Table 3.
VMC photometric parameters for all the 339 LMC and SMC T2Cs analysed in this work.
| ID | RA | Dec | Class | P | ⟨Y⟩ | σ⟨Y⟩ | A(Y) | σA(Y) | fY | ⟨J⟩ | σ⟨J⟩ | A(J) | σA(J) | fJ | ⟨Ks⟩ | σ⟨Ks⟩ | A(Ks) | σA(Ks) | fKs | E(V − I) | fE(V − I) | Source |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| (deg) | (deg) | (days) | (mag) | (mag) | (mag) | (mag) | (mag) | (mag) | (mag) | (mag) | (mag) | (mag) | (mag) | (mag) | ||||||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) | (12) | (13) | (14) | (15) | (16) | (17) | (18) | (19) | (20) | (21) | (22) | (23) |
| OGLE-SMC-T2CEP-44 | 1.82732 | −74.47599 | RVTau | 22.14387 | 15.094 | 0.002 | 0.57 | 0.01 | f | 14.910 | 0.010 | 0.63 | 0.04 | f | 14.472 | 0.001 | 0.81 | 0.03 | f | 0.040 | 1 | OGLE |
| OGLE-LMC-T2CEP-287 | 95.17501 | −72.52670 | BLHer | 1.344 | 17.650 | 0.010 | 0.35 | 0.01 | t | 17.610 | 0.030 | 0.25 | 0.08 | f | 17.259 | 0.007 | 0.20 | 0.02 | f | 0.102 | 1 | OGLE |
| OGLE-LMC-T2CEP-285 | 94.45717 | −69.76087 | BLHer | 1.050 | 17.900 | 0.020 | 0.44 | 0.03 | f | 17.720 | 0.010 | 0.38 | 0.05 | f | 17.430 | 0.010 | 0.30 | 0.03 | f | 0.093 | 1 | OGLE |
| OGLE-LMC-T2CEP-283 | 94.24198 | −71.51516 | WVir | 9.503 | 15.858 | 0.001 | 0.39 | 0.03 | f | 15.609 | 0.002 | 0.23 | 0.01 | t | 15.131 | 0.004 | 0.23 | 0.01 | f | 0.115 | 1 | OGLE |
| OGLE-LMC-T2CEP-282 | 93.73022 | −67.06919 | pWVir | 6.304 | 16.140 | 0.009 | 0.24 | 0.06 | f | 15.787 | 0.001 | 0.86 | 0.01 | f | 15.621 | 0.005 | 0.24 | 0.03 | f | 0.072 | 1 | OGLE |
Notes. Columns: (1) Identification; (2) and (3) RA and Dec; (4) class of T2C: BLHer = BLHerculis, RVTau = RV Tauri, WVir = W Virginis, pWVir = peculiar W Virginis; (5) period; (6) and (7) intensity-averaged magnitude in Y and relative uncertainty; (8) and (9) peak-to-peak amplitude in Y and relative uncertainty; (10) tag indicating if a fixed value for the amplitude was used to calculate the averaged-intensity magnitude (f = false, t = true); (11)–(15) as for Cols. (6)–(10) but for the J band; (16)–(20) as for Cols. (6)–(10) but for the Ks band; (21) E(V − I) values adopted in this work; (22) flag indicating the origin of the reddening value; (23) flag indicating the source (OGLE IV or Gaia) of period, identification and epoch of maximum. A portion is shown here for guidance regarding its form and content. The machine-readable version of the full table is published at the CDS.
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