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## (from tabmap V6.0 (2016-08-18)) 2024-04-27T10:41:57 #--------------------------------------------------------------------------- #-- J/AcA/65/297 OGLE4 LMC and SMC Cepheids (Soszynski+, 2015) #-------------------------------------------------------------------------- #---Table: J/AcA/65/297/./lremarks.dat LMC remarks on selected objects (138 records) # Star A17 --- Star's ID # Rem A90 --- Remark ------------------------------------------------------------------------------------------------------------ Star |Rem -----------------|------------------------------------------------------------------------------------------ OGLE-LMC-CEP-0016|uncertain (possible spotted star) OGLE-LMC-CEP-0086|secondary period of 1.270830 d OGLE-LMC-CEP-0093|secondary period of 1.353821 d OGLE-LMC-CEP-0133|secondary period of 0.845056 d OGLE-LMC-CEP-0145|secondary period of 1.537832 d OGLE-LMC-CEP-0227|Cepheid in an eclipsing binary system (P_ecl = 309.67 d) OGLE-LMC-CEP-0245|blended with an eclipsing binary OGLE-LMC-CEP-0248|secondary period of 235.85 d OGLE-LMC-CEP-0251|secondary period of 5.054590 d OGLE-LMC-CEP-0265|secondary period of 1.455312 d OGLE-LMC-CEP-0323|secondary period of 1.360213 d OGLE-LMC-CEP-0385|variable mean magnitude, uncertain OGLE-LMC-CEP-0399|secondary period of 1.738535 d OGLE-LMC-CEP-0403|secondary period of 1.036039 d OGLE-LMC-CEP-0420|secondary period of 1.107464 d OGLE-LMC-CEP-0470|secondary period of 1.167109 d OGLE-LMC-CEP-0571|double F+1O Cepheid (3.079937 d + 2.100885 d) OGLE-LMC-CEP-0581|secondary period of 1.220420 d OGLE-LMC-CEP-0661|secondary period of 0.930945 d OGLE-LMC-CEP-0735|secondary period of 0.731049 d OGLE-LMC-CEP-0835|double F+F Cepheid (4.562781 d + 2.750956 d) OGLE-LMC-CEP-0839|secondary period of 1.367447 d OGLE-LMC-CEP-0855|secondary period of 1.148557 d OGLE-LMC-CEP-0864|secondary period of 1.179959 d OGLE-LMC-CEP-0898|secondary period of 1.409056 d OGLE-LMC-CEP-0911|secondary period of 1.302005 d OGLE-LMC-CEP-0953|secondary period of 1.509901 d OGLE-LMC-CEP-0988|secondary period of 1.472886 d OGLE-LMC-CEP-1005|secondary period of 1.277487 d OGLE-LMC-CEP-1178|secondary period of 0.996140 d OGLE-LMC-CEP-1228|Blazhko modulation OGLE-LMC-CEP-1346|secondary period of 1.526727 d OGLE-LMC-CEP-1388|blended with an eclipsing binary OGLE-LMC-CEP-1451|secondary period of 4.238725 d OGLE-LMC-CEP-1456|secondary period of 3.194786 d OGLE-LMC-CEP-1501|secondary period of 1.539345 d OGLE-LMC-CEP-1546|Blazhko modulation OGLE-LMC-CEP-1583|blended OGLE-LMC-CEP-1583|blended with a semiregular variable OGLE-LMC-CEP-1654|secondary period of 1.248006 d OGLE-LMC-CEP-1669|secondary period of 1.015097 d OGLE-LMC-CEP-1696|secondary period of 1.239824 d OGLE-LMC-CEP-1714|secondary period of 4.014613 d OGLE-LMC-CEP-1718|two 1O Cepheids in an eclipsing binary system (P_orb = 412.81 d) OGLE-LMC-CEP-1752|secondary period of 1.402031 d OGLE-LMC-CEP-1759|secondary period of 1.254016 d OGLE-LMC-CEP-1771|secondary period of 2.234512 d OGLE-LMC-CEP-1775|uncertain (blue color) OGLE-LMC-CEP-1812|Cepheid in an eclipsing binary system (P_ecl = 551.80 d) OGLE-LMC-CEP-1883|blended with an eclipsing binary OGLE-LMC-CEP-1919|secondary period of 3.914967 d OGLE-LMC-CEP-1952|secondary period of 4.477278 d OGLE-LMC-CEP-1971|secondary period of 1.257087 d OGLE-LMC-CEP-1978|secondary period of 1.914286 d OGLE-LMC-CEP-1987|secondary period of 1.916752 d OGLE-LMC-CEP-2011|secondary period of 2.631025 d OGLE-LMC-CEP-2049|secondary period of 2.784902 d OGLE-LMC-CEP-2095|secondary period of 0.990178 d OGLE-LMC-CEP-2103|uncertain (possible RR Lyrae star) OGLE-LMC-CEP-2113|decreasing mean brightness OGLE-LMC-CEP-2137|secondary period of 6.139489 d OGLE-LMC-CEP-2199|secondary period of 4.105259 d OGLE-LMC-CEP-2221|secondary period of 1.170687 d OGLE-LMC-CEP-2277|secondary period of 2.727828 d OGLE-LMC-CEP-2518|secondary period of 1.514218 d OGLE-LMC-CEP-2532|Cepheid in an eclipsing binary system (P_ecl = 800.42 d) OGLE-LMC-CEP-2557|secondary period of 1.302607 d OGLE-LMC-CEP-2570|secondary period of 1.279060 d OGLE-LMC-CEP-2575|Blazhko modulation OGLE-LMC-CEP-2597|secondary period of 1.190747 d OGLE-LMC-CEP-2618|secondary period of 1.336584 d OGLE-LMC-CEP-2658|secondary period of 1.581913 d OGLE-LMC-CEP-2685|secondary period of 1.342091 d OGLE-LMC-CEP-2690|secondary period of 1.327033 d OGLE-LMC-CEP-2705|Blazhko modulation OGLE-LMC-CEP-2717|secondary period of 1.239302 d OGLE-LMC-CEP-2720|secondary period of 1.429809 d OGLE-LMC-CEP-2735|secondary period of 1.349672 d OGLE-LMC-CEP-2824|blended with an eclipsing binary OGLE-LMC-CEP-2850|secondary period of 1.222117 d OGLE-LMC-CEP-2855|secondary period of 1.298924 d OGLE-LMC-CEP-2860|secondary period of 0.964544 d OGLE-LMC-CEP-2887|blended with an eclipsing binary OGLE-LMC-CEP-2887|secondary period of 0.888676 d (blended eclipsing binary or doubled third-overtone period) OGLE-LMC-CEP-2923|secondary period of 1.480801 d OGLE-LMC-CEP-2935|secondary period of 1.115720 d OGLE-LMC-CEP-2955|secondary period of 1.216449 d OGLE-LMC-CEP-2996|variable mean magnitude OGLE-LMC-CEP-3062|secondary period of 1.800731 d OGLE-LMC-CEP-3072|re-classified mode of pulsation F -> 1O OGLE-LMC-CEP-3103|secondary period of 1.359575 d OGLE-LMC-CEP-3149|Blazhko modulation OGLE-LMC-CEP-3231|secondary period of 1.081143 d OGLE-LMC-CEP-3356|uncertain (possible RR Lyrae star) OGLE-LMC-CEP-3362|secondary period of 0.406684 d OGLE-LMC-CEP-3397|uncertain OGLE-LMC-CEP-3432|secondary period of 2.384126 d OGLE-LMC-CEP-3478|uncertain OGLE-LMC-CEP-3518|variable mean magnitude OGLE-LMC-CEP-3569|re-classified RR Lyrae star (OGLE-LMC-RRLYR-04426) OGLE-LMC-CEP-3600|secondary period of 1.103459 d OGLE-LMC-CEP-3617|secondary period of 1.558783 d OGLE-LMC-CEP-3656|secondary period of 7.077141 d OGLE-LMC-CEP-3682|secondary period of 1.147572 d OGLE-LMC-CEP-3716|secondary period of 1.263220 d OGLE-LMC-CEP-3782|additional eclipsing variability (P_orb = 242.72 d) OGLE-LMC-CEP-3983|secondary period of 1.089230 d OGLE-LMC-CEP-3985|secondary period of 6.835737 d OGLE-LMC-CEP-4085|secondary period of 1.006233 d OGLE-LMC-CEP-4101|secondary period of 2.192723 d OGLE-LMC-CEP-4172|secondary period of 1.383279 d OGLE-LMC-CEP-4177|secondary period of 1.368360 d OGLE-LMC-CEP-4207|uncertain (small amplitude) OGLE-LMC-CEP-4212|secondary period of 1.415390 d OGLE-LMC-CEP-4216|uncertain OGLE-LMC-CEP-4217|secondary period of 2.928026 d OGLE-LMC-CEP-4231|secondary period of 1.557814 d OGLE-LMC-CEP-4245|secondary period of 0.912733 d OGLE-LMC-CEP-4268|secondary period of 1.238119 d OGLE-LMC-CEP-4300|uncertain OGLE-LMC-CEP-4339|secondary period of 1.510622 d OGLE-LMC-CEP-4372|secondary period of 1.148559 d OGLE-LMC-CEP-4373|secondary period of 1.280685 d OGLE-LMC-CEP-4397|secondary period of 1.371106 d OGLE-LMC-CEP-4404|secondary period of 6.056935 d OGLE-LMC-CEP-4412|secondary period of 0.766201 d OGLE-LMC-CEP-4420|secondary period of 1.176133 d OGLE-LMC-CEP-4441|secondary period of 1.080978 d OGLE-LMC-CEP-4450|secondary period of 0.922890 d OGLE-LMC-CEP-4467|secondary period of 1.355785 d OGLE-LMC-CEP-4473|uncertain OGLE-LMC-CEP-4477|Blazhko modulation OGLE-LMC-CEP-4482|secondary period of 0.653573 d OGLE-LMC-CEP-4505|secondary period of 1.468983 d OGLE-LMC-CEP-4506|Cepheid in an eclipsing binary system (P_ecl = 1550.4 d) OGLE-LMC-CEP-4562|uncertain OGLE-LMC-CEP-4567|uncertain OGLE-LMC-CEP-4677|uncertain ------------------------------------------------------------------------------------------------------------