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<ri:Resource created="2022-10-10T07:00:50Z" 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>R, I and L bands light curve of OGLE-2016-BLG-1093Lb</title><shortName>J/AJ/163/254</shortName><identifier>ivo://CDS.VizieR/J/AJ/163/254</identifier><altIdentifier>doi:10.26093/cds/vizier.51630254</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Shin I.-G.</name></creator><creator><name>Yee J.C.</name></creator><creator><name>Hwang K.-H.</name></creator><creator><name>Gould A.</name></creator><creator><name>Udalski A.</name></creator><creator><name>Bond I.A.,Albrow M.D.</name></creator><creator><name>Chung S.-J.</name></creator><creator><name>Han C.</name></creator><creator><name>Kil Jung Y.</name></creator><creator><name>Woo Kim H.</name></creator><creator><name>Ryu Y.-H.,Shvartzvald Y.</name></creator><creator><name>Zang W.</name></creator><creator><name>Cha S.-M.</name></creator><creator><name>Kim D.-J.</name></creator><creator><name>Kim S.-L.</name></creator><creator><name>Lee C.-U.,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><creator><name>Mroz P.</name></creator><creator><name>Szymanski M.K.,Skowron J.</name></creator><creator><name>Poleski R.</name></creator><creator><name>Soszynski I.</name></creator><creator><name>Pietrukowicz P.</name></creator><creator><name>Kozlowski S.,Ulaczyk K.</name></creator><creator><name>Beichman C.A.</name></creator><creator><name>Bryden G.</name></creator><creator><name>Calchi Novati S.</name></creator><creator><name>Carey S.,Gaudi B.S.</name></creator><creator><name>Henderson C.B.</name></creator><creator><name>Zhu W.</name></creator><creator><name>Abe F.</name></creator><creator><name>Barry R.K.</name></creator><creator><name>Bennett D.P.,Bhattacharya A.</name></creator><creator><name>Fujii H.</name></creator><creator><name>Fukui A.</name></creator><creator><name>Hirao Y.</name></creator><creator><name>Itow Y.</name></creator><creator><name>Kirikawa R.,Koshimoto N.</name></creator><creator><name>Kondo I.</name></creator><creator><name>Matsubara Y.</name></creator><creator><name>Matsumoto S.</name></creator><creator><name>Miyazaki S.</name></creator><creator><name>Muraki Y.,Olmschenk G.</name></creator><creator><name>Okamura A.</name></creator><creator><name>Ranc C.</name></creator><creator><name>Rattenbury N.J.</name></creator><creator><name>Satoh Y.</name></creator><creator><name>Silva S.I.,Sumi T.</name></creator><creator><name>Suzuki D.</name></creator><creator><name>Toda T.</name></creator><creator><name>Tristram P.J.</name></creator><creator><name>Vandorou A.</name></creator><creator><name>Yama H.,Leading authors</name></creator><creator><name>The KMTNet Collaboration</name></creator><creator><name>The OGLE Collaboration,The Spitzer team</name></creator><creator><name>The MOA Collaboration</name></creator><date role="Updated">2022-11-09T06:06:12Z</date><date role="Created">2022-10-10T07:00:50Z</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>gravitational-lensing</subject><subject>exoplanets</subject><subject>infrared-photometry</subject><description>OGLE-2016-BLG-1093 is a planetary microlensing event that is part of the statistical Spitzer microlens parallax sample. The precise measurement of the microlens parallax effect for this event, combined with the measurement of finite-source effects, leads to a direct measurement of the lens masses and system distance, M_host_=0.38-0.57M{sun} and m_p_=0.59-0.87MJup, and the system is located at the Galactic bulge (DL~8.1kpc). Because this was a high-magnification event, we are also able to empirically show that the "cheap-space parallax" concept produces well-constrained (and consistent) results for |{pi}E|. This demonstrates that this concept can be extended to many two-body lenses. Finally, we briefly explore systematics in the Spitzer light curve in this event and show that their potential impact is strongly mitigated by the color constraint.</description><source format="bibcode">2022AJ....163..254S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/163/254</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/529/A102">J/A+A/529/A102 : MOA-2007-BLG-387Lb light curve I band (Batista+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/533/A134">J/A+A/533/A134 : Abundances of microlensed stars in the Bulge (Bensby+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/154/210">J/AJ/154/210 : 2015 high-cadence Spitzer microlensing events (Zhu+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/160/74">J/AJ/160/74 : Optical and IR photometry of OGLE-2017-BLG-0406 (Hirao+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/160/255">J/AJ/160/255 : KMTNet &amp; OGLE I-band photo. of KMT-2019-BLG-0842 (Jung+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/162/267">J/AJ/162/267 : I-band light curve OGLE2019-BLG-1058 with KMTNet (Shin+, 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. 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