Discovery of Two Quasars at z=5 from the OGLE Survey

Kozlowski, Szymon; Banados, Eduardo; Udalski, A.; Morrell, N.; Ji, A. P.; Wyrzykowski, L.; Rau, A.; Mroz, P.; Greiner, J.; Gromadzki, M.; Szymanski, M. K.; Soszynski, I.; Poleski, R.; Pietrukowicz, P.; Skowron, J.; Skowron, D. M.; Ulaczyk, K.; Rybicki, K.; Iwanek, P.; Wrona, M.
2019
ASTROPHYSICAL JOURNAL
DOI
10.3847/1538-4357/ab20d1
We used Optical Gravitational Lensing Experiment (OGLE-IV) deep (stacked) images (V less than or similar to 23 mag, I less than or similar to 23 mag at 3 sigma) of the Magellanic System, encompassing an area of similar to 670 deg(2), to perform a search for high-z quasar candidates. We combined the optical OGLE data with the mid-IR Wide-field Infrared Survey Explorer 3.4/4.6/12 mu m data, and devised a multicolor selection procedure. We identified 33 promising candidates and then spectroscopically observed the two most variable sources. We report the discovery of two high-z quasars, OGLE.J015531-752807 at a redshift z = 5.09 and OGLE.J005907-645016.at a redshift of z = 4.98. The variability amplitude of both quasars at the rest-frame wavelength similar to 1300 angstrom is much larger (similar to 0.4 mag) than other quasars (similar to 0.15 mag) at the same rest-frame wavelength but lower redshifts (2 < z < 5). A larger sample of such sources with at least decade-long light curves would be necessary to determine whether increased variability is typical in the population of high-z quasars, or whether we are finding extreme outliers. The Large Synoptic Survey Telescope will provide such light curves for sources 3-4 mag fainter than OGLE.