(1) Department of Physics, University of Toronto, 60 St. George St., Toronto, ON, M5S 1A7, Canada;(2) Department of Astronomy and Astrophysics, University of Toronto, 50 St. George St., Toronto, ON, M5S 3H4, Canada
Abstract:
We set constraints and an upper bound on the masses required for a configuration of n point lenses to produce the maximum of 5n − 5 images of a distant source. We show how this result can be used to detect and constrain the mass of planets or brown
dwarfs in multiple-star systems.