Byun, DoyeeArav, NahumHall, Patrick B.2022-07-182022-07-182022-030004-637X176http://hdl.handle.net/10919/111275We analyze Very Large Telescope/UVES observations of the quasar SDSS J024221.87+004912.6. We identify four absorption outflow systems: a C iv broad absorption line (BAL) at v approximate to -18,000 km s(-1) and three narrower low-ionization systems with centroid velocities ranging from -1200 to -3500 km s(-1). These outflows show similar physical attributes to the [O iii] outflows studied by Liu et al. (2013). We find that two of the systems are energetic enough to contribute to active galactic nucleus feedback, with one system reaching above 5% of the quasar's Eddington luminosity. We also find that this system is at a distance of 67 kpc away from the quasar, the farthest detected mini-BAL absorption outflow from its central source to date. In addition, we examine the time-variability of the BAL and find that its velocity monotonically increases, while the trough itself becomes shallower over time.application/pdfenCreative Commons Attribution 4.0 Internationalkeck hires observationsagn feedbackhst/cos observationsintrinsic fractionionized-gasvlt-uvesemissionaccelerationdynamicsdatabaseArticle - Refereedhttps://doi.org/10.3847/1538-4357/ac503d92721538-4357