Estimating Finite Source Effects in Microlensing Events due to Free-Floating Planets with the Euclid Survey

Table 1

For different populations of FFPs in the Galactic bulge and thin and thick disks and assuming the mass function index , we give the percentage of expected events in each indicated bin for the magnification peak value.

	1.001, 5	5, 10	10, 15	15, 20	20, 25	25, 30	>30
Bulge	12.25%	1.15%	0.20%	0.30%	0.05%	0.25%	0.05%
Thin disk	7.10%	1.45%	0.40%	0.25%	0.20%	0.05%	0.55%
Thick disk	5.85%	0.80%	0.15%	0.30%	0.20%	0.15%	0.35%