Fig. 11
Testing different IMFs. The (B − V)T distributions correspond to the (top) entire Galactic plane | b | < 10, (middle) entire stripe of the sky at 10 < | b | ≤ 30, and (bottom) the stripe of the sky at 30 < | b | ≤ 90. In dotted orange line the simulations, which are obtained with the default model A (Haywood-Robin IMF); in solid blue line we have the default model B (Kroupa-Haywood v6 IMF), and the default model combined with the best fit SFR and IMF from Just & Jahreiß (2010) is in dash-dotted magenta line. The Tycho-2 data is in dashed green line.
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