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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);

(b)

a detection with photometric error <0.3 mag is referred to as a good detection.

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