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Table 1:

The C-star sample: identifiers and pulsation periods for the first few entries.
Names RA Declination Identifier Period Ref. Ampl. (Filter)
IRAS 04496-6958, MSX LMC 1130 72.327000 -69.887361 iras04496 723, 741 1, 18 0.44 (K)
IRAS 05278-6942, MSX LMC 635 81.850458 -69.662472 iras05278 980 9 1.20 (K)
IRAS 00554-7351, [GB98] S16 14.266458 -73.587389 iras00554 720 8 0.72 (K)
MSX LMC 1298, LMC134.1 40407 74.133958 -68.880833 msxlmc1298 683 pp 1.12 (I)
MSX LMC 775, LMC166.2 19640, MACHO 8.8541.68 83.234083 -68.213528 msxlmc775 2067, 2170 pp, pp 1.84 (I), 0.62 (R)

References: pp = present paper ; 1 = Whitelock et al. (2003); 2 = Groenewegen (2004); 3 = Nishida et al. (2000); 4 = Raimondo et al. (2005); 5 = Reid et al. (1988); 6 = Sloan et al. (2006); 7 = Wood (1998); 8 = Dodion (2003); 9 = Wood et al. (2008, in prep.); 10 = Groenewegen et al. (2007), 11 = Hughes (1989); 12 = Whitelock et al. (1994), 13 = Wood et al. (1992); 14 = Lloyd Evans (1985); 15 = Wood et al. (1983, periods actually from Payne-Gaposhkin, 1971); 16 = Cioni et al. (2003); 17 = Sloan et al. (2008); 18 = Fraser et al. (2008); 19 = Pojmanski (2002, ASAS data in general).


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