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Table 1

Complete source sample of the COSAS program.

Source Chemistry and Source Chemistry and Source Chemistry and
name variability or type name variability or type name variability or type

in this paper: in forthcoming papers: in forthcoming papers:
WX Psc O, Mira, OH/IR R Gem S, Mira OH 26.5+0.6 O, Mira, OH/IR
IK Tau O, Mira OH 127.8+0.0 O, Mira, OH/IR R Sct O, RVa
TX Cam O, Mira IRC +50049 O, SRb W Aql S, Mira
RX Boo O, SRb CRL 292 O, SR? RR Aql O, Mira
X Her O, SRb α Ori O, SRc CRL 2494 C, Mira
CRL 2362 O, OH/IR IRAS 06192+4657 C, ? T Cep O, Mira
χ Cyg S, Mira UU Aur C, SRb CRL 3068 C, Mira
V Cyg C, Mira BM Gem C?, SRb LP And C, Mira
S Cep C, Mira R LMi O, Mira TX Psc C, Lb
OH 104.9+2.4 O, OH/IR R Leo O, Mira He 3-1475 O, e-pAGB
R Cas O, Mira CIT-6 C, Mira IRAS 19500-1709 C, e-pAGB
IRAS 19475+3119 C?, e-pAGB V Hya C, SRa IRAS 22223+4327 C, e-pAGB
IRAS 20028+3910 ?, e-pAGB RT Vir O, SRb OH 17.7-2.0 O, e-pAGB?, OH/IR
IRAS 21282+5050 C, e-pAGB R Hya O, Mira
IRAS 23321+6545 C, e-pAGB S CrB O, Mira
CRL 2477 C, e-pAGB? V CrB C, Mira

Notes. The sources were selected to cover the large diversity of AGB and early post-AGB (e-pAGB) types. When known, we specify the chemical type (O, C and S), the variability type if they are variable sources [Mira, semiregular (SRa, SRb, SRc or SR?), RV Tauri variable (RVa) or irregular (Lb)], and other relevant characteristics, as if they are OH/IR, early post-AGB sources (e-pAGB) or unclassified (?).

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