<?xml version="1.0" encoding="UTF-8"?><rdf:RDF xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:dcq="http://purl.org/dc/terms/"><records count="1" morepages="false" start="1" end="1"><record rownumber="1"><dc:product_type>Journal Article</dc:product_type><dc:title>Varstrometry for Off-nucleus and Dual Subkiloparsec AGN (VODKA). SDSS J1608+2716: A Subarcsecond Quadruply Lensed Quasar at z = 2.575</dc:title><dc:creator>Li, Junyao; Liu, Xin; Shen, Yue; Oguri, Masamune; Gross, Arran C.; Zakamska, Nadia L.; Chen, Yu-Ching; Hwang, Hsiang-Chih</dc:creator><dc:corporate_author/><dc:editor/><dc:description>Abstract                          We report Hubble Space Telescope (HST) Wide Field Camera 3 deep IR (F160W) imaging of SDSS J1608+2716. This system, located at a redshift of              z              = 2.575, was recently reported as a triple-quasar candidate with subarcsecond separations (∼0.″25) based on selection from Gaia astrometry and follow-up Keck adaptive optics–assisted integral field unit spectroscopy. Our new HST deep IR imaging reveals the presence of a fourth point-like component located ∼0.″9 away from the triple system. Additionally, we detect an edge-on disk galaxy located in between the four point sources. The entire system exhibits a characteristic cusp structure in the context of strong gravitational lensing, and the observed image configuration can be successfully reproduced using a lens model based on a singular isothermal ellipsoid mass profile. These findings indicate that this system is a quadruply lensed quasar. Our results highlight the challenges associated with identifying dual/multiple quasars on ∼kiloparsec scales at high redshifts and emphasize the crucial role of deep, high-resolution IR imaging in robustly confirming such systems.</dc:description><dc:publisher/><dc:date>2023-09-01</dc:date><dc:nsf_par_id>10466090</dc:nsf_par_id><dc:journal_name>The Astrophysical Journal Letters</dc:journal_name><dc:journal_volume>955</dc:journal_volume><dc:journal_issue>1</dc:journal_issue><dc:page_range_or_elocation>L16</dc:page_range_or_elocation><dc:issn>2041-8205</dc:issn><dc:isbn/><dc:doi>https://doi.org/10.3847/2041-8213/acf27a</dc:doi><dcq:identifierAwardId>2108162</dcq:identifierAwardId><dc:subject/><dc:version_number/><dc:location/><dc:rights/><dc:institution/><dc:sponsoring_org>National Science Foundation</dc:sponsoring_org></record></records></rdf:RDF>