<?xml-stylesheet href='/static/xsl/oai.xsl' type='text/xsl'?>
<ri:Resource created="2017-02-22T12:28:28Z" status="active" updated="2025-05-19T09:50:00Z" 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>I-band light curves of OGLE LMC Miras</title><shortName>J/AJ/152/164</shortName><identifier>ivo://CDS.VizieR/J/AJ/152/164</identifier><altIdentifier>doi:10.26093/cds/vizier.51520164</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>He S.</name></creator><creator><name>Yuan W.</name></creator><creator><name>Huang J.Z.</name></creator><creator><name>Long J.</name></creator><creator><name>Macri L.M.</name></creator><date role="Updated">2018-03-28T09:31:16Z</date><date role="Created">2017-02-22T12:28:28Z</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>magellanic-clouds</subject><subject>variable-stars</subject><subject>infrared-photometry</subject><subject>visible-astronomy</subject><subject>photometry</subject><description>We develop a nonlinear semi-parametric Gaussian process model to estimate periods of Miras with sparsely sampled light curves. The model uses a sinusoidal basis for the periodic variation and a Gaussian process for the stochastic changes. We use maximum likelihood to estimate the period and the parameters of the Gaussian process, while integrating out the effects of other nuisance parameters in the model with respect to a suitable prior distribution obtained from earlier studies. Since the likelihood is highly multimodal for period, we implement a hybrid method that applies the quasi-Newton algorithm for Gaussian process parameters and search the period/frequency parameter space over a dense grid. A large-scale, high-fidelity simulation is conducted to mimic the sampling quality of Mira light curves obtained by the M33 Synoptic Stellar Survey. The simulated data set is publicly available and can serve as a testbed for future evaluation of different period estimation methods. The semi-parametric model outperforms an existing algorithm on this simulated test data set as measured by period recovery rate and quality of the resulting period-luminosity relations.</description><source format="bibcode">2016AJ....152..164H</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/152/164</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/149/117">J/AJ/149/117 : LMC infrared survey. I. Photometry of Cepheids (Macri+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/193/26">J/ApJS/193/26 : The M33 synoptic stellar survey. I. (Pellerin+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AcA/59/239">J/AcA/59/239 : Light curves of LMC long-period variables (Soszynski+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/130/776">J/AJ/130/776 : Secular evolution in Mira pulsations (Templeton+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/353/705">J/MNRAS/353/705 : OGLE Variables in Magellanic Clouds (Ita+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/121/861">J/AJ/121/861 : BVI photometry of central part of M33 (Macri+, 2001)</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/AJ/152/164</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/152/164</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/152/164</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/152/164</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/152/164</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AJ/152/164</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/AJ/152/164/table2 (*OGLE LMC Miras from Soszynski et al. 2009 (Cat. J/AcA/59/239))</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/AJ/152/164/table2?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/AJ/152/164/table2?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/AJ/152/164/table2?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>67.6873333</ra><dec>-69.8447222</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>4/2068 5/8263 8269 8280 6/33045 33046 33047 33051 33069 33073 33074 33075 33080 33081 33084 33085 33104 33105 33106 33112 33124 33125 33126 33128 33129 33130 37416 37418 37504 37506 37507 37512 37514 37515 37536</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/AJ/152/164?format=ascii</footprint><waveband>Infrared</waveband><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/AJ/152/164/table2</name><description>*OGLE LMC Miras from Soszynski et al. 2009 (Cat. J/AcA/59/239)</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Star</name><description>[82/91878] OGLE LMC Mira identification number (OGLE-LMC-LPV-NNNNN) from Soszynski et al. 2009 (Cat. J/AcA/59/239)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Nlc</name><description>Number of simulated I-band light curves</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Type</name><description>Spectral type Oxygen-rich or Carbon-rich</description><ucd>src.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="11*">char</dataType></column><column><name>&lt;Imag&gt;</name><description>[12.178/15.25] Mean I-band magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>&lt;Vmag&gt;</name><description>[15.101/21.472] Mean V-band magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>f_&lt;Vmag&gt;</name><description>[1] Extrapolated mean V magnitude for object with missing data (identified with a "1")</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Per</name><description>[103.06/1265] Main period</description><unit>d</unit><ucd>time.period;meta.main</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Simbad</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>_RA</name><description>Position from Soszynski et al. 2009 (Cat. J/AcA/59/239) (right ascension part)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Position from Soszynski et al. 2009 (Cat. J/AcA/59/239) (declination part)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column></table><table><name>J/AJ/152/164/lc</name><description>Mapping between simulated light curve ID and the original OGLE object</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>LCNum</name><description>[1/100000] Light curve identification number</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Star</name><description>[82/91878] OGLE LMC Mira identification number from Soszynski et al. 2009 (Cat. J/AcA/59/239)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Code</name><description>Light curve internal code</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="16*">char</dataType></column><column><name>LC</name><description>Light Curve</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column></table></schema></tableset></ri:Resource>