Table 3
Mid-IR fluxes for new candidate LBVs and BHGs.
| Name | Class. | [3.6] | [4.5] | [5.8] | [8.0] |
|
|
|||||
| UIT005 | BHG | 16.46 | 16.35 | – | – |
| [HS80] B133 | BHG | 16.33 | 16.20 | – | – |
| IFM-B 1330 | BHG | 15.96 | 15.95 | – | – |
|
|
|||||
| M 33 Var B | LBV | 15.65 | 15.53 | 14.82 | 13.20 |
| N93351 | iron star | 13.30 | 12.64 | 11.67 | 10.60 |
| N125093 | iron star | 12.36 | 11.73 | 11.05 | 10.00 |
| Romano’s star | LBV | 14.95 | 14.76 | 14.72 | 14.74 |
|
|
|||||
| 013235.25+303017.6 | iron star | 16.32 | 15.87 | – | – |
| 013242.26+302114.1 | iron star | 13.70 | 13.61 | – | 13.18 |
| 013309.14+302328.4 | Ofpe/WN9 | 17.32 | 17.01 | – | – |
| 013350.92+303936.9 | iron star | 10.99 | 11.08 | – | 11.40 |
| 013355.96+304530.6 (=B324) | YHG? | 12.74 | 12.52 | – | – |
| 013357.73+301714.2 | BHG | 16.74 | 16.53 | – | – |
| 013416.44+303120.8 | BHG | 16.61 | 16.66 | – | – |
Notes. Top panel: fluxes from the catalogue of Thompson et al. (2009), middle panel: fluxes from Valeev et al. (2009, priv. comm.) and bottom panel: fluxes from the McQuinn et al. (2007). Note that the values from McQuinn et al. (2007) have not been subject to correction due to a systematic offset with those of Thompson et al. (2009), while the former do not provide [5.8] mag. Classifications given follow the ammended morphological scheme of Ma07, noting that Massey et al. (1996) associate 013350.92+303936.9 (=UIT218) with the galactic nucleus; hence it is likely that it is a composite source.
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