----------------------------------------------------------- log M/Msun all ages <0.3 Myr 0.3-1 Myr 1-3 Myr ----------------------------------------------------------- (all A_V's) ----------------------------------------------------------- -1.3 1 1 0 0 -1.2 6 5 1 0 -1.1 4 3 0 1 -1.0 54 36 3 15 -0.9 109 63 10 36 -0.8 112 72 12 22 -0.7 145 87 24 29 -0.6 138 57 48 27 -0.5 92 22 57 9 -0.4 69 6 35 18 -0.3 29 5 11 9 -0.2 34 4 18 6 -0.1 27 4 6 5 0.0 26 6 7 7 0.1 29 4 8 8 0.2 17 3 3 2 0.3 18 1 6 4 0.4 25 1 8 9 0.5 6 0 3 2 0.6 9 -- -- -- 0.7 4 -- -- -- 0.8 2 -- -- -- 0.9 2 -- -- -- 1.0 0 -- -- -- 1.1 1 -- -- -- 1.2 2 -- -- -- 1.3 1 -- -- -- 1.4 0 -- -- -- 1.5 1 -- -- -- 1.6 0 -- -- -- 1.7 1 -- -- -- 1.8 0 -- -- -- 1.9 0 -- -- -- 2 0 -- -- -- ----------------------------------------------------------- (A_V < 2 mag only) ----------------------------------------------------------- -1.3 1 1 0 0 -1.2 6 5 1 0 -1.1 4 3 0 1 -1.0 51 33 3 15 -0.9 99 54 9 36 -0.8 90 53 11 20 -0.7 99 51 19 24 -0.6 96 38 35 17 -0.5 70 16 43 7 -0.4 39 2 20 7 -0.3 19 2 6 9 -0.2 19 2 9 4 -0.1 15 2 3 3 0.0 14 2 4 5 0.1 12 1 4 4 0.2 7 0 2 2 0.3 13 1 2 4 0.4 16 1 3 6 0.5 5 0 2 2 0.6 2 -- -- -- 0.7 3 -- -- -- 0.8 1 -- -- -- 0.9 2 -- -- -- 1.0 0 -- -- -- 1.1 1 -- -- -- 1.2 1 -- -- -- 1.3 1 -- -- -- 1.4 0 -- -- -- 1.5 1 -- -- -- 1.6 0 -- -- -- 1.7 1 -- -- -- 1.8 0 -- -- -- 1.9 0 -- -- -- 2.0 0 -- -- -- ----------------------------------------------------------- ----------------------------------------------------------- The derived mass distribution is ~100% complete above ~1 M_sun and ~60% complete below ~1 M_sun. The shift in the peak of the mass distribution with age is likely due to the lack of inclusion of an appropriate initial mass-radius relationship in the evolutionary tracks.