<?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 Sub-kiloparsec Active Galactic Nuclei (VODKA): Very Long Baseline Array Searches for Dual or Off-nucleus Quasars and Small-scale Jets</dc:title><dc:creator>Chen, Yu-Ching; Liu, Xin; Lazio, Joseph; Breiding, Peter; Burke-Spolaor, Sarah; Hwang, Hsiang-Chih; Shen, Yue; Zakamska, Nadia L.</dc:creator><dc:corporate_author/><dc:editor/><dc:description>&lt;title&gt;Abstract&lt;/title&gt; &lt;p&gt;Dual and off-nucleus active supermassive black holes are expected to be common in the hierarchical structure formation paradigm, but their identification at parsec scales remains a challenge due to strict angular resolution requirements. We conducted a systematic study using the Very Long Baseline Array (VLBA) to examine 23 radio-bright candidate dual and off-nucleus quasars. The targets are selected by a novel astrometric technique (&lt;italic&gt;varstrometry&lt;/italic&gt;) from Gaia, aiming to identify dual or off-nucleus quasars at (sub)kiloparsec scales. Among these quasars, eight exhibit either multiple radio components or significant (&gt;3&lt;italic&gt;σ&lt;/italic&gt;) positional offsets between the VLBA and Gaia positions. The radio emission from the three candidates, which exhibit multiple radio components, is likely to originate from small-scale jets based on their morphology. Among the remaining five candidates with significant VLBA-Gaia offsets, three are identified as potential dual quasars at parsec scales, one is likely attributed to small-scale jets, and the origin of the last candidate remains unclear. We explore alternative explanations for the observed VLBA-Gaia offsets. We find no evidence for optical jets at kiloparsec scales, nor any contamination to Gaia astrometric noise from the host galaxy; misaligned coordinate systems are unlikely to account for our offsets. Our study highlights the promise of the varstrometry technique in discovering candidate dual or off-nucleus quasars and emphasizes the need for further confirmation and investigation to validate and understand these intriguing candidates.&lt;/p&gt;</dc:description><dc:publisher>AAS Jounals</dc:publisher><dc:date>2023-11-01</dc:date><dc:nsf_par_id>10473890</dc:nsf_par_id><dc:journal_name>The Astrophysical Journal</dc:journal_name><dc:journal_volume>958</dc:journal_volume><dc:journal_issue>1</dc:journal_issue><dc:page_range_or_elocation>29</dc:page_range_or_elocation><dc:issn>0004-637X</dc:issn><dc:isbn/><dc:doi>https://doi.org/10.3847/1538-4357/ad00b3</dc:doi><dcq:identifierAwardId>2108162; 2020265</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>