Table 2
Comparison of the two source classification methods.
| Method A: sub-mm | ||||||
| Method B: | Protostel. | Starless | Undet. | |||
| mid-IR | 195 | 44 | 4006 | |||
|
|
||||||
| Protostel.449 | PS[2] | 100 | Undet. | 6 | PS[1] | 343 |
| including | ||||||
| − Class 0 | 3 | 0 | 7 | |||
| − Class I | 56 | 2 | 131 | |||
| − Class II | 41 | 4 | 205 | |||
|
|
||||||
| Starless1384 | PS[1] | 11 | SL[2] | 14 | SL[1] | 1359 |
|
|
||||||
| Undet.2412 | PS[1] | 84 | SL[1] | 24 | Undet. | 2304 |
Notes. The columns give the classification obtained using submillimetre data (method A, see Sect. 4.4.1). The rows give the classification obtained using mid-IR data (method B, see Sect. 4.4.2). The final categories are protostellar (PS), starless (SL) and undetermined (Undet.). Numbers in brackets are quality flags; other numbers are the number of sources falling simultaneously in the row/column categories.
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