List of observed Seyfert galaxies - observational parameters.
Object Observation Integration time Integration time Spatial sampling Spatial sampling
  date in MR1 [s] in MR2 [s] MR1 MR2
Mrk 34 14-15/03/2001 $1\times 2700$ $2\times 2700$ HR LR
Mrk 622 24/11/2000 $2\times 1800$ $2\times 1800$ HR HR
Mrk 1066 22/11/2000 $3\times 1800 + 1\times 1200$ $2\times 1800$ HR HR
NGC 262 25/11/2000 $2\times 1800$ $2\times 1800$ HR HR
NGC 449 24/11/2000 3 fields $\times~2 \times 1800$ 3 fields $\times~2 \times 1800$ HR HR
NGC 2273 24/11/2000 $2\times 1800$ -- LR --
NGC 2992 16-17/03/2001 $1\times 1800 + 1\times 2700$ $2\times 1800$ LR HR
NGC 3081 17/01/2002 $2\times3600$ -- LR --
NGC 4388 17/01/2002 $3\times3300$ -- LR --
NGC 5728 15/03/2001 $2\times 1800$ $1\times 1800 + 1\times 2700$ LR LR
NGC 5929 16/03/2001 $2\times 2700$ -- LR --
The abbreviations used: MR1: spectral mode of wavelength range (4760,5558) Å, dispersion 2.15 Å/pixel, resolving power 1210; MR2: spectral mode of wavelength range (6210,7008) Å, dispersion 2.17 Å/pixel, resolving power 1525; HR: high spatial resolution mode with sky sampling  $0.27\hbox{$^{\prime\prime}$ }$, field of view $10.4\hbox{$^{\prime\prime}$ }$ $\times$ $8.3\hbox{$^{\prime\prime}$ }$; LR: low spatial resolution mode, sky sampling  $0.41\hbox{$^{\prime\prime}$ }$, field of view $15\hbox{$^{\prime\prime}$ }$ $\times$ $12\hbox{$^{\prime\prime}$ }$.

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