📝 SummarXiv

Abstract

We present monitoring observations of quasar microlensing in the quadruple quasar HE0435-1223. The microlensing-induced light curves of the quasar images are chromatic, i.e. they depend on the applied filter band. Comparison with microlensing simulations allows us to infer properties of the accretion disk. We determine the R and V band light curves of the four images of HE0435-1223 from 79 and 80 epochs respectively, taken from 2014 to 2024 at the Las Cumbres Observatory using difference imaging analysis. We consider difference light curves to remove the intrinsic quasar variability. This reveals a prominent long-term chromatic microlensing event in image B. We use microlensing light curve simulations with both Gaussian and standard thin accretion disk brightness profiles to analyse this signal. The particularly strong signal observed in image B of HE0435-1223 makes it possible to detect a size ratio of the accretion disk in the R band compared to the V band of $1.24^{+0.08}_{-0.20}$ and $1.42^{+0.11}_{-0.22}$ for the Gaussian and the thin disk model, respectively. These values are in agreement with standard thin disk theory. For the absolute size we find large disk half-light radii of around 0.7 to 1.0 Einstein radii with an uncertainty of about 0.6 dex (depending on the filter bands and the models). Finally, our calculations show that image B undergoes caustic crossings about once per year.