Table 3
Details of the SED fit parameters.
| SST GC No. | Model | Ndata | Nfits |
|
⟨ AV ⟩ (mag) | ⟨ log 10(L⋆) ⟩ (L⊙) | ⟨ Teff ⟩ (K) | ⟨ M⋆ ⟩ (M⊙) | AVmap (mag) |
|
|
|||||||||
| 238110 | spubhmia | 8 | 2 | 96.7 | 20.5 ± 0.4 | 4.4 ± 0.0 | 8329 ± 936 | 20.0 ± 5.0 | 25.5 ± 1.1 |
| 352034 | sp–s-ib | 7 | 329 | 1.1 | 22.8 ± 2.4 | 3.7 ± 0.4 | 6668 ± 2213 | 12.4 ± 3.8 | 45.0 ± 11.3 |
| 358063 | sp–s-ib | 8 | 45 | 30.1 | 20.3 ± 0.3 | 3.7 ± 0.1 | 9091 ± 979 | 9.4 ± 1.5 | 32.3 ± 5.8 |
| 373107 | sp–h-ic | 8 | 9 | 104.5 | 24.8 ± 0.6 | 4.1 ± 0.0 | 10524 ± 499 | 15.0* | 31.7 ± 5.1 |
| 388790 | spubsmid | 7 | 13 | 0.9 | 22.2 ± 1.2 | 3.7 ± 0.2 | 6946 ± 1255 | 12.7 ± 2.9 | 43.0 ± 12.4 |
| 395315 | spubsmid | 5 | 91 | 1.9 | 24.2 ± 3.5 | 3.2 ± 0.2 | 9397 ± 3981 | 7.8 ± 2.0 | 34.3 ± 4.2 |
| 405235 | spu-smie | 7 | 1 | 32.7 | 20.0 | 3.9 | 6671 | 15.0+ | 37.5 ± 2.5 |
| 609669 | spubsmid | 7 | 132 | 8.6 | 22.8 ± 2.7 | 3.3 ± 0.2 | 9932 ± 3436 | 8.2 ± 1.7 | 26.7 ± 2.6 |
Notes. For each source represented by their SST GC No., average values of parameters from the model set corresponding to the best fit SED with the lowest 
value are chosen and listed. The errors or uncertainties for parameters are roughly determined from the standard deviation in mass from all fits. The last column shows the AV values from the extinction map of Schultheis et al. (2009) within 2′ of each source. (∗) Only one closest stellar track to source position (see Fig. 8) from all SED fits of the chosen model set. (+) Only one SED fit to the observed photometry by the chosen model set.
A complex model in which the central star with a disk, a variable disk inner radius, and bipolar cavities are enclosed in a rotationally flattened envelope structure surrounded by ambient interstellar medium.
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