A Microlensing Accretion Disk Size Measurement in the Lensed Quasar WFI 2026-4536
arXiv:1911.06218 · doi:10.3847/1538-4357/ab557a
Abstract
We use thirteen seasons of R-band photometry from the 1.2m Leonard Euler Swiss Telescope at La Silla to examine microlensing variability in the quadruply-imaged lensed quasar WFI 2026-4536. The lightcurves exhibit of uncorrelated variability across all epochs and a prominent single feature of within a single season. We analyze this variability to constrain the size of the quasar's accretion disk. Adopting a nominal inclination of 60, we find an accretion disk scale radius of at a rest-frame wavelength of $2043\,\unicode{xC5}$, and we estimate a black hole mass of , based on the CIV line in VLT spectra. This size measurement is fully consistent with the Quasar Accretion Disk Size - Black Hole Mass relation, providing another system in which the accretion disk is larger than predicted by thin disk theory.
arXiv comment26 pages, 8 figures, Appendix with data table, pg 12-25
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