Table 1: Source parameters.

Source name		 Date Inst/AOT a FOV/slit b R $\alpha (2000)$ $\delta (2000)$ z L Mag c
Galactic center                
GC SgrA* 19 Feb. 1996 ISO/ SWS01 $14''\times 20''$ R 17h45m39.97s -29d00'28.7'' - 3.1
GC SgrA* 21 Feb. 1997 ISO/ SWS06 $14''\times 20''$ R 17h45m39.97s -29d00'28.8'' -  
GCS 3 I 29 Aug. 1996 ISO/ SWS01 $14''\times 20''$ R 17h46m14.84s -28d49'33.8'' - 3.2
GCS 3 I 08 Oct. 1996 ISO/ SWS06 $14''\times 20''$ R 17h46m14.84s -28d49'33.7'' -  
IRAS 17424-2859 01 Apr. 1996 ISO/ SWS01 $14''\times 20''$ R 17h45m39.93s -29d00'22.8'' - 5
GC IRS7 29 May 2002 VLT ISAAC/LWS3 LR 0.6'' 600 17h45m41.1s -29d00'44.8'' - 5
Seyfert sources                
NGC 1068 18 Aug. 2001 VLT ISAAC/LWS3 LR 1.0'' 360 02h42m40.7s -00d00m48s 0.003793 5.4
NGC 7172 05 Aug. 2001 VLT ISAAC/LWS3 LR 1.0'' 360 22h02m01.7s -31d52m18s 0.008683 8.5
IRAS 19254-7245 04 Jun. 2002 VLT ISAAC/LWS3 LR 1.0'' 360 19h31m21.4s -72d39m18s 0.061709 11.4
NGC 5506 18 Jun. 2003 VLT ISAAC/LWS3 LR 1.0'' 360 14h13m14.87s -03d12m27s 0.006068 7.4
    a AOT: Astronomical Observation Template.
    b FOV: Field Of View, for ISO-SWS data; slit width for VLT-ISAAC ones.
    c given L band magnitude are approximate as they are aperture dependent for most of the sources.
     ISO-SWS spectra are recorded in a source crowded area with a beam size of about $14''\times 20''$.

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