The article 'The Structure of the Young Star Cluster NGC 6231. I Stellar Population', Kuhn et al. 2017 fits a Maschberger (2013) IMF modified with a completeness function:
The 50% mass is a free parameter, but I'm not sure if w is also a free parameter.
The article 'The Structure of the Young Star Cluster NGC 6231. I Stellar Population', Kuhn et al. 2017 fits a Maschberger (2013) IMF modified with a completeness function:
The 50% mass is a free parameter, but I'm not sure if
wis also a free parameter.