19254-7245$^2$                       7.1         7.0       11.3         –           8.3           –           –         –    
   IRAS 19254-7245$^3$                       3.4         3.6         –          –            –            –           –         –    
   IRAS 23128-5919$^4$                       7.2         7.0       11.5         –           8.5           –           –         –    
   IRAS 23128-5919$^5$                        –           –          –          –            –            –           –       148.7  
   IRAS 14348-1447$^6$                       8.6         8.4         –          –            –            –           –         –    
  --------------------- ---------------- ------------ ---------- --------- ------------ ------------ ------------ ---------- ------- --

**Table note:** The numbers following each galaxy denote the total on-source exposure time (in minutes) for each filter used, and two galaxies were observed more than once under different configurations, the details of which are: (1) IRAS19254-7245 observed in proposal CAMACTI2 (PI I.F. Mirabel), 7 LW filters, integration time per frame Tint=5s, pfov=1.5“. (2) IRAS19254-7245 observed in proposal CAMACTIV (PI I.F. Mirabel), 4 LW filters, Tint=2s, pfov=1.5”. (3) IRAS19254-7245 observed in proposal SAM12N\_2 proposal (PI L. Spinoglio), 2 LW filters, Tint=2s, pfov=3“. (4) IRAS23128-5919 observed in proposal CAMACTIV (PI I.F. Mirabel), 4 LW filters, Tint=2s, pfov=1.5”. (5) IRAS23128-5919 observed in proposal CAMACTI2 (PI I.F. Mirabel), CVF, Tint=5s, pfov=1.5“. (6) IRAS14348-1447 observed in proposal CAMACTIV (PI I.F. Mirabel), 2 LW filters, Tint=2s, pfov=1.5”.

Results
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Background and General Properties {#sec:results}
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The sensitivity and spatial resolution capabilities of ISOCAM enable us 