<?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>Redder than Red: Discovery of an Exceptionally Red L/T Transition Dwarf</dc:title><dc:creator>Schneider, Adam C.; Burgasser, Adam J.; Bruursema, Justice; Munn, Jeffrey A.; Vrba, Frederick J.; Caselden, Dan; Kabatnik, Martin; Rothermich, Austin; Sainio, Arttu; Bickle, Thomas P.; Dahm, Scott E.; Meisner, Aaron M.; Kirkpatrick, J. Davy; Suárez, Genaro; Gagné, Jonathan; Faherty, Jacqueline K.; Vos, Johanna M.; Kuchner, Marc J.; Williams, Stephen J.; Gagliuffi, Daniella Bardalez; Aganze, Christian; Hsu, Chih-Chun; Theissen, Christopher; Cushing, Michael C.; Marocco, Federico; Casewell, Sarah</dc:creator><dc:corporate_author/><dc:editor/><dc:description>&lt;title&gt;Abstract&lt;/title&gt; &lt;p&gt;We present the discovery of CWISE J050626.96+073842.4 (CWISE J0506+0738), an L/T transition dwarf with extremely red near-infrared colors discovered through the Backyard Worlds: Planet 9 citizen science project. Photometry from UKIRT and CatWISE give a (&lt;italic&gt;J&lt;/italic&gt;−&lt;italic&gt;K&lt;/italic&gt;)&lt;sub&gt;MKO&lt;/sub&gt;color of 2.97 ± 0.03 mag and a&lt;italic&gt;J&lt;/italic&gt;&lt;sub&gt;MKO&lt;/sub&gt;− W2 color of 4.93 ± 0.02 mag, making CWISE J0506+0738 the reddest known free-floating L/T dwarf in both colors. We confirm the extremely red nature of CWISE J0506+0738 using Keck/NIRES near-infrared spectroscopy and establish that it is a low-gravity, late-type L/T transition dwarf. The spectrum of CWISE J0506+0738 shows possible signatures of CH&lt;sub&gt;4&lt;/sub&gt;absorption in its atmosphere, suggesting a colder effective temperature than other known, young, red L dwarfs. We assign a preliminary spectral type for this source of L8&lt;italic&gt;γ&lt;/italic&gt;–T0&lt;italic&gt;γ&lt;/italic&gt;. We tentatively find that CWISE J0506+0738 is variable at 3–5&lt;italic&gt;μ&lt;/italic&gt;m based on multiepoch WISE photometry. Proper motions derived from follow-up UKIRT observations combined with a radial velocity from our Keck/NIRES spectrum and a photometric distance estimate indicate a strong membership probability in the&lt;italic&gt;β&lt;/italic&gt;Pic moving group. A future parallax measurement will help to establish a more definitive moving group membership for this unusual object.&lt;/p&gt;</dc:description><dc:publisher>The Astrophysical Journal Letters</dc:publisher><dc:date>2023-01-31</dc:date><dc:nsf_par_id>10468215</dc:nsf_par_id><dc:journal_name>The Astrophysical Journal Letters</dc:journal_name><dc:journal_volume>943</dc:journal_volume><dc:journal_issue>2</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/acb0cd</dc:doi><dcq:identifierAwardId>2009177; 2009136</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>