<?xml-stylesheet href='/static/xsl/oai.xsl' type='text/xsl'?>
<ri:Resource created="2024-02-29T13:39:37Z" 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>Microlensing event rate in the GC. I. UKIRT obs.</title><shortName>J/ApJS/269/28</shortName><identifier>ivo://CDS.VizieR/J/ApJS/269/28</identifier><altIdentifier>doi:10.26093/cds/vizier.22690028</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Wen Y.</name></creator><creator><name>Zang W.</name></creator><creator><name>Ma Bo</name></creator><date role="Updated">2024-11-06T20:30:25Z</date><date role="Created">2024-02-29T13:39:37Z</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>gravitational-lensing</subject><subject>infrared-sources</subject><subject>surveys</subject><subject>astronomical-object-identification</subject><subject>galactic-center</subject><description>To overcome the high optical extinction, near-infrared (NIR) observations are needed for probing the microlensing events toward the Galactic center. The 2015-2019 UKIRT microlensing survey toward the Galactic center is the first dedicated precursor NIR survey for the Nancy Grace Roman Space Telescope. Here, we analyze the online data from the UKIRT microlensing survey, reaching l=b=0{deg}. Using the event-finder algorithm of KMTNet with the {Delta}{chi}^2^ threshold of 250, we find 522 clear events, 436 possible events, and 27 possible anomalous events. We fit a point-source point-lens (PSPL) model to all the clear events and derive the PSPL parameters with uncertainties using a Markov Chain Monte Carlo method. Assuming perfect detection efficiency, we compute the uncorrected event rates, which should serve as the lower limits on the true event rate. We find that the uncorrected NIR event rates are likely rising toward the Galactic center and are higher than the optical event rates.</description><source format="bibcode">2023ApJS..269...28W</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/269/28</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/other/Nat/481.167">J/other/Nat/481.167 : 2002-2007 PLANET microlensing events (Assan+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/778/150">J/ApJ/778/150 : Microlensing events toward the Bulge (Sumi+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/457/4089">J/MNRAS/457/4089 : Frequency of snowline-region planets (Shvartzvald+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/827/139">J/ApJ/827/139 : Microlensing opt. depths from MOA-II (Sumi+, 2016)</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/155/186">J/AJ/155/186 : The KMTNet/K2-C9 (Kepler) Data Release (Kim+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/244/29">J/ApJS/244/29 : Microlensing events toward the Galactic bulge (Mroz+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/889/56">J/ApJ/889/56 : VVV survey microlensing events (Navarro+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/161/126">J/AJ/161/126 : I-band LC of KMT-2017-BLG-2820 (Ryu+, 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>http://kmtnet.kasi.re.kr/~ulens/ : KMTNet microlensing events archive</relatedResource><relatedResource>http://ogle.astrouw.edu.pl/ogle4/ews/ews.html : OGLE-IV EWS archive</relatedResource><relatedResource>http://www.massey.ac.nz/~iabond/moa/alerts/ : MOA Transient alerts archive</relatedResource><relatedResource>http://exoplanetarchive.ipac.caltech.edu/docs/UKIRTMission.html : UKIRT home</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/ApJS/269/28</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/269/28</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/269/28</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJS/269/28</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJS/269/28</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJS/269/28</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/ApJS/269/28/table5 (Summary of microlensing events with observations from UKIRT and at least one other microlensing survey (OGLE, MOA, or KMTNet))</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJS/269/28/table5?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJS/269/28/table5?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJS/269/28/table5?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>265.90683306</ra><dec>-27.37333306</dec><sr>0.005555555555555556</sr></testQuery></capability><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/ApJS/269/28/tablea1 (Parameters of the clear point source point lens microlensing events from the UKIRT survey)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJS/269/28/tablea1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJS/269/28/tablea1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJS/269/28/tablea1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>269.33126694</ra><dec>-28.07066</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>5/7207 7212-7213 7216 6/28782 28819 28821-28823 28825-28827 28837 28839 28857 28860 28868 28870-28874 28898</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJS/269/28?format=ascii</footprint><waveband>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJS/269/28/table5</name><description>Summary of microlensing events with observations from UKIRT and at least one other microlensing survey (OGLE, MOA, or KMTNet)</description><column><name>KB</name><description>? Events names of KMTNet if available (KMT-20YY-BLG-NNNN; see also Kim+ 2018, J/AJ/155/186)</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>OB</name><description>? Events names of OGLE if available (&lt;OGLE-20YY-BLG-NNNN&gt; in Simbad)</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><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>ID</name><description>Source ID in the UKIRT database (ukirt_c_2015_a_NN_N_NNNNNNN) (1)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="27*">char</dataType></column><column><name>RAJ2000</name><description>[263/272] Right Ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>[-31/-26] Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>K18</name><description>Display data from Kim+ 2018, J/AJ/155/186 within 2"</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>MB</name><description>? Events names of MOA if available (MOA-20YY-BLG-NNN)</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>M19</name><description>Display data from Mroz+ 2019, J/ApJS/244/29 within 0.5"</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column></table><table><name>J/ApJS/269/28/tablea1</name><description>Parameters of the clear point source point lens microlensing events from the UKIRT survey</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>Seq</name><description>[1/522] UKIRT running sequence number identifier</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>RAJ2000</name><description>[263/272] Right Ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>[-31/-26] Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>u0</name><description>[0/1.5] Impact parameter</description><ucd>src.impactParam</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_u0</name><description>[0/1] Upper uncertainty in u0</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_u0</name><description>[0/0.6] Lower uncertainty in u0</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>t0</name><description>[7182/8731] Julian Date peak magnification; JD-24540000.0</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>E_t0</name><description>[0.003/7] Upper uncertainty in t0</description><unit>d</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_t0</name><description>[0.003/9] Lower uncertainty in t0</description><unit>d</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>tE</name><description>[1.6/348] Einstein radius crossing time</description><unit>d</unit><ucd>time.crossing</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_tE</name><description>[0.07/153] Upper uncertainty in tE</description><unit>d</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_tE</name><description>[0.05/259] Lower uncertainty in tE</description><unit>d</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>fbl</name><description>[0.001/1] Blending parameter (1=no blending; ~0=extreme blending) (1)</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_fbl</name><description>[0/0.8] Upper uncertainty in fbl</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_fbl</name><description>[0/0.3] Lower uncertainty in fbl</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>