The stellar initial mass function of nearby young moving groups

Open Access

Fig. 3

Resulting K_min,0.99 for all the hyper-parameter combinations as a function of the RPS density threshold $ρ_{ε_{r, v}, N_{min}}$ $Mathematical equation: $\rho_{\varepsilon_{r,v},N_{\text{min}}}$$ corresponding to the hyper-parameter combination. The colour-map for the top and bottom plots indicates the age A and the value of N_min, respectively.

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