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xmlns:vodm="http://www.ivoa.net/xml/DataModel/v1" xmlns:voe="http://www.ivoa.net/xml/VOEventRegExt/v2" xmlns:vosi10="http://www.ivoa.net/xml/VOSITables/v1.0" xmlns:vot="http://www.ivoa.net/xml/VOTable/v1.2" xmlns:vot0="http://www.ivoa.net/xml/VOTable/v1.3" xmlns:vot1="http://www.ivoa.net/xml/VOTable/v1.1" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vr0="https://www.ivoa.net/xml/VOResource/v1.0" xmlns:vr1="http://www.ivoa.net/xml/VOResource/v1.1" xmlns:vr2="http://Www.ivoa.net/xml/VOResource/v1.0" xmlns:vr3="http://www.ivoa.net/xml/VOResource/v1%20.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:vs0="http://www.ivoa.net/xml/VODataService/v1.0" xmlns:vs1="https://www.ivoa.net/xml/VODataService/v1.0" xmlns:vstd="http://www.ivoa.net/xml/StandardsRegExt/v1.0" xmlns:xdtn="http://www.w3.org/2004/07/xpath-datatypes" xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:xlink0="https://www.w3.org/1999/xlink" xmlns:xsd="http://www.w3.org/2001/XMLSchema" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns:xsi0="https://www.w3.org/2001/XMLSchema-instance" xmlns:xu="http://www.xmldb.org/xupdate"><oai:identifier>ivo://CDS.VizieR/J/MNRAS/516/2736</oai:identifier><oai:datestamp>2025-11-03T00:00:00Z</oai:datestamp><oai:setSpec>J.MNRAS</oai:setSpec></oai:header><oai:metadata><eudc:resource xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns:eudc="http://schema.eudat.eu/schema/kernel-1" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:oai="http://www.openarchives.org/OAI/2.0/" xmlns:dachs="urn:dachs" xsi:schemaLocation="http://schema.eudat.eu/schema/kernel-1           http://docs.g-vo.org/schemata/eudat-core.xsd"><eudc:community>IVOA</eudc:community><eudc:titles><eudc:title>Optical variability of ~700 low mass AGNs</eudc:title></eudc:titles><eudc:descriptions><eudc:description>We present a sample of 706, z &lt; 1.5 active galactic nuclei (AGNs) selected from optical photometric variability in three of the Dark Energy Survey (DES) deep fields (E2, C3, and X3) over an area of 4.64 deg^2^. We construct light curves using difference imaging aperture photometry for resolved sources and non- difference imaging PSF photometry for unresolved sources, respectively, and characterize the variability significance. Our DES light curves have a mean cadence of 7 d, a 6-yr baseline, and a single-epoch imaging depth of up to g ~ 24.5. Using spectral energy distribution (SED) fitting, we find 26 out of total 706 variable galaxies are consistent with dwarf galaxies with a reliable stellar mass estimate (M* &lt; 10^9.5^M_{Sun}_; median photometric redshift of 0.9). We were able to constrain rapid characteristic variability time-scales (~ weeks) using the DES light curves in 15 dwarf AGN candidates (a subset of our variable AGN candidates) at a median photometric redshift of 0.4. This rapid variability is consistent with their low black hole (BH) masses. We confirm the low-mass AGN nature of one source with a high S/N optical spectrum. We publish our catalogue, optical light curves, and supplementary data, such as X-ray properties and optical spectra, when available. We measure a variable AGN fraction versus stellar mass and compare to results from a forward model. This work demonstrates the feasibility of optical variability to identify AGNs with lower BH masses in deep fields, which may be more 'pristine' analogues of supermassive BH seeds.</eudc:description></eudc:descriptions><eudc:keywords><eudc:keyword>black-holes</eudc:keyword><eudc:keyword>galaxies</eudc:keyword><eudc:keyword>dwarf-galaxies</eudc:keyword><eudc:keyword>active-galactic-nuclei</eudc:keyword><eudc:keyword>astrometry</eudc:keyword><eudc:keyword>photometry</eudc:keyword><eudc:keyword>visible-astronomy</eudc:keyword><eudc:keyword>stellar-masses</eudc:keyword><eudc:keyword>redshifted</eudc:keyword><eudc:keyword>spectroscopy</eudc:keyword><eudc:keyword>infrared-astronomy</eudc:keyword><eudc:keyword>x-ray-sources</eudc:keyword><eudc:keyword>interdisciplinary-astronomy</eudc:keyword><eudc:keyword>galactic-and-extragalactic-astronomy</eudc:keyword><eudc:keyword>high-energy-astrophysics</eudc:keyword><eudc:keyword>stellar-astronomy</eudc:keyword><eudc:keyword>cosmology</eudc:keyword><eudc:keyword>observational-astronomy</eudc:keyword></eudc:keywords><eudc:identifiers><eudc:identifier identifierType="URL">https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/MNRAS/516/2736</eudc:identifier></eudc:identifiers><eudc:relatedIdentifiers><eudc:relatedIdentifier relatedIdentifierType="URL">https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/516/2736</eudc:relatedIdentifier><eudc:relatedIdentifier relatedIdentifierType="bibcode">2022MNRAS.516.2736B</eudc:relatedIdentifier><eudc:relatedIdentifier relatedIdentifierType="URL">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/516/2736</eudc:relatedIdentifier><eudc:description>Cone search capability for table J/MNRAS/516/2736/table2 (Variability-selected AGN candidates regardless of stellar mass or variability properties)</eudc:description><eudc:description>Cone search capability for table J/MNRAS/516/2736/table3 (Catalogue of 15 variable AGN candidates with rapid variability log({tau}_DRW_)&lt;1.5)</eudc:description></eudc:relatedIdentifiers><eudc:creators><eudc:creator><eudc:creatorName>Burke C.J.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Liu X.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Shen Y.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Phadke K.A.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Yang Q.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Hartley W.G.,Harrison I.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Palmese A.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Guo H.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Zhang K.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Kron R.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Turner D.J.,Giles P.A.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Lidman C.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Chen Y.-C.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Gruendl R.A.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Choi A.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Amon A.,Sheldon E.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Aguena M.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Allam S.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Andrade-Oliveira F.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Bacon D.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Bertin E.,Brooks D.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Carnero Rosell A.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Carrasco Kind M.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Carretero J.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Conselice C.,Costanzi M.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Da Costa 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D.L.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Honscheid K.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Hoyle B.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>James D.J.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Kuehn K.,Maia M.A.G.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Marshall J.L.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Menanteau F.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Miquel R.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Morgan R.,Paz-Chinchon F.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Pieres A.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Plazas Malagon A.A.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Reil K.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Romer A.K.,Sanchez E.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Schubnell M.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Serrano S.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Sevilla-Noarbe I.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Smith M.,Suchyta E.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Tarle G.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Thomas D.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>To C.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Varga T.N.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Wilkinson R.D.,(The DES Collaboration)</eudc:creatorName></eudc:creator></eudc:creators><eudc:publishers><eudc:publisher>CDS</eudc:publisher></eudc:publishers><eudc:instruments/><eudc:publicationYear>2025</eudc:publicationYear><eudc:rightsList><eudc:rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</eudc:rights></eudc:rightsList><eudc:fundingReferences/><eudc:contacts><eudc:contact>CDS support team &lt;cds-question@unistra.fr&gt;</eudc:contact></eudc:contacts><eudc:resourceTypes><eudc:resourceType>Dataset</eudc:resourceType><eudc:resourceType>AstroObjects</eudc:resourceType></eudc:resourceTypes><eudc:disciplines><eudc:discipline>astronomy</eudc:discipline></eudc:disciplines></eudc:resource></oai:metadata></oai:record></oai:GetRecord></oai:OAI-PMH>