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<ri:Resource created="2020-05-04T08:24:26Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" 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/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>Transit analysis for the K2-25 system</title><shortName>J/AJ/159/83</shortName><identifier>ivo://CDS.VizieR/J/AJ/159/83</identifier><altIdentifier>doi:10.26093/cds/vizier.51590083</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Kain I.J.</name></creator><creator><name>Newton E.R.</name></creator><creator><name>Dittmann J.A.</name></creator><creator><name>Irwin J.M.</name></creator><creator><name>Mann A.W.</name></creator><creator><name>Thao P.C.,Charbonneau D.</name></creator><creator><name>Winters J.G.</name></creator><date role="Updated">2020-07-21T12:57:35Z</date><date role="Created">2020-05-04T08:24:26Z</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>m-stars</subject><subject>exoplanets</subject><subject>infrared-photometry</subject><subject>visible-astronomy</subject><subject>photometry</subject><description>The abundance of planets with orbital periods of a few to tens of days suggests that exoplanets experience complex dynamical histories. Planets in young stellar clusters or associations have well-constrained ages and therefore provide an opportunity to explore the dynamical evolution of exoplanets. K2-25b is a Neptune-sized planet in an eccentric, 3.48day orbit around an M4.5 dwarf star in the Hyades cluster (650Myr). In order to investigate its non-zero eccentricity and tight orbit, we analyze transit timing variations (TTVs) which could reveal clues to the migration processes that may have acted on the planet. We obtain 12 nonconsecutive transits using the MEarth observatories and long-term photometric monitoring, which we combine with 10 transits from the Spitzer Space Telescope and 20 transits from K2. Tables of MEarth photometry accompany this work. We fit each transit lightcurve independently. We first investigate whether inhomogeneities on the stellar surface (such as spots or plages) are differentially affecting our transit observations. The measured transit depth does not vary significantly between transits, though we see some deviations from the fiducial transit model. We then looked for TTVs as evidence of a nontransiting perturber in the system. We find no evidence for &gt;1M_{Earth}_ mass companions within a 2:1 period ratio, or for &gt;5M_{Earth}_ mass planets within a 7:2 period ratio.</description><source format="bibcode">2020AJ....159...83K</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/159/83</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>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/331/81">J/A+A/331/81 : Hyades membership (Perryman+ 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/367/111">J/A+A/367/111 : A Hipparcos study of the Hyades cluster (de+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/709/168">J/ApJ/709/168 : Eccentric orbits in exoplanets (Anglada-Escude+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/795/161">J/ApJ/795/161 : Activity &amp; rotation in Praesepe and the Hyades (Douglas+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/216/7">J/ApJS/216/7 : Planets Around Low-Mass Stars (PALMS). IV. (Bowler+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/818/153">J/ApJ/818/153 : MEarth photometry: nearby M-dwarf magnitudes (Dittmann+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/821/93">J/ApJ/821/93 : Rotation &amp; Galactic kinematics of mid M dwarfs (Newton+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/592/A13">J/A+A/592/A13 : HD 219828 radial velocity curve (Santos+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/825/19">J/ApJ/825/19 : Mass-radius relationship for planets with Rp&lt;4 (Wolfgang+,2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/836/167">J/ApJ/836/167 : K2 planetary syst. around low-mass stars. I. (Dressing+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/154/142">J/AJ/154/142 : Corrected photometry for GJ1132 for eclipses (Dittmann+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/154/224">J/AJ/154/224 : Transiting planets in young clusters from K2 (Rizzuto+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/156/140">J/AJ/156/140 : 4 new eclipsing mid M-dwarf systems from MEarth (Irwin+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/156/217">J/AJ/156/217 : Stellar properties for M dwarfs in MEarth-South (Newton+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/610/A20">J/A+A/610/A20 : HITEP. II. Transiting exoplanets imaging (Evans+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/613/A41">J/A+A/613/A41 : 5 exoplanet light and RV curves (Mancini+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/616/A10">J/A+A/616/A10 : 46 open clusters GaiaDR2 HR diagrams (Gaia Collaboration, 2018)</relatedResource><relatedResource>http://www.cfa.harvard.edu/MEarth : MEarth project home page</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/159/83</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/159/83</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/159/83</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/159/83</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/159/83</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AJ/159/83</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><coverage><footprint ivo-id="ivo://ivoa.net/std/moc"/><waveband>Optical</waveband><waveband>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/AJ/159/83/fig1</name><description>*MEarth transits photometry</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>N</name><description>[87/192] Transit number</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>BJD</name><description>[2457365/2457732] Barycentric Julian Date</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Dmag</name><description>[-0.28/0.08] Differential magnitude</description><unit>mag</unit><ucd>phot.mag;arith.diff</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_Dmag</name><description>[0.002/0.09] Uncertainty in Dmag</description><unit>mag</unit><ucd>stat.error;phot.mag;arith.diff</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Tel</name><description>[1/18] MEarth telescope identifier</description><ucd>meta.id;instr.tel</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column></table><table><name>J/AJ/159/83/fig2</name><description>Stellar rotational variability over three years</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>BJD</name><description>[2457366/2458335] Barycentric Julian Date</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>mag</name><description>[-0.06/0.05] Relative brightness</description><unit>mag</unit><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_mag</name><description>[0.002/0.03] Uncertainty in mag</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table></schema></tableset></ri:Resource>