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Table 3

Normalized flux densities of the median SED, upper SED (fourth quartile) and lower SED (first quartile) of the Class II objects in Cha I and Cha II, after extinction correction.

λ (μm) Median transitional Median Upper Lower Detections
(Fλ arbitrary units)

R 1.01 0.79 1.00 0.38 32
I 1.22 1.02 1.34 0.74 32
J 1.00 1.00 1.00 1.00 107
H 0.67 0.67 0.72 0.61 107
Ks 0.35 0.38 0.45 0.32 107
IRAC 3.6 7.1e-2 0.10 0.15 7.5e-2 78
IRAC 4.5 3.2e-2 5.5e-2 8.5e-2 4.0e-2 70
IRAC 5.8 2.0e-2 3.0e-2 4.5e-2 2.2e-2 86
IRAC 8.0 4.7e-3 1.5e-2 2.7e-2 1.1e-3 78
MIPS 24 3.5e-3 2.5e-3 4.4e-3 1.6e-4 95
PACS 70 1.8e-3 4.2e-4 7.0e-4 3.0e-4 23
PACS 100 6.8e-4 2.5e-4 3.5e-4 1.2e-4 41
PACS 160 3.5e-4 7.7e-5 1.5e-4 5.5e-5 19
SPIRE 250 5.7e-5 5.1e-5 1.2e-4 1.3e-5 9
SPIRE 350 1.9e-5 2.9e-5 7.5e-5 2.8e-6 9
SPIRE 500 5.2e-6 9.1e-6 2.3e-5 6.3e-7 7

Notes. Transitional disks are not included. The number of stars detected in each band is also indicated. For comparison, we also include the median value for the six transitional disks detected in this study, although we stress its very low number statistics.

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