cadence, continuously growing light curves from the microlensing surveys of the LMC. Completing the existing Magellanic Quasars Survey fields in the LMC and Small Magellanic Cloud should yield a sample of $\sim$700 well-monitored AGNs, and expanding it to the larger regions covered by the OGLE-IV survey should yield a sample of $\sim$3600 AGNs.'
author:
- 'Szymon Koz[ł]{}owski, C. S. Kochanek, A. M. Jacyszyn, A. Udalski, M. K. Szyma[ń]{}ski, R. Poleski, M. Kubiak, I. Soszy[ń]{}ski, G. Pietrzy[ń]{}ski, [Ł]{}. Wyrzykowski, K. Ulaczyk, and P. Pietrukowicz'
title: 'The Magellanic Quasars Survey. II. Confirmation of [144 ]{}New Active Galactic Nuclei Behind the Southern Edge of the Large Magellanic Cloud'
---

Introduction
============

[@2009ApJ...698..895K], [@2010ApJ...708..927K], and [@2010ApJ...721.1014M] introduced, developed, and applied a new approach to quantitatively modeling the variability of individual quasars, describing the light curves as damped random walks (DRW) characterized by two parameters, a timescale and an amplitude. These parameters are then found to be correlated with the physical properties of the quasar – wavelength, luminosity, and black hole mass. Unfortunately, accurately measuring the parameters of individual quasars requires long ($\gtrsim$decade) well-sampled light curves that are generally not available (see @2011ApJ...728...26M). While this may ultimately be solved by projects such as the Panoramic 