|8 kpc||distance to Galactic bulge|
|most abundant type of star|
|km s-1 at kpc|
|*||10-3||Jupiter/Sun mass ratio|
|*||wide separation caustic|
|*||10-2||Moon/Earth mass ratio|
|*||planetary Einstein radius|
|*||brightness requirements vs. stellar abundance|
|*||20 mmag||typical value in past observations|
Notes. Parameters marked with an asterisk (*) are varied in our simulations in order to evaluate their influence on the lunar detection rate and to compare different triple-lens scenarios. The fixed parameters lead to values for the Einstein ring radius, mas, i.e. 1.9 AU in the lens plane, and the Einstein time, days. The lensed system is a Saturn-mass planet at a projected separation of 2.5 AU from its M-dwarf host, the Earth-mass satellite orbits the planet at 0.06 AU, i.e. 0.01 mas angular separation, cf. Fig. 10.
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