Table A.1.
Sample for which a period analysis and LC fitting was performed.
RA | Dec | Names | Object type | Spectral type | Gaia type | Spitzer type |
---|---|---|---|---|---|---|
(deg) | (deg) | |||||
4.876441 | −72.465755 | 2MASS J00193036−7227567 | Can. AGB | MIRA_SR | ||
5.993721 | −73.631895 | OGLE SMC-LPV-190, 2MASS J00235849−7337548 | Mira | |||
6.088240 | −72.107443 | |||||
6.498306 | −73.895774 | OGLE SMC-LPV-367 2MASS J00255959−7353448 | Mira | |||
6.795538 | −73.408413 | OGLE SMC-LPV-486 2MASS J00271093−7324303 | Mira | |||
7.329711 | −71.063852 | IRAS F00271-7120 2MASS J00291916−7103499 | C | C | ||
7.572240 | −72.472302 | OGLE SMC-LPV-881 2MASS J00301737−7228202 | Mira | MIRA_SR | ||
7.669748 | −73.712530 | OGLE SMC-LPV-929 2MASS J00304075−7342450 | Mira | |||
7.917060 | −73.798217 | |||||
7.987056 | −73.520435 | |||||
8.051002 | −74.801395 | OGLE SMC-LPV-1168 2MASS J00321227−7448049 | Mira | |||
8.117008 | −71.789106 | 2MASS J00322809−7147207 | Can. AGB | |||
8.442051 | −72.749582 | 2MASS J00334612−7244584 | Can. AGB | |||
8.511784 | −72.363404 | 2MASS J00340283−7221482 | Can. AGB | MIRA_SR | ||
8.816105 | −73.424329 | OGLE SMC-LPV-1690 2MASS J00351587−7325275 | Mira | |||
8.931123 | −73.352948 | LIN 19 2MASS J00354347−7321106 | Em | |||
8.955451 | −74.127210 | 2MASS J00354932−7407381 | Star | |||
9.108186 | −73.432101 | |||||
9.164485 | −72.274068 | 2MASS J00363946−7216266 | Can. AGB | |||
9.193053 | −73.526474 | MSX SMC 029 2MASS J00364631−7331351 | PAGB | C | C (1) CPAGB (2) CPAGB (3) | |
9.230702 | −74.741285 | |||||
9.236272 | −72.421530 | MSX SMC 091 2MASS J00365671−7225175 | C | C (1) CAGB (2) CAGB (3) | ||
9.246025 | −71.636344 | [FBR2002] J003659−713813 | Radio | |||
9.328809 | −72.284239 | 2MASS J00371893−7217031 | Can. AGB | |||
9.384601 | −73.506030 | OGLE J003732.32−733021.3 2MASS J00373232−7330216 | LPV | |||
9.387759 | −72.879192 | 2MASS J00373306−7252451 | Can. AGB | |||
9.446274 | −73.650656 | RAW 21 2MASS J00374710−7339022 | C | C | ||
9.466017 | −69.829967 | |||||
9.491884 | −75.208617 | [KID97] C0036−7529 2MASS J00375807−7512309 | C | |||
9.507699 | −73.790561 | OGLE J003801.87−734725.7 2MASS J00380186−7347259 | Mira | |||
9.614211 | −74.260202 | OGLE SMC-LPV-2488 2MASS J00382740−7415366 | Mira | |||
9.660904 | −72.008445 | 2MASS J00383862−7200304 | Can. AGB | MIRA_SR | ||
9.794922 | −71.569425 | |||||
9.828878 | −70.131865 | [MH95] 414 2MASS J00391894−7007546 | C | C | MIRA_SR | |
9.887294 | −70.295891 | |||||
10.067795 | −73.020987 | OGLE J004016.25−730115.1 2MASS J00401627−7301156 | Mira | |||
10.137255 | −73.477785 | OGLE J004032.93−732839.7 2MASS J00403293−7328399 | Mira | |||
10.147153 | −73.324740 | OGLE J004035.31−731928.7 2MASS J00403531−7319291 | Mira |
Notes. Column 1 lists the coordinates (right ascension and declination) of the source in decimal degrees. Column 2 gives some names, as listed by the SIMBAD database. A “?” indicates the name of a source that is located close to the nominal position. Column 3 gives the object type, as listed by the SIMBAD database (As of January 2019. As the SIMBAD database is continuously updated this may change in time). Column 4 gives the spectral type(s), as listed in Skiff (2014). In case of many entries only a selection is listed. Column 5 gives the variable star classification as listed in the GDR2 Gaia Collaboration (2018), Holl et al. (2018). Column 6 gives the classification based on the MIR Spitzer IRS spectra. The full table is available at the CDS.
References. (1) Groenewegen & Sloan (2018); (2) Kraemer et al. (2017); (3) Ruffle et al. (2015); (4) Jones et al. (2017); (5) Seale et al. (2009); (6) Sloan et al. (2016) (all stars listed as “C” in Groenewegen & Sloan 2018, also listed in Sloan et al. 2016); (7) Woods et al. (2011). The classifications are taken directly from those papers. For the exact meaning of the abbreviations see the original papers.
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