Table 4
Summary of the overlap between our sample of new candidates and other works.
| Photometric surveys | |||
|
|
|||
| Paper | Cloud | Candidates | Confirmed |
|
|
|||
| Westerlund et al. (1981) | LMC | 39 | 29 |
| Prevot et al. (1983) | SMC | 36 | 33 |
| Massey (2002) | SMC | 8 | 4 |
| Massey (2002) | LMC | 6 | 5 |
| Groenewegen et al. (2009) | SMC | 7 | 5 |
| Groenewegen et al. (2009) | LMC | 4 | 1 |
| Boyer et al. (2011) | SMC | 108 | 99 |
|
|
|||
| Spectroscopic surveys | |||
|
|
|||
| Paper | Cloud | SGs | Other |
|
|
|||
| Elias et al. (1985) | SMC | 18 | 0 |
| Elias et al. (1985) | LMC | 7 | 0 |
| OSK19981 | LMC | 3 | 0 |
| Massey (2003) | SMC | 0 (1) | 7 (6) |
| Buchanan et al. (2006) | LMC | 0 (1) | 0 |
| Neugent et al. (2012) | LMC | 28 | 8 |
Notes. In the upper panel, we show the objects in common with other purely photometric surveys, and the number of them that we have confirmed spectroscopically as SGs. In the lower panel, we perform the comparison for spectroscopic surveys, indicating the number of SGs and other populations in common. In parentheses are indicated those cases in which our classification contradicts that of the original work.
Reference. (1) Oestreicher & Schmidt-Kaler (1998).
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