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<ri:Resource created="2024-03-04T14:44:43Z" 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>NIR photometry of the core of R136</title><shortName>J/MNRAS/503/292</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/503/292</identifier><altIdentifier>doi:10.26093/cds/vizier.75030292</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Khorrami Z.</name></creator><creator><name>Langlois M.</name></creator><creator><name>Clark P.C.</name></creator><creator><name>Vakili F.</name></creator><creator><name>Buckner A.S.M.,Gonzalez M.</name></creator><creator><name>Crowther P.</name></creator><creator><name>Wunsch R.</name></creator><creator><name>Palous J.</name></creator><creator><name>Lumsden S.</name></creator><creator><name>Moraux E.</name></creator><date role="Updated">2024-11-06T20:33:21Z</date><date role="Created">2024-03-04T14:44:43Z</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>open-star-clusters</subject><subject>infrared-photometry</subject><description>We present the sharpest and deepest near-infrared photometric analysis of the core of R136, a newly formed massive star cluster at the centre of the 30 Doradus star-forming region in the Large Magellanic Cloud. We used the extreme adaptive optics of the SPHERE focal instrument implemented on the ESO Very Large Telescope and operated in its IRDIS imaging mode for the second time with longer exposure time in the H and K filters. Our aim was to (i) increase the number of resolved sources in the core of R136, and (ii) to compare with the first epoch to classify the properties of the detected common sources between the two epochs. Within the field of view (FOV) of 10.8"x12.1" (2.7pc*3.0pc), we detected 1499 sources in both H and K filters, for which 76 per cent of these sources have visual companions closer than 0.2". The larger number of detected sources enabled us to better sample the mass function (MF). The MF slopes are estimated at ages of 1, 1.5, and 2Myr, at different radii, and for different mass ranges. The MF slopes for the mass range of 10-300M_{sun}_ are about 0.3dex steeper than the mass range of 3-300M_{sun}_, for the whole FOV and different radii. Comparing the JHK colours of 790 sources common in between the two epochs, 67 per cent of detected sources in the outer region (r&gt;3") are not consistent with evolutionary models at 1-2Myr and with extinctions similar to the average cluster value, suggesting an origin from ongoing star formation within 30 Doradus, unrelated to R136.</description><source format="bibcode">2021MNRAS.503..292K</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/503/292</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/ApJ/448/179">J/ApJ/448/179 : HST photometry in R136 (Hunter+ 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/602/A56">J/A+A/602/A56 : R136 JKs photometry from VLT/SPHERE EAO (Khorrami+, 2017)</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/MNRAS/503/292</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/503/292</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/503/292</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/503/292</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/503/292</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/503/292</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/MNRAS/503/292/tablea1 (List of brightest spectroscopically known stars in the core of R136 studied in optical)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/503/292/tablea1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/503/292/tablea1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/503/292/tablea1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>84.67665</ra><dec>-69.1007972</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/MNRAS/503/292/tablea2 (List of detected sources in the centre of R136 brighter than 16mag in K)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/503/292/tablea2?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/503/292/tablea2?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/503/292/tablea2?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>84.67665</ra><dec>-69.1007972</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/33094</spatial><spectral>7.952274030004205e-20 4.2441532724171825e-19</spectral><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/503/292?format=ascii</footprint><waveband>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/MNRAS/503/292/tablea1</name><description>List of brightest spectroscopically known stars in the core of R136 studied in optical</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>HSH95</name><description>Identification number in Hunter et al. (1995ApJ...448..179H, Cat. J/ApJ/448/179), [HSH95] NNNN in Simbad</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Simbad</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>WB85</name><description>Name in Weigelt &amp; Baier (1985A&amp;A...150L..18W), RMC 136aN in Simbad</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>IDK</name><description>Star identification in the SPHERE/IRDIS/K-band catalogue</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Kmag18</name><description>SPHERE IRDIS K magnitude in 2018 (error +/-0.01)</description><unit>mag</unit><ucd>phot.mag;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Hmag18</name><description>SPHERE IRDIS H magnitude in 2018 (error +/-0.01)</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Jmag15</name><description>SPHERE IRDIS J magnitude in 2015 (error +/-0.13)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>r</name><description>Distance from r136a1 in our K data</description><unit>arcsec</unit><ucd>pos.angDistance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Teff</name><description>Effective temperature</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>SpType</name><description>Spectral type</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType" arraysize="12*">char</dataType></column><column><name>e_Teff</name><description>Effective temperature error</description><unit>K</unit><ucd>stat.error;phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>r_Teff</name><description>Reference for Teff if not from Bestenlehner et al., 2014A&amp;A...570A..38B (1)</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column><column><name>logL</name><description>Luminosity</description><unit>log(solLum)</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_logL</name><description>Luminosity error (upper value)</description><unit>log(solLum)</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_logL</name><description>Luminosity error (lower value)</description><unit>log(solLum)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>r_logL</name><description>Reference for logL if not from Bestenlehner et al., 2014A&amp;A...570A..38B (1)</description><ucd>meta.ref</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column><column><name>logg</name><description>? 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