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<ri:Resource created="2025-12-04T12:31:36Z" status="active" updated="2026-08-03T07:26:00Z" 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>O'Connell effect in contact binaries. I.</title><shortName>J/ApJS/276/25</shortName><identifier>ivo://CDS.VizieR/J/ApJS/276/25</identifier><altIdentifier>doi:10.26093/cds/vizier/bb-8m-s</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Kleftogiannis G.D.</name></creator><creator><name>Christopoulou P.-E.</name></creator><creator><name>Papageorgiou A.</name></creator><date role="Updated">2026-08-03T07:26:00Z</date><date role="Created">2025-12-04T12:31:36Z</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>eclipsing-binary-stars</subject><subject>variable-stars</subject><subject>surveys</subject><subject>photometry</subject><subject>visible-astronomy</subject><description>Asymmetries between the two maxima of the light curves of contact binaries, known as the O'Connell effect, have been identified using the All Sky Automated Survey, All-Sky Automated Survey for Supernovae, Northern Sky Variability Survey, Optical Gravitational Lensing Experiment, and Optical Monitoring Camera sky surveys. The morphology of the mean light curve has been analyzed for a total of 43659 objects already classified as contact binaries. After applying several filters and criteria, we present a sample of 797 systems representing the largest sample to date of maxima asymmetries of EW-type binaries with |{Delta}m| up to 0.13 mag. We also added information on distance and temperature from Gaia DR3 and The Large Sky Area Multi-Object Fiber Spectroscopic Telescope. We investigated the statistical distributions of periods, temperatures, signs of maximum asymmetry, O'Connell effect ratio and light-curve asymmetry indices of asymmetry, and their correlations. While starspots could explain the different maxima asymmetries in stars with convection zones and differential rotations, the discovery of sizeable asymmetric maxima in 161 early-type systems above the upper limit of the Kraft break (T&gt;6700K) may indicate a different mechanism. We also report systems with peculiar unequal maxima.</description><source format="bibcode">2025ApJS..276...25K</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/276/25</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/II/287">II/287 : Northern Sky Variability Survey (NSVS) (Wozniak+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/264">II/264 : ASAS Variable Stars in Southern hemisphere (Pojmanski+, 2002-2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/366">II/366 : ASAS-SN catalog of variable stars (Jayasinghe+, 2018-2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/357">I/357 : Gaia DR3 Part 3. 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>ID</name><description>System Name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="28*">char</dataType></column><column><name>Flag</name><description>Flag (1)</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>RAJ2000</name><description>Right Ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Per</name><description>[0.2/1.9] Period</description><unit>d</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Nobs</name><description>[77/3100] Number of observations</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Delm</name><description>[-0.13/0.1] Difference in magnitude between two maxima, {Delta}m</description><unit>mag</unit><ucd>phot.mag;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Delm/Afit</name><description>[-0.09/0.12] Ratio, Delm to amplitude, |{Delta}m|/A_fit_</description><ucd>src.var.amplitude;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>DeltaI</name><description>Normalized flux, {Delta}I</description><ucd>phot.flux;arith.ratio;em.opt.I</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>OER</name><description>[0.499/1.88] O'Connell Effect Ratio indicator of asymmetry, equation 3</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>LCA</name><description>[0.007/0.31] LC Asymmetry indicator of asymmetry, equation 4</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>OName</name><description>Other name</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="29*">char</dataType></column><column><name>ASASSN</name><description>Display data from ASAS-SN (II/366) within 1.5"</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>ASAS3</name><description>Display data from ASAS (II/264) within 10"</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>NSVS</name><description>Display data from NSVS (Hoffman+ 2009, J/AJ/138/466) within 10.5"</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>OGLE</name><description>Display data from OGLE (Udalski+ 1998, J/AcA/48/563; Wyrzykowski+ 2003, J/AcA/53/1; Graczyk+ 2011, J/AcA/61/103; Pawlak+ 2013, J/AcA/63/323 and Pietrukowicz+ 2013, J/AcA/63/115) within 3"</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>SimbadName</name><description>Simbad column added by the CDS</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="29*">char</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>