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

Figure 3

(a) Time variation of the amplification for a microlensing event (, ) with linear LDC () (continuous line) and with four-parameter nonlinear power law (, , , and ) (dashed line). (b) The residual curve between the two curves is shown. The time is given in units of the Einstein time of the event.

(a)

(b)