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Table 6

Individual distances, ages, and metallicities for SMC Cepheids.

Cepheid log P Agea Distance Distance Uncertainty on [Fe/H]
(d) (Myr) (MIR) (pc) (NIR) (pc) NIR distances (pc) (dex)

HV 817 1.277 212.4 57 502 55 636c 1136 –0.79
HV 823 1.504 186.9 60 770b 964 –0.77
HV 824 1.819 161.2 56 700 51 195c 957 –0.70
HV 829 1.926 154.2 55 506 53 625c 964 –0.73
HV 834 1.867 157.9 57 420 60 463c 1168 –0.60
HV 837 1.631 175.5 60 752 57 692c 1033 –0.80
HV 847 1.433 194.2 63 160 60 129b 1175 –0.72
HV 865 1.523 185.2 54 586 58 401c 1018 –0.84
HV 1365 1.094 239.7 71 595 68 986b 1094 –0.79
HV 1954 1.222 219.8 54 265 57 702b 1027 –0.73
HV 2064 1.527 184.7 65 503 58 973c 1182 –0.61
HV 2195 1.621 176.3 58 568 58 703c 1163 –0.64
HV 2209 1.355 202.8 56 286 56 543b 1006 –0.62
HV 11211 1.330 205.8 54 140 53 884c 966 –0.80

HV 822 1.224 219.6 67 447 64 428b 1022 –0.70
HV 1328 1.200 223.0 61 750 61 526b 976 –0.63
HV 1333 1.212 221.2 69 244 69 002b 1094 –0.86
HV 1335 1.158 229.3 69 493 68 231b 1214 –0.78

Notes. Metallicities from Romaniello et al. (2008) have been put on the same metallicity scale (by adding 0.03 dex to them) as our data.

(a)

Period-age relation from Bono et al. (2005).

(b)

Distance based on IRSF/SIRIUS near-infrared photometry (Kato et al. 2007).

(c)

Distance based on 2MASS near-infrared photometry (Skrutskie et al. 2006).

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