Variations in integrated galactic initial mass functions due to sampling method and cluster mass function

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Table 1:

The factor $A_{\rm IGIMF}$ from Eq. (8) for Salpeter and all our IGIMFs.
IGIMF	$A_{\rm IGIMF, Salpeter}$	$A_{\rm IGIMF, Kroupa}$	ratio
Underlying IMF	2610	4090	1.9
Stop nearest	1650	2670	1.62
Stop before	1490
Stop after	1830
Stop 50/50	1710
Analytic	1050
Number	1810
Number unlimited	2610
Sorted sampling	1200	2050	1.71
CMF slope -1.8	2530
CMF slope -3.2	280	450	1.61
CMF slope -4.2	60
Min. cluster mass 1 $M_{\odot }$	1210
Min. cluster mass 50 $M_{\odot }$	2570

Source LaTeX | All tables | In the text

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