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Table 2:

Adopted age, spectral type range, $f_{\rm acc}$ and $f_{\rm IRAC}$ (when available) in Figs. 3 and 4.

Cluster 		Age Sp.T range $f_{\rm acc}$ $f_{\rm IRAC}$ Age ref. $f_{\rm acc}$ ref. $f_{\rm IRAC}$ ref.
  [Myr]   [%] [%]      
rho Oph 1 K0-M4 50 $\pm$ 16   M05 M05  
Taurus 1.5 K0-M4 59 $\pm$ 9 62 M05 M05 Ha05
NGC 2068/71 2 K1-M5 61 $\pm$ 9 70 FM08 FM08 FM08
Cha I 2 K0-M4 44 $\pm$ 8 52-64 Lu08 M05 Lu08
IC348 2.5 K0-M4 33 $\pm$ 6 47 L06 M05 L06
NGC 6231 3 K0-M3 15 $\pm$ 5   S07 this work  
$\sigma$ Ori 3 K4-M5 30 $\pm$ 17 35 C08 this work He07
Upper Sco 5 K0-M4 7 $\pm$ 2 19 C06 M05 C06
NGC 2362 5 K1-M4 5 $\pm$ 5 19 D07 D07 D07
NGC 6531 7.5 K4-M4 8 $\pm$ 5   P01 this work  
$\eta$ Cha 8 K4-M4 27 $\pm$ 19 50 S09 JA06 S09
TWA 8 K3-M5 6 $\pm$ 6   D06 JA06  
NGC 2169 9 K5-M6 0+3   JE07 JE07  
25 Ori 10 K2-M5 6 $\pm$ 2   B07 B07  
NGC 7160 10 K0-M1 2 $\pm$ 2 4 SA06 SA05 SA06
ASCC 58 10 K0-M5 0+5   K05 this work  
$\beta$ Pic 12 K6-M4 0+13   ZS04 JA06  
NGC 2353 12 K0-M4 0+6   K05 this work  
Collinder 65 25 K0-M5 0+7   K05 this work  
Tuc-Hor 27 K1-M3 0+8   ZS04 JA06  
NGC 6664 46 K0-M1 0+4   S82 this work  

References.  Schmidt (1982, S82), Park et al. (2001, P01), Hartmann et al. (2005, Ha05), Kharchenko et al. (2005, K05), Mohanty et al. (2005, M05), Sicilia-Aguilar et al. (2005, SA05), Carpenter et al. (2006, C06), Lada et al. (2006, L06), Jayawardhana et al. (2006, JA06), Sicilia-Aguilar et al. (2006, SA06), Dahm & Hillenbrand (2007, D07), Briceño et al. (2007, B07), Jeffries et al. (2007, JE07), Hernández et al. (2007, He07), Sana et al. (2007, S07), Caballero (2008, C08), Flaherty & Muzerolle (2008, FM08), Luhman et al. (2008, L08), Sicilia-Aguilar et al. (2009, S09), Zuckerman & Song (2004, ZS04).


Source LaTeX | All tables | In the text

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