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<ri:Resource created="2013-03-27T15:44:29Z" 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>Chandra monitoring of QSO J2240+0321</title><shortName>J/ApJ/740/L34</shortName><identifier>ivo://CDS.VizieR/J/ApJ/740/L34</identifier><altIdentifier>doi:10.26093/cds/vizier.17409034</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Chen B.</name></creator><creator><name>Dai X.</name></creator><creator><name>Kochanek C.S.</name></creator><creator><name>Chartas G.</name></creator><creator><name>Blackburne J.A.</name></creator><creator><name>Kozlowski S.</name></creator><date role="Updated">2013-04-16T13:26:24Z</date><date role="Created">2013-03-27T15:44:29Z</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>quasars</subject><subject>x-ray-sources</subject><description>We present our long-term Chandra X-ray monitoring data for the gravitationally lensed quasar Q2237+0305 with 20 epochs spanning 10 years. We easily detect microlensing variability between the images in the full (0.2-8keV), soft (0.2-2keV), and hard (2-8keV) bands at very high confidence. We also detect, for the first time, chromatic microlensing differences between the soft and hard X-ray bands. The hard X-ray band is more strongly microlensed than the soft band, suggesting that the corona above the accretion disk thought to generate the X-rays has a non-uniform electron distribution, in which the hotter and more energetic electrons occupy more compact regions surrounding the black holes. Both the hard and soft X-ray bands are more strongly microlensed than the optical (rest-frame UV) emission, indicating that the X-ray emission is more compact than the optical, confirming the microlensing results from other lenses.</description><source format="bibcode">2011ApJ...740L..34C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/740/L34</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/B/chandra">B/chandra : The Chandra Archive Log (CXC, 1999-2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/134">V/134 : Atlas of Radio/X-ray associations (ARXA) (Flesch, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/IX/41">IX/41 : XMM-Newton Serendipitous Source Catalogue 2XMMi-DR3 (XMM-SSC, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/493/339">J/A+A/493/339 : XMM-Newton serendipitous Survey. V. (Watson+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/169/401">J/ApJS/169/401 : ChaMP X-ray point source catalog (Kim+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AZh/84/885">J/AZh/84/885 : VRI observations of radio source S5 0716+71 (Koptelova+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/420/447">J/A+A/420/447 : VRI photometry of lensed QSO B2237+0305 (Vakulik+, 2004)</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/ApJ/740/L34</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/740/L34</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/740/L34</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/740/L34</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/740/L34</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/740/L34</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><coverage><footprint ivo-id="ivo://ivoa.net/std/moc"/><waveband>X-ray</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/740/L34/table1</name><description>Chandra count rates of Q2237+0305 corrected for absorption</description><column><name>JD</name><description>[51794/55528] Julian Date (JD-2400000)</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">int</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>ObsID</name><description>[431/13195] Chandra observation number</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Exp</name><description>[7264/30287] Exposure time</description><unit>s</unit><ucd>time.duration;obs.exposure</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Image</name><description>[A-D] Image identification (1)</description><ucd>meta.id;obs.image</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>CRfull</name><description>[2/211.9] Full 0.2-8keV band count rate</description><unit>ct/ks</unit><ucd>phot.count;em.X-ray</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_CRfull</name><description>[0.5/14.5] Uncertainty in CRfull</description><unit>ct/ks</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>CRsoft</name><description>[1.5/197.2] Soft 0.2-2keV band count rate</description><unit>ct/ks</unit><ucd>phot.count;em.X-ray</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_CRsoft</name><description>[0.4/9.7] Uncertainty in CRsoft</description><unit>ct/ks</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>CRhard</name><description>[0.3/22.7] Hard 2-8keV band count rate</description><unit>ct/ks</unit><ucd>phot.count;em.X-ray</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_CRhard</name><description>[0.2/2.1] Uncertainty in CRhard</description><unit>ct/ks</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>