We have selected 198 IRAS sources in the Large Magellanic Cloud, and 11 in the Small Magellanic Cloud, which are the best candidates to be mass-loosing AGB stars (or possibly post-AGB stars). We used the catalogues of Schwering & Israel (1990, Cat. II/181) and Reid et al. (1990, Cat. J/ApJ/348/98). They are based on the IRAS pointed observations and have lower detection limits than the Point Source Catalogue. We also made cross-identifications between IRAS sources and optical catalogues.

Cone search capability for table J/A+AS/125/419/table5 (IRAS sources from group 2 : IRAS data does not allow to conclude on their nature; they can be anything)

Cone search capability for table J/A+AS/125/419/table6 (Foreground stars associated with IRAS sources from groups 1 and 2)

Cone search capability for table J/A+AS/125/419/table1 (Optically known red supergiants or AGB stars with an IRAS counterpart.)

Cone search capability for table J/A+AS/125/419/table2 (Obscured AGB (without any known optical counterpart) identified as such through JHK(L) photometry)

Cone search capability for table J/A+AS/125/419/table3 (Planetary nebulae with an IRAS counterpart)

Cone search capability for table J/A+AS/125/419/table4 (IRAS sources from group 1, i.e. the best candidates to be AGB or post-AGB stars, or PNe.)

Cone search capability for table J/A+AS/125/419/table7 (IRAS sources associated with hot stars, clusters, HII regions, or galaxies)