Table A.2.
Literature data.
| RA | Dec | Type | Evo | SpT | Vm | Im | P1 | A1 | P2 | A2 | VC | RC | PR | AR | PB | AB | erBm | erBR | erP | erRm | erBR | erP1 | erAR | Pother | Ref. |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| (deg) | (deg) | (mag) | (mag) | (d) | (mag) | (d) | (mag) | (mag) | (mag) | (d) | (mag) | (d) | (mag) | (mag) | (mag) | (d) | (mag) | (mag) | (d) | (mag) | (d) | ||||
| 4.876441 | −72.465755 | 335 ± 29 | 80 | ||||||||||||||||||||||
| 5.993721 | −73.631895 | Mira | – | – | – | 17.24 | 479 | 1.6 | 175 | 0.1 | |||||||||||||||
| 6.088240 | −72.107443 | ||||||||||||||||||||||||
| 6.498306 | −73.895774 | Mira | – | – | 21.06 | 17.27 | 463 | 1.6 | 306 | 0.4 | |||||||||||||||
| 6.795538 | −73.408413 | Mira | – | – | 20.04 | 16.17 | 457 | 1.3 | 245 | 0.2 | |||||||||||||||
| 7.329711 | −71.063852 | ||||||||||||||||||||||||
| 7.572240 | −72.472302 | Mira | – | – | 18.23 | 15.84 | 508 | 1.6 | 202 | 0.1 | 531 ± 85 | 80 | |||||||||||||
| 7.669748 | −73.712530 | Mira | – | – | 20.77 | 17.80 | 456 | 1.9 | 211 | 0.3 | |||||||||||||||
| 7.917060 | −73.798217 | ||||||||||||||||||||||||
| 7.987056 | −73.520435 | ||||||||||||||||||||||||
| 8.051002 | −74.801395 | Mira | – | – | 20.46 | 17.79 | 495 | 2.0 | 259 | 0.4 | |||||||||||||||
| 8.117008 | −71.789106 | ||||||||||||||||||||||||
| 8.442051 | −72.749582 | ||||||||||||||||||||||||
| 8.511784 | −72.363404 | 336 ± 37 | 80 | ||||||||||||||||||||||
| 8.816105 | −73.424329 | Mira | – | – | 21.97 | 17.82 | 478 | 1.6 | 263 | 0.2 | |||||||||||||||
| 8.931123 | −73.352948 | ||||||||||||||||||||||||
| 8.955451 | −74.127210 | ||||||||||||||||||||||||
| 9.108186 | −73.432101 | ||||||||||||||||||||||||
| 9.164485 | −72.274068 | ||||||||||||||||||||||||
| 9.193053 | −73.526474 | ||||||||||||||||||||||||
| 9.230702 | −74.741285 | ||||||||||||||||||||||||
| 9.236272 | −72.421530 | 405 | 99 | ||||||||||||||||||||||
| 9.246025 | −71.636344 | ||||||||||||||||||||||||
| 9.328809 | −72.284239 | ||||||||||||||||||||||||
| 9.384601 | −73.506030 | SRV | – | – | 21.32 | 18.72 | 573 | 0.5 | 1007 | 0.4 | |||||||||||||||
| 9.387759 | −72.879192 | ||||||||||||||||||||||||
| 9.446274 | −73.650656 | ||||||||||||||||||||||||
| 9.466017 | −69.829967 | ||||||||||||||||||||||||
| 9.491884 | −75.208617 | ||||||||||||||||||||||||
| 9.507699 | −73.790561 | Mira | – | – | 18.87 | 15.63 | 511 | 1.4 | 466 | 0.2 | |||||||||||||||
| 9.614211 | −74.260202 | Mira | – | – | 20.47 | 16.28 | 463 | 1.5 | 2137 | 0.3 | |||||||||||||||
| 9.660904 | −72.008445 | 513 ± 90 | 80 | ||||||||||||||||||||||
| 9.794922 | −71.569425 | ||||||||||||||||||||||||
| 9.828878 | −70.131865 | 343 ± 27 | 80 | ||||||||||||||||||||||
| 9.887294 | −70.295891 | ||||||||||||||||||||||||
| 10.067795 | −73.020987 | Mira | – | – | – | 17.72 | 489 | 1.6 | 305 | 0.1 | |||||||||||||||
| 10.137255 | −73.477785 | Mira | – | – | – | 18.27 | 566 | 2.2 | 897 | 0.2 | |||||||||||||||
| 10.147153 | −73.324740 | Mira | – | – | – | 18.28 | 515 | 1.6 | 612 | 0.2 |
Notes. Column 1 lists the right ascension and declination of the source in decimal degrees. Columns 2−10 are taken from the OGLE-III database of LPVs in the LMC and SMC (Soszyński et al. 2009a, 2011). They list the pulsation type (Mira, SRV, or OSARG) in Col. 2, and for the LMC only, the evolutionary status (AGB or RGB) and spectral type (C or O) in Cols. 3 and 4. Columns 5 and 6 list the mean magnitudes in the V and I bands. Columns 7−10 list the period and amplitude of the primary and secondary period (rounded values are listed, and the OGLE catalogue also lists a tertiary period). Columns 11−16 are taken from the analysis of MACHO data for LPVs in the LMC by Fraser et al. (2008). Mean magnitudes in the V and R bands (in the Cousins system) are listed in Cols. 11 and 12. Period and amplitude in the red and blue band are listed in Cols. 13−16. Columns 17−23 are taken from the analysis of EROS-2 data by Kim et al. (2014) (Cols. 17−19), and Spano et al. (2011) (Cols. 20−23). Listed are the EROS B magnitude, the B − R colour index, and the period and its error (The error is derived from the period and the S/N of the period listed by Kim et al. 2014), respectively, the EROS R magnitude, the B − R colour index, the first fitted period (out of up to five periods listed in Spano et al. 2011), and the amplitude in the R-band. Column 24 lists other periods from the literature, with references listed in Col. 25. The full table is available at the CDS.
References. (34) Wood et al. (1992); (35) Whitelock et al. (2003); (36) Whitelock et al. (1989); (38) Wood et al. (1983); (43) Nishida et al. (2000); (45) Kamath et al. (2010); (80) Holl et al. (2018); (89) present work: re-analysis of the data in ref. (90); (90) Soszyński et al. (2012); (91) Ulaczyk et al. (2013); (92) Hughes (1989); (93) Payne-Gaposchkin (1971); (94) present work: re-analysis of ASAS (Pojmanski 2002) data; (95) Soszyński et al. (2009b); (96) Soszyński et al. (2008a); (97) Soszyński et al. (2008b); (98) Soszyński et al. (2010); (99) Groenewegen & Sloan (2018).
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