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<ri:Resource created="2025-11-19T11:06:20Z" status="active" updated="2026-07-02T11:52:23Z" 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>Kepler stars predicted rotation period: Deep Learning</title><shortName>J/AJ/169/59</shortName><identifier>ivo://CDS.VizieR/J/AJ/169/59</identifier><altIdentifier>doi:10.26093/cds/vizier/be-59-1v</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Kamai I.</name></creator><creator><name>Perets H.B.</name></creator><date role="Updated">2026-07-02T11:52:23Z</date><date role="Created">2025-11-19T11:06:20Z</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>multiple-stars</subject><subject>visible-astronomy</subject><subject>photometry</subject><subject>astronomical-models</subject><description>We propose a new framework to predict stellar properties from light curves. We analyze the light-curve data from the Kepler space mission and develop a novel tool for deriving the stellar rotation periods for main-sequence stars. Using this tool, we provide rotation periods for more than 80K stars. Our model, LightPred, is a novel deep-learning model designed to extract stellar rotation periods from light curves. The model utilizes a dual-branch architecture combining long short-term memory and transformer components to capture temporal and global data features. We train LightPred on self-supervised contrastive pretraining and simulated light curves generated using a realistic spot model. Our evaluation demonstrates that LightPred outperforms classical methods like the autocorrelation function in terms of accuracy and average error. We apply LightPred to the Kepler data set, generating the largest catalog to date. Using error analysis based on learned confidence and consistency metric, we were able to filter the predictions and remove stellar types with variability, which is different than spot-induced variability. Our analysis shows strong correlations between error levels and stellar parameters. Additionally, we confirm tidal synchronization in eclipsing binaries with orbital periods shorter than 10 days. Our findings highlight the potential of deep learning in extracting fundamental stellar properties from light curves, opening new avenues for understanding stellar evolution and population demographics.</description><source format="bibcode">2025AJ....169...59K</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/169/59</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/V/133">V/133 : Kepler Input Catalog (Kepler Mission Team, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/687/1264">J/ApJ/687/1264 : Age estimation for solar-type dwarfs (Mamajek+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/534/A125">J/A+A/534/A125 : Variability of A- and F-stars from Kepler (Uytterhoeven+ 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/775/L11">J/ApJ/775/L11 : Stellar rotation periods for KOIs (McQuillan+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/557/L10">J/A+A/557/L10 : Rotation periods of 12000 Kepler stars (Nielsen+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/560/A4">J/A+A/560/A4 : Rotation periods of active Kepler stars (Reinhold+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/572/A34">J/A+A/572/A34 : Pulsating solar-like stars in Kepler (Garcia+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/572/A34">J/A+A/572/A34 : Pulsating solar-like stars in Kepler (Garcia+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/211/24">J/ApJS/211/24 : Rotation periods of Kepler MS stars (McQuillan+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/149/68">J/AJ/149/68 : A-F type variable stars from Kepler (Bradley+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/801/3">J/ApJ/801/3 : Rotation periods for Q3-Q14 KOIs (Mazeh+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/151/101">J/AJ/151/101 : Kepler Mission. 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