Analysis of 204 lensed quasars yields mean source crossing time of 2.59 years, Einstein radius crossing time of 11.29 years, average quasar half-light radius of 5.4 light-days, microlens mass fraction lower limit of 0.15, and 9% probability of high-magnification events.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
years
2026 2verdicts
UNVERDICTED 2representative citing papers
Forward modeling of synthetic debris disc images demonstrates that recovered scattering phase functions are biased by observational limits and do not directly reflect intrinsic dust properties.
citing papers explorer
-
Microlensing time-scales and flux magnification probabilities of a sample of 204 lensed quasars
Analysis of 204 lensed quasars yields mean source crossing time of 2.59 years, Einstein radius crossing time of 11.29 years, average quasar half-light radius of 5.4 light-days, microlens mass fraction lower limit of 0.15, and 9% probability of high-magnification events.
-
What you see is not necessarily what you get: Interpreting near-infrared scattering phase functions of debris discs
Forward modeling of synthetic debris disc images demonstrates that recovered scattering phase functions are biased by observational limits and do not directly reflect intrinsic dust properties.