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Table 3
Estimated [3.6] completeness limits and corresponding stellar masses for given extinction values.
Image area | Good detectionsb in | Good detectionsb in | Good detectionsb in | ||||||||
4 bands | 3 adjacent lowest bands | 2 adjacent lowest bands | |||||||||
|
|||||||||||
Naked | Class | Naked | Class | Naked | Class | Naked | Class | ||||
PMS | II | PMS | II | PMS | II | PMS | II | ||||
[3.6] | M | M | [3.6] | M | M | [3.6] | M | M | M | M | |
(mag) | (M⊙) | (M⊙) | (mag) | (M⊙) | (M⊙) | (mag) | (M⊙) | (M⊙) | (M⊙) | (M⊙) | |
AV = 5.5 mag | AV = 5.5 mag | AV = 5.5 mag | AV = 10−20 mag | ||||||||
|
|||||||||||
Faint diffuse emission | 10.25 | 6–10 | 2.5 | 11.75 | 3 | 1.5 | 12.25 | 2 | 1 | – | – |
Intense diffuse emissiona | – | – | – | – | – | – | 10.75 | – | – | ~6–10 | ~2.5–3 |
Notes.
(a)
Completeness limits unreliable when requiring good detections in more than two bands (see Appendix C);
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