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Table 3

Effect of dust on the colours of CCs.

Name Teff (K) L (L) BIC Bp (mag) G (mag) Rp (mag) V (mag) I (mag) J (mag) K (mag) F160W (mag) WG (mag) WVI (mag) WJK (mag) WH (mag)
LMC0619 4625 48057 ± 1645 2809 12.37 11.71 11.12 12.27 10.97 10.18 9.45 9.67 9.34 8.96 8.95 9.18
4750 45036 ± 946 713 12.42 11.79 11.20 12.30 11.06 10.30 9.60 9.81 9.47 9.14 9.12 9.35
Tc = 535 ± 26 K −0.05 −0.08 −0.08 −0.03 −0.09 −0.12 −0.15 −0.14 −0.13 −0.18 −0.17 −0.17
LMC1616 4875 4026 ± 85 752 14.88 14.30 13.75 14.78 13.62 12.92 12.28 12.47 12.15 11.82 11.84 12.03
4875 4185 ± 91 614 14.93 14.34 13.77 14.81 13.64 12.91 12.25 12.45 12.14 11.83 11.79 12.01
Tc = 329 ± 40 K −0.05 −0.04 −0.02 −0.03 −0.02 +0.01 +0.03 +0.02 +0.01 −0.01 +0.05 +0.02
LMC0966 5000 21971 ± 379 971 12.99 12.44 11.92 12.89 11.79 11.13 10.54 10.71 10.41 10.08 10.13 10.29
5000 21876 ± 387 885 13.02 12.46 11.92 12.90 11.80 11.14 10.55 10.71 10.37 10.10 10.14 10.29
Tc = 417 ± 125 K −0.03 −0.02 +0.00 −0.01 −0.01 −0.01 −0.01 +0.00 +0.04 −0.02 −0.01 +0.00
SMC1172 5250 4960 ± 83 214 14.97 14.50 14.02 14.89 13.89 13.31 12.79 12.93 12.69 12.34 12.43 12.55
5500 5958 ± 182 130 14.96 14.52 14.05 14.87 13.94 13.30 12.77 12.93 12.79 12.50 12.40 12.58
Tc = 90 ± 7 K +0.01 −0.02 −0.03 +0.02 −0.05 +0.01 +0.02 +0.00 −0.10 −0.16 +0.03 −0.03
LMC0107 5750 3834 ± 31 55 14.89 14.46 14.01 14.81 13.89 13.35 12.92 13.04 12.79 12.46 12.62 12.69
5875 4047 ± 39 60 14.88 14.46 14.01 14.79 13.90 13.36 12.94 13.06 12.81 12.52 12.65 12.73
Tc = 217 ± 28 K +0.01 +0.00 +0.00 +0.02 −0.01 −0.01 −0.02 −0.02 −0.02 −0.06 −0.03 −0.04
LS Pup 5500 4395 ± 152 3436 10.49 9.76 9.11 10.39 8.94 8.08 7.43 7.67 7.14 6.69 6.98 7.13
5750 4364 ± 153 2752 10.55 9.81 9.15 10.45 8.97 8.05 7.40 7.65 7.15 6.68 6.95 7.10
Tc = 3620 ± 1182 K −0.06 −0.05 −0.04 −0.06 −0.03 +0.03 +0.03 +0.02 −0.01 +0.01 +0.03 +0.03

Notes. For every star the first line gives the best-fitting parameters based on the model atmosphere, the second line when including a dust component, and the third line the difference in magnitude. In the column of the luminosity the dust temperature at the inner radius (Tc) is listed in the third line. W refers to the Wesenheit magnitudes, defined as follows: WG = G – 1.90 • (BpRp), WVI = I – 1.55 • (VI), WJK = K – 0.69 • (JK), WH = F160W −0.386 • (F555W – F814W). Note that F555W and F814W magnitudes are not explicitly listed in the table (they are close to V and I) but were calculated and used in calculating the WH magnitude.

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