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<ri:Resource created="2026-07-22T10:28:34Z" status="active" updated="2026-07-22T09:43:29Z" 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>20yr phot. observations of the SMC with OGLE</title><shortName>J/ApJS/280/49</shortName><identifier>ivo://CDS.VizieR/J/ApJS/280/49</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Mroz P.</name></creator><creator><name>Udalski A.</name></creator><creator><name>Szymanski M.K.</name></creator><creator><name>Soszynski I.</name></creator><creator><name>Pietrukowicz P.,Kozlowski S.</name></creator><creator><name>Poleski R.</name></creator><creator><name>Skowron J.</name></creator><creator><name>Skowron D.</name></creator><creator><name>Ulaczyk K.,Gromadzki M.</name></creator><creator><name>Rybicki K.</name></creator><creator><name>Iwanek P.</name></creator><creator><name>Wrona M.</name></creator><creator><name>Ratajczak M.</name></creator><date role="Updated">2026-07-22T09:43:29Z</date><date role="Created">2026-07-22T10:28:34Z</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-photometry</subject><subject>visible-astronomy</subject><subject>photometry</subject><description>Some previous studies have suggested that massive and intermediate-mass primordial black holes (PBHs) could comprise a substantial fraction of dark matter in the Universe. Such black holes, if they existed in the Milky Way halo, would give rise to long-duration microlensing events that may potentially last for years. However, earlier searches were not sufficiently sensitive to detect such events. Here, we present the results of searches for long-timescale gravitational microlensing events toward the Small Magellanic Cloud (SMC) using nearly 20yr of photometric observations collected by the Optical Gravitational Lensing Experiment (OGLE) from 2001-2020. We found six events, three of which are new discoveries. We use a sample of five events to measure the microlensing optical depth toward the SMC {tau}=(0.32{\pm}0.18)x10^-7^ and the event rate {Gamma}=(1.18{\pm}0.57)x10^-7^/yr/star. The properties of the detected events are consistent with lenses originating from known stellar populations within the SMC or in the Milky Way disk. No events with timescales longer than 1yr were detected, which provides competitive limits on the fraction of massive compact objects, including PBHs, in the Milky Way dark matter halo. Together with the earlier OGLE studies of microlensing events in the direction of the Large Magellanic Cloud, these observations rule out PBHs and other compact objects with masses ranging from 10^-8^-10^3^M_{sun}_ as dominant components of dark matter.</description><source format="bibcode">2025ApJS..280...49M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/280/49</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/I/355">I/355 : Gaia DR3 Part 1. Main source (Gaia Collaboration, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AcA/50/421">J/AcA/50/421 : OGLE-II DIA BUL_SC1 field (Wozniak, 2000)</relatedResource><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/AJ/144/4">J/AJ/144/4 : Dwarf galaxies in the Local Group (McConnachie+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/616/A12">J/A+A/616/A12 : Gaia DR2 sources in GC and dSph (Gaia Collaboration+, 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/904/13">J/ApJ/904/13 : Radial velocity for 10 giant EBs (Graczyk+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/649/A7">J/A+A/649/A7 : MC structure and properties (Gaia Collaboration+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/252/23">J/ApJS/252/23 : Reddening map of MCs from OGLE-IV RC stars (Skowron+, 2021)</relatedResource><relatedResource>https://www.astrouw.edu.pl/ogle/ogle4/SMC_OPTICAL_DEPTH/ : associated data of</relatedResource><relatedResource>this paper (also doi:10.5281/zenodo.16735482)</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/280/49</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/280/49</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/280/49</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Field</name><description>OGLE-IV field name (SMCNNN)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType><flag>primary</flag></column><column><name>RAJ2000</name><description>Hour of Right ascension (J2000)</description><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Degree of Declination (J2000)</description><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Nepoch1</name><description>[0/702] Minimal number of OGLE-III epochs in I band; 2001-2009</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Nepoch2</name><description>[0/3318] Maximal number of OGLE-III epochs in V band; 2001-2009</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Nepoch3</name><description>[151/1090] Number of OGLE-IV epochs in I band; 2010-2020</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Nepoch4</name><description>[7/321] Number of OGLE-IV epochs in V band; 2010-2020</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Nstars1</name><description>[0/1463.1] Number of stars observed during both OGLE-III and OGLE-IV; in thousands</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Nstars2</name><description>[0/137.9] Number of stars observed during OGLE-IV only; in thousands</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Nstars3</name><description>[21.3/1473] Total number of stars; in thousands</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Nsf</name><description>Number of subfields for this field (link to Tables 2+6)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column></table><table><name>J/ApJS/280/49/subfields</name><description>Number of microlensing source stars observed in OGLE-IV fields (Table 6) and Error bar correction coefficients for the I-band data (Table 2)</description><column><name>Field</name><description>OGLE-IV field name (SMCNNN)</description><ucd>obs.field</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></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>sField</name><description>OGLE-IV subfield name (NN; SMCNNN.NN for a complete designation)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>RAJ2000</name><description>Right ascention (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>[-83/-62.7] Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>N21Tot</name><description>[398/174447] Total number of sources brighter than I=21 mag</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>N21Corr</name><description>[0/173678] Corrected number of sources brighter than I=21 mag</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>N21.5Tot</name><description>[434/244105] Number of sources brighter than I=21.5 mag</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>N21.5Corr</name><description>[0/243240] Corrected number of sources brighter than I=21.5 mag</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>N22Tot</name><description>[481/338613] Total number of sources brighter than I=22 mag</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>N22Corr</name><description>[0/337698] Corrected number of sources brighter than I=22 mag</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>gam3</name><description>[0.9/1.96]? 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