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 Obscured AGB in Magellanic Clouds. I. (Loup+ 1997)
    J/A+AS/125/419/table1(c)Optically known red supergiants or AGB stars with an IRAS counterpart. (59 rows)
    J/A+AS/125/419/table2(c)Obscured AGB (without any known optical counterpart) identified as such through JHK(L) photometry (36 rows)
    J/A+AS/125/419/table3(c)Planetary nebulae with an IRAS counterpart (23 rows)
    J/A+AS/125/419/table4(c)IRAS sources from group 1, i.e. the best candidates to be AGB or post-AGB stars, or PNe. (209 rows)
    J/A+AS/125/419/table5(c)IRAS sources from group 2 : IRAS data does not allow to conclude on their nature; they can be anything (143 rows)
    J/A+AS/125/419/table6(c)Foreground stars associated with IRAS sources from groups 1 and 2 (164 rows)
    J/A+AS/125/419/table7(c)IRAS sources associated with hot stars, clusters, HII regions, or galaxies (91 rows)
    J/A+AS/125/419/table8Comparison between IRAS fluxes determinations (61 rows)

       (c)  indicates tables which contain celestial coordinates 

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