Image Details
Caption: Figure 4.
Same as Figure 3, but for the opposite orientation of the caustic, i.e., for ﹩{\theta }_{{\rm{c}}}=270^\circ ﹩. Note that the amplification patterns are independent of the direction of the movement of the caustic. The magnification patterns of Figures 3 and 4 could both run from the left to the right or vice versa.
© 2017. The American Astronomical Society. All rights reserved.