Table 5.
Optical photometric parameters for all the 339 LMC and SMC T2Cs analysed in this work.
| ID | RA | Dec | Class | P | σP | ⟨V⟩ | ⟨I⟩ | epochI | A(I) | ⟨G⟩ | σ⟨G⟩ | ⟨GBP⟩ | σ⟨GBP⟩ | ⟨GRP⟩ | σ⟨GRP⟩ | Source | SOS | VI |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| (deg) | (deg) | (days) | (days) | (mag) | (mag) | (days) | (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) |
| DR3_4687428801808318208 | 16.12685 | −72.61781 | RVTau | 60.100 | 0.100 | – | – | 1529.710 | – | 15.158 | 0.002 | 15.380 | 0.005 | 14.673 | 0.007 | Gaia | 1 | P22;P22 |
| OGLE-LMC-T2CEP-016 | 73.94154 | −69.12951 | RVTau | 20.305 | 0.002 | 15.883 | 15.454 | 7008.381 | 0.166 | 15.794 | 0.009 | 15.930 | 0.007 | 15.488 | 0.008 | OGLE | 1 | OGLE;OGLE |
| OGLE-LMC-T2CEP-017 | 74.06676 | −68.271 | WVir | 14.456 | 0.002 | – | 15.995 | 7014.267 | 0.856 | 16.730 | 0.010 | 17.140 | 0.050 | 16.060 | 0.030 | OGLE | 1 | P22;OGLE |
| OGLE-LMC-T2CEP-018 | 74.62422 | −69.40808 | BLHer | 1.380 | 0.001 | 18.634 | 17.959 | 7000.813 | 0.615 | 18.498 | 0.007 | 18.560 | 0.070 | 18.000 | 0.020 | OGLE | 1 | OGLE;OGLE |
| OGLE-LMC-T2CEP-019 | 74.70599 | −68.07435 | pWVir | 8.673 | 0.001 | 16.850 | 15.989 | 7002.910 | 0.633 | 16.665 | 0.007 | 16.860 | 0.010 | 15.960 | 0.050 | OGLE | 1 | OGLE;OGLE |
| OGLE-SMC-T2CEP-15 | 12.40383 | −73.16708 | BLHer | 2.570 | 0.001 | 17.189 | 16.884 | 7002.500 | 0.172 | 17.181 | 0.003 | 17.253 | 0.006 | 16.900 | 0.010 | OGLE | 1 | OGLE;OGLE |
Notes. Columns: (1) Identification from OGLE IV or Gaia; (2) and (3) RA and Dec; (4) class: BLHer = BLHerculis (T2C); RVTau = RV Tauri (T2C); WVir = W Virginis (T2C); pWVir = peculiar W Virginis (T2C); (5) period; (6) period error; (7) magnitude in I band from OGLE; (8) magnitude in V band from OGLE; (9) epoch; (10) amplitude in the I band; (11) and (12) magnitude in G and relative uncertainty; (13) and (14) as for Cols. (11) and (12) but for the GBP; (15) and (16) as for Cols. (11) and (12) but for the GRP; (17) flag indicating the source used for identification; (18) flag indicating how the Gaia magnitudes have been calculated; (19) flag indicating what is the origin of the V I magnitude. 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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