Statistical Analysis of Caustic Crossings in Multiply Imaged Quasars
Comparison between microlensing on quasars observed and simulated makes it possible to draw conclusions about physical parameters such as source size, quasar brightness profile, mass distribution of the lens, abundance and mass of microlenses, and relative transverse velocity between source and lens. By simulating magnification maps for different
Mediavilla, T. et al.
Fecha de publicación:
0
2012