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Table 2.

A summary of our sample of RV Tauri stars in the SMC.

Star RA Dec I (mag) V (mag) P0 (days) Nepochs Ref.
OGLE-SMC-T2CEP-07 00:42:57.49 –73:07:14.8 13.572 14.440 30.961 1015 a
OGLE-SMC-T2CEP-12 00:45:19.69 –73:20:13.7 15.415 16.369 29.219 1020 a
OGLE-SMC-T2CEP-18* 00:51:07.23 –73:41:33.4 14.813 15.627 39.519 710 a,b,c
OGLE-SMC-T2CEP-19 00:53:27.69 –73:38:09.5 14.481 15.064 40.912 710 a
OGLE-SMC-T2CEP-20 00:53:35.98 –72:34:21.8 14.894 15.890 50.623 1033 a
OGLE-SMC-T2CEP-24 00:55:20.55 –73:21:37.9 14.511 15.308 43.961 870 a
OGLE-SMC-T2CEP-29 00:57:38.09 –72:18:12.2 13.648 14.556 33.676 846 a,c
OGLE-SMC-T2CEP-41 01:13:19.05 –73:18:07.8 15.353 16.068 29.118 653 a
OGLE-SMC-T2CEP-43 01:23:53.06 –72:16:45.9 15.398 16.342 23.743 595 a

Notes. Columns 2 and 3 give the position of the stars in the SMC. Columns 4 and 5 display the mean I and V magnitude of each star, respectively. In Col. 6 the fundamental period of each star is shown and Col. 7 represents the number of I-band datapoints available for each star. The stars marked by an asterisk (∗) indicate the ones which have already been studied spectroscopically.

References.

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