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<ri:Resource created="2020-12-15T09:45:53Z" status="active" updated="2025-06-13T15:25:00Z" 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>BVRI photom. of DV Psc and known short-period EBs</title><shortName>J/ApJ/877/75</shortName><identifier>ivo://CDS.VizieR/J/ApJ/877/75</identifier><altIdentifier>doi:10.26093/cds/vizier.18770075</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Pi Q.-F.</name></creator><creator><name>Zhang L.-Y.</name></creator><creator><name>Bi S.-L.</name></creator><creator><name>Han X.L.</name></creator><creator><name>Lu H.-P.</name></creator><creator><name>Yue Q.</name></creator><creator><name>Long L.</name></creator><creator><name>Yan Y.</name></creator><date role="Updated">2021-03-29T12:26:21Z</date><date role="Created">2020-12-15T09:45:53Z</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>infrared-photometry</subject><subject>visible-astronomy</subject><subject>Wide-band photometry</subject><subject>stellar-flares</subject><subject>stellar-spectral-types</subject><description>Using 27 sets of new multiband photometry light curves acquired from our long-term photometric campaign carried out in the last 5yr and high-resolution spectroscopic data from seven nights, we analyzed the physical mechanisms of period variation, starspot cycle, optical flares, and chromospheric activities of the eclipsing binary DV Psc. Our updated O-C diagram covering a period of approximately 20yr shows an oscillation in its orbital period. This variations might be caused by a third body with an orbital period of 14.58+/-0.28yr. There are two active regions of starspots at longitude belts of about 90{deg} and 270{deg}. We obtained its starspot cycles with periods of 3.60+/-0.03yr and 3.42+/-0.02yr at about 90{deg} and 270{deg}, respectively. Moreover, the magnitude difference of Max.I-Max.II shows cyclic oscillation of 5.15+/-0.01yr. During our decade long photometric campaign, we observed DV Psc a total of 326.4hr, detected 18 outbursts (12 of them have never been reported) with flare energies in the range of (6.62-1106.85)x10^24^J. The slope of the relationship between the phase of the max flare and spots is 0.842 +/-0.083, implying a correlation between spots and flares. We discovered evidence for a correlation between the rotation period and the activity cycle for the short-period eclipsing binaries. Our high-resolution spectroscopic observations of DV Psc show obvious emissions above continuum in the H{alpha} line and small self-reversal emissions of the CaII IRT lines.</description><source format="bibcode">2019ApJ...877...75P</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/877/75</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/AJ/108/268">J/AJ/108/268 : HK survey emission-line candidates positions (Beers+ 1994)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/285/459">J/A+A/285/459 : RZ Dra (Kreiner+ 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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>Type</name><description>Cycle type ("Single" or "Complex"=multi-cycles)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column><column><name>ID</name><description>Identifier</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="13*">char</dataType></column><column><name>SpType</name><description>Spectral type</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType" arraysize="12*">char</dataType></column><column><name>EBs</name><description>Eclipsing binary type (1)</description><ucd>src.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>PRot</name><description>[0.06/8] Rotational period</description><unit>d</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_PRot</name><description>[0/30]? Uncertainty in the last digits of PRot</description><unit>d</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>P1</name><description>[1/181] First period</description><unit>yr</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_P1</name><description>[1/90]? Uncertainty in P1</description><unit>yr</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>P2</name><description>[1.8/88.4]? Second period; if available</description><unit>yr</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_P2</name><description>[1/90]? Uncertainty in P2</description><unit>yr</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>P3</name><description>[2/22.8]? 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