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<ri:Resource created="2024-05-13T07:56:21Z" status="active" updated="2025-05-19T09:50:00Z" 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>Transit depth variability with TESS</title><shortName>J/AJ/167/1</shortName><identifier>ivo://CDS.VizieR/J/AJ/167/1</identifier><altIdentifier>doi:10.26093/cds/vizier.51670001</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Wang G.</name></creator><creator><name>Espinoza N.</name></creator><date role="Updated">2024-11-06T20:19:16Z</date><date role="Created">2024-05-13T07:56:21Z</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>exoplanets</subject><subject>photometry</subject><subject>visible-astronomy</subject><description>The phenomenon of transit depth variability offers a pathway through which processes such as exoplanet atmospheric activity and orbital dynamics can be studied. In this work we conduct a blind search for transit depth variations among 330 known planets observed by the Transiting Exoplanet Survey Satellite within its first four years of operation. Through an automated periodogram analysis, we identify four targets (KELT-8b, HAT-P-7b, HIP 65 Ab, and TrES-3b) that appear to show significant transit depth variability. We find that KELT-8b's transit depth variability likely comes from contaminating flux from a nearby star, while the apparent variabilities of HIP65Ab and TrES-3b are probable artifacts due to their grazing orbits. HAT-P-7b indicates signs of variability that possibly originate from the planet or its host star. A population-level analysis does not reveal any significant correlation between transit depth variability and the effective temperature and mass of the host star; such correlation could arise if stellar activity was the cause of depth variations via the transit light source effect. Extrapolating our ~1% detection rate to the upcoming Roman mission, predicted to yield of order 100000 transiting planets, we expect that ~1000 of these targets will be found to exhibit significant transit depth variability.</description><source format="bibcode">2024AJ....167....1W</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/167/1</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/J/A+A/478/507">J/A+A/478/507 : Distances &amp; atmospheric parameters MSU stars (Morales+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/628/A115">J/A+A/628/A115 : WASP-12, CoRoT-1 and TrES-3 light curves (von Essen+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/259/62">J/ApJS/259/62 : TESS transit timing of hot Jupiters (Ivshina+, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/163/228">J/AJ/163/228 : Limb-darkening coeffi of 176 TESS exoplanets (Patel+, 2022)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/AJ/167/1</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/167/1</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/167/1</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL 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