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Home All issues Volume 499 / No 2 (May IV 2009) A&A, 499 2 (2009) 541-555 Full HTML
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Table 7:

IRAC and MIPS/24 $\mu $m magnitudes and SED slope ( $\alpha_{[K \& 24~\rm \mu m]}$) for the 10 objects showing IR excess emission at 24 $\mu $m identified in this work.
ID Designation Status$^\wedge$ IRAC/3.6 $\mu $m IRAC/4.5 $\mu $m IRAC/5.8 $\mu $m IRAC/8.0 $\mu $m MIPS/24 $\mu $m $\alpha_{[K_{\rm S} \& 24~\mu \rm m]}$
1 WFI J08403964-5250429 HR-C 14.26 $\pm$ 0.01 14.02 $\pm$ 0.01 14.13 $\pm$ 0.08 14.11 $\pm$ 0.13 11.07 $\pm$ 0.25 -1.63
30 WFI J08404683-5302487 M 15.76 $\pm$ 0.04 15.61 $\pm$ 0.06 15.92 $\pm$ 0.34 15.90 $\pm$ 0.98 10.71 $\pm$ 0.18 -0.89
31 WFI J08410019-5249088 IR-C 12.46 $\pm$ 0.01 12.54 $\pm$ 0.01 12.47 $\pm$ 0.02 12.39 $\pm$ 0.04 10.31 $\pm$ 0.14 -2.07
7 WFI J08410886-5248387 HR-C, X 12.32 $\pm$ 0.01 12.21 $\pm$ 0.01 12.22 $\pm$ 0.02 12.10 $\pm$ 0.03 11.42 $\pm$ 0.47 -2.45
32 WFI J08412176-5247289 M 15.58 $\pm$ 0.03 15.59 $\pm$ 0.05 15.26 $\pm$ 0.23 16.88 $\pm$ 1.60 11.41 $\pm$ 0.32 -1.44
33 WFI J08412550-5300154$^\dag $ IR-C 15.88 $\pm$ 0.05 15.93 $\pm$ 0.06 - - 10.54 $\pm$ 0.17 -0.96
34 WFI J08413601-5309274 M 12.35 $\pm$ 0.01 12.24 $\pm$ 0.01 12.14 $\pm$ 0.02 12.17 $\pm$ 0.03 11.44 $\pm$ 0.30 -2.46
35 WFI J08413888-5259492 IR-C 13.70 $\pm$ 0.01 13.58 $\pm$ 0.02 13.28 $\pm$ 0.05 12.95 $\pm$ 0.06 9.86 $\pm$ 0.09 -1.34
36 WFI J08414904-5255192 IR-C 14.07 $\pm$ 0.02 13.83 $\pm$ 0.02 13.44 $\pm$ 0.06 13.03 $\pm$ 0.06 10.20 $\pm$ 0.15 -1.26
37 WFI J08415780-5252140 M 10.18 $\pm$ 0.01 10.22 $\pm$ 0.01 10.17 $\pm$ 0.01 10.10 $\pm$ 0.01 9.73 $\pm$ 0.15 -2.71
$^\wedge$ M = confirmed cluster member; HR-C = member candidate according to the location on the HR diagram; X = X-ray sources (Marino et al. 2005); IR-C: young stellar object candidate according to the IR properties (Sect. 6.1).
$^\dag $ Flux at 5.8 and 8 $\mu $m not available.

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