<?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>Variability-selected Intermediate-mass Black Hole Candidates in Dwarf Galaxies from ZTF and WISE</dc:title><dc:creator>Ward, Charlotte; Gezari, Suvi; Nugent, Peter; Bellm, Eric C.; Dekany, Richard; Drake, Andrew; Duev, Dmitry A.; Graham, Matthew J.; Kasliwal, Mansi M.; Kool, Erik C.; Masci, Frank J.; Riddle, Reed L.</dc:creator><dc:corporate_author/><dc:editor/><dc:description>Abstract                          While it is difficult to observe the first black hole seeds in the early universe, we can study intermediate-mass black holes (IMBHs) in local dwarf galaxies for clues about their origins. In this paper we present a sample of variability-selected active galactic nuclei (AGN) in dwarf galaxies using optical photometry from the Zwicky Transient Facility (ZTF) and forward-modeled mid-IR photometry of time-resolved Wide-field Infrared Survey Explorer (WISE) co-added images. We found that 44 out of 25,714 dwarf galaxies had optically variable AGN candidates and 148 out of 79,879 dwarf galaxies had mid-IR variable AGN candidates, corresponding to active fractions of 0.17% ± 0.03% and 0.19% ± 0.02%, respectively. We found that spectroscopic approaches to AGN identification would have missed 81% of our ZTF IMBH candidates and 69% of our WISE IMBH candidates. Only nine candidates have been detected previously in radio, X-ray, and variability searches for dwarf galaxy AGN. The ZTF and WISE dwarf galaxy AGN with broad Balmer lines have virial masses of 10              5              M              ⊙              &lt;              M              BH              &lt; 10              7              M              ⊙              , but for the rest of the sample, BH masses predicted from host galaxy mass range between 10              5.2              M              ⊙              &lt;              M              BH              &lt; 10              7.25              M              ⊙              . We found that only 5 of 152 previously reported variability-selected AGN candidates from the Palomar Transient Factory in common with our parent sample were variable in ZTF. We also determined a nuclear supernova fraction of 0.05% ± 0.01% yr              −1              for dwarf galaxies in ZTF. Our ZTF and WISE IMBH candidates show the promise of variability searches for the discovery of otherwise hidden low-mass AGN.</dc:description><dc:publisher/><dc:date>2022-09-01</dc:date><dc:nsf_par_id>10423983</dc:nsf_par_id><dc:journal_name>The Astrophysical Journal</dc:journal_name><dc:journal_volume>936</dc:journal_volume><dc:journal_issue>2</dc:journal_issue><dc:page_range_or_elocation>104</dc:page_range_or_elocation><dc:issn>0004-637X</dc:issn><dc:isbn/><dc:doi>https://doi.org/10.3847/1538-4357/ac8666</dc:doi><dcq:identifierAwardId>2034437</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>