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xmlns:cea0="http://www.ivoa.net/xml/CEA/v1.0" xmlns:ceab="http://www.ivoa.net/xml/CEA/base/v1.0" xmlns:ceab0="http://www.ivoa.net/xml/CEA/base/v1.1" xmlns:ceaimpl="http://www.astrogrid.org/schema/CEAImplementation/v2.0" xmlns:ceaimpl0="http://www.astrogrid.org/schema/CEAImplementation/v2.1" xmlns:ceat="http://www.ivoa.net/xml/CEA/types/v1.1" xmlns:ceat0="http://www.ivoa.net/xml/CEA/types/v1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" xmlns:cs0="https://www.ivoa.net/xml/ConeSearch/v1.0" xmlns:dachs="http://docs.g-vo.org/schemata/DaCHS.xsd" xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:doc="http://www.ivoa.net/xml/DocRegExt/v1" xmlns:doc0="http://www.ivoa.net/xml/DocRegExt/v1.0" xmlns:esatapplus="http://esa.int/xml/EsaTapPlus" xmlns:g-colstat="http://dc.g-vo.org/ColStats-1" xmlns:htxs="http://www.helio-vo.eu/xml/HELIO-TAP/v1.0" xmlns:impl="http://www.astrogrid.org/schema/CEAImplementation/v1.0" xmlns:ns1="http://www.astrogrid.org/wsdl/RegistryUpdate/v1.0" 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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/A+A/708/A373</oai:identifier><oai:datestamp>2026-05-19T14:14:26Z</oai:datestamp><oai:setSpec>J.A_A</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>Major merger classification in COSMOS-Web</eudc:title></eudc:titles><eudc:descriptions><eudc:description>Galaxy major mergers are a potential mechanism for triggering active galactic nuclei (AGN) activity, but their role remains debated, particularly beyond the local Universe. We aim to shed light on the merger-AGN connection at z=0.5-2, exploiting the multi-wavelength datasets and James Webb Space Telescope (JWST) observations in the COSMOS field. We construct a stellar mass-limited sample and identify AGN via mid-infrared (MIR) colours, X-ray detections, and spectral energy distribution (SED) fitting. We train convolutional neural networks to identify mergers with mock JWST observations. We create non-AGN and non-merger control samples matching the redshift, stellar mass, and star-formation rate distributions of the AGN and mergers. We find AGN to be moderately more frequent in mergers than in non-mergers, with excess ratios ranging from ~2.5 (X-ray AGN) to ~1.3 (MIR) and ~1.1-1.2 (SED AGN). Similarly, AGN galaxies show a higher merger fraction (f_merg_) than non-AGN controls. We then study f_merg_ as a function of relative and absolute AGN power, utilising the AGN fraction (f_AGN_) and accretion disc luminosity (L_disc_) parameters. We uncover a f_merg_-f_AGN_ relation with two regimes: f_merg_ stays roughly flat for less-dominant AGN (f_AGN_&lt;0.8) but increases at f_AGN_&gt;0.8 for the MIR and X-ray AGN, and more gently for SED AGN, where mergers appear to be the main triggering mechanism. Additionally, f_merg_ increases monotonically as a function of L_disc_, for all AGN types, reaching f_merg_&gt;50% for the most luminous AGN (L_disc_&gt;~10^46^erg/s). Overall, our results suggest that major mergers can trigger AGN out to the cosmic noon at z~2. Furthermore, the role of major mergers shows a clear dependence on AGN luminosity and remains the principal mechanism for fuelling the most powerful AGN.</eudc:description></eudc:descriptions><eudc:keywords><eudc:keyword>galaxies</eudc:keyword><eudc:keyword>catalogs</eudc:keyword><eudc:keyword>redshifted</eudc:keyword><eudc:keyword>stellar-masses</eudc:keyword><eudc:keyword>visible-astronomy</eudc:keyword><eudc:keyword>infrared-astronomy</eudc:keyword><eudc:keyword>cosmology</eudc:keyword><eudc:keyword>stellar-astronomy</eudc:keyword><eudc:keyword>galactic-and-extragalactic-astronomy</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/A+A/708/A373</eudc:identifier></eudc:identifiers><eudc:relatedIdentifiers><eudc:relatedIdentifier relatedIdentifierType="URL">https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/708/A373</eudc:relatedIdentifier><eudc:relatedIdentifier relatedIdentifierType="bibcode">2026A&amp;A...708A.373L</eudc:relatedIdentifier><eudc:relatedIdentifier relatedIdentifierType="URL">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/708/A373</eudc:relatedIdentifier><eudc:description>Cone search capability for table J/A+A/708/A373/catalog (COSMOS Web Master Catalogue z=0.5-2)</eudc:description></eudc:relatedIdentifiers><eudc:creators><eudc:creator><eudc:creatorName>La Marca A.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Margalef-Bentabol B.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Wang L.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Trager S.C.,Rodriguez-Gomez V.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Martin G.</eudc:creatorName></eudc:creator></eudc:creators><eudc:publishers><eudc:publisher>CDS</eudc:publisher></eudc:publishers><eudc:instruments/><eudc:publicationYear>2026</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>