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<ri:Resource created="2023-06-16T06:37:37Z" 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>KMTNet light curve for 4 microlensing planets</title><shortName>J/AJ/165/83</shortName><identifier>ivo://CDS.VizieR/J/AJ/165/83</identifier><altIdentifier>doi:10.26093/cds/vizier.51650083</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Ryu Y.-H.</name></creator><creator><name>Shin I.-G.</name></creator><creator><name>Yang H.</name></creator><creator><name>Gould A.</name></creator><creator><name>Albrow M.D.</name></creator><creator><name>Chung S.-J.</name></creator><creator><name>Han C.,Hwang K.-H.</name></creator><creator><name>Jung Y.K.</name></creator><creator><name>Shvartzvald Y.</name></creator><creator><name>Yee J.C.</name></creator><creator><name>Zang W.</name></creator><creator><name>Cha S.-M.,Kim D.-J.</name></creator><creator><name>Kim S.-L.</name></creator><creator><name>Lee C.-U.</name></creator><creator><name>Lee D.-J.</name></creator><creator><name>Lee Y.</name></creator><creator><name>Park B.-G.</name></creator><creator><name>Pogge R.W.</name></creator><date role="Updated">2023-09-27T06:58:38Z</date><date role="Created">2023-06-16T06:37:37Z</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>exoplanets</subject><subject>gravitational-lensing</subject><subject>infrared-photometry</subject><subject>visible-astronomy</subject><subject>photometry</subject><description>We continue our program of publishing all planets (and possible planets) found by eye in 2021 Korea Microlensing Telescope Network (KMTNet) online data. We present four planets (KMT-2021-BLG-0712Lb, KMT-2021-BLG-0909Lb, KMT-2021-BLG-2478Lb, and KMT-2021-BLG-1105Lb), with planet-to-host mass ratios in the range -3.3&lt;~logq&lt;~-2.2. This brings the total of secure, by-eye, 2021 KMTNet planets to 16, including 8 in this series. The by-eye sample is an important check of the completeness of semiautomated detections, which are the basis for statistical analyses. One of the planets, KMT-2021-BLG-1105Lb, is blended with a relatively bright (I,V)~(18.9, 21.6) star that may be the host. This could be verified immediately by high-resolution imaging. If so, the host is an early G-dwarf, and the planet could be characterized by radial velocity observations on 30m class telescopes.</description><source format="bibcode">2023AJ....165...83R</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/165/83</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>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/II/323">II/323 : OGLE-III Bulge Photometric Catalog (Szymanski+ 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/549/A147">J/A+A/549/A147 : Abundances microlensed bulge dwarf stars. V. (Bensby+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/152/141">J/AJ/152/141 : Solar neighborhood. XXXVII. RVs for M dwarfs (Benedict+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/159/256">J/AJ/159/256 : Light curve of OGLE-2018-BLG-0677 (Herrera-Martin+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/161/293">J/AJ/161/293 : LCs of OGLE-2018-BLG-0567 and OGLE-2018-BLG-0962 (Jung+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/162/163">J/AJ/162/163 : Systematic KMTNet Planetary Anomaly Search. I. (Zang+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/163/43">J/AJ/163/43 : Systematic KMTNet Planetary Anomaly Search. II. (Hwang+, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/164/180">J/AJ/164/180 : Mass Prod. 2021 KMTNet Microlensing Planets. I. 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