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<ri:Resource created="2025-06-06T13:28:56Z" status="active" updated="2025-08-11T20:18:58Z" 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>CFIS CNN post-merger galaxies catalog</title><shortName>J/MNRAS/514/3294</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/514/3294</identifier><altIdentifier>doi:10.26093/cds/vizier.75143294</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Bickley R.W.</name></creator><creator><name>Ellison S.L.</name></creator><creator><name>Patton D.R.</name></creator><creator><name>Bottrell C.</name></creator><creator><name>Gwyn S.</name></creator><creator><name>Hudson M.J.</name></creator><date role="Updated">2025-08-11T20:18:58Z</date><date role="Created">2025-06-06T13:28:56Z</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>interacting-galaxies</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><subject>photometry</subject><subject>astronomical-object-identification</subject><subject>astrometry</subject><subject>redshifted</subject><subject>stellar-masses</subject><subject>star-forming-regions</subject><subject>classification</subject><description>The importance of the post-merger epoch in galaxy evolution has been well documented, but post-mergers are notoriously difficult to identify. While the features induced by mergers can sometimes be distinctive, they are frequently missed by visual inspection. In addition, visual classification efforts are highly inefficient because of the inherent rarity of post-mergers (~1 per cent in the low-redshift Universe), and non-parametric statistical merger selection methods do not account for the diversity of post-mergers or the environments in which they appear. To address these issues, we deploy a convolutional neural network (CNN) that has been trained and evaluated on realistic mock observations of simulated galaxies from the IllustrisTNG simulations, to galaxy images from the Canada France Imaging Survey, which is part of the Ultraviolet Near Infrared Optical Northern Survey. We present the characteristics of the galaxies with the highest CNN-predicted post-merger certainties, as well as a visually confirmed subset of 699 post-mergers. We find that post-mergers with high CNN merger probabilities [p(x)&gt;0.8] have an average star formation rate that is 0.1 dex higher than a mass- and redshift-matched control sample. The SFR enhancement is even greater in the visually confirmed post-merger sample, a factor of 2 higher than the control sample.</description><source format="bibcode">2022MNRAS.514.3294B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/514/3294</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/MNRAS/486/390">J/MNRAS/486/390 : Morphology of 16908 SDSS Stripe 82 galaxies (Bottrell+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/582/A21">J/A+A/582/A21 : Merging galaxies (mis)alignments (Barrera-Ballesteros+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/130/1516">J/AJ/130/1516 : MCG pairs and triples of galaxies (De Propris+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/221/11">J/ApJS/221/11 : CANDELS visual classifications for GOODS-S (Kartaltepe+,2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/210/3">J/ApJS/210/3 : SDSS bulge, disk and total stellar mass estimates</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/294">II/294 : The SDSS Photometric Catalog, Release 7</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/349">II/349 : The Pan-STARRS release 1 (PS1) Survey - DR1 (Chambers+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource>https://cas.sdss.org/dr7/en/tools/explore/ : SDSS-DR7 explore tool</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/MNRAS/514/3294</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/514/3294</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/514/3294</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/514/3294</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/514/3294</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South 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