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<ri:Resource created="2025-12-23T10:55:31Z" status="active" updated="2026-03-02T06:25:50Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>TEQUILA catalog of TESS images variables</title><shortName>J/A+A/704/A317</shortName><identifier>ivo://CDS.VizieR/J/A+A/704/A317</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Ogunwale B.B.</name></creator><creator><name>Zaguri Y.</name></creator><creator><name>Perdelwitz V.</name></creator><creator><name>Voelschow M.</name></creator><creator><name>Azulay S.Y.,Guetta D.</name></creator><creator><name>Tal-Or L.</name></creator><date role="Updated">2026-03-02T06:25:50Z</date><date role="Created">2025-12-23T10:55:31Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>surveys</subject><subject>variable-stars</subject><subject>exoplanets</subject><subject>photometry</subject><subject>visible-astronomy</subject><description>Stellar variability and transient events provide critical insights into many areas of astrophysics. Progress in these fields has been accelerated by high-precision space-based photometry missions such as CoRoT, Kepler, and K2. NASA's ongoing Transiting Exoplanet Survey Satellite (TESS) represents another significant milestone, offering a unique combination of long observational baseline, high cadence, and nearly all-sky coverage. However, extracting high-quality light curves from TESS full-frame images (FFIs) remains challenging due to contamination from scattered light and blending in crowded fields. In this study, we processed TESS FFIs to produce a comprehensive catalog of light curves for variable point sources observed during the satellite's prime mission. The resulting database, TESS Quick-look and Light curve Analysis (TEQUILA), provides over six million light curves. These include stellar variables, transient events, instrumental systematics, and moving objects. The data were obtained using a pipeline based on difference image analysis, construction of high S/N reference frames, and fixed-radius aperture photometry. A convolutional neural network was used to flag systematic noise, and cross-matching with known Solar System objects was performed to identify contamination. All extracted light curves are publicly accessible as a high-level science product through the MAST archive.</description><source format="bibcode">2025A&amp;A...704A.317O</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/704/A317</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/IV/39">IV/39 : TESS Input Catalog version 8.2 (TIC v8.2) (Paegert+, 2021)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL 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