<?xml-stylesheet href='/static/xsl/oai.xsl' type='text/xsl'?>
<ri:Resource created="2019-05-28T15:27:08Z" 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>Strong-lensing systems from 4 surveys</title><shortName>J/ApJ/806/185</shortName><identifier>ivo://CDS.VizieR/J/ApJ/806/185</identifier><altIdentifier>doi:10.26093/cds/vizier.18060185</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Cao S.</name></creator><creator><name>Biesiada M.</name></creator><creator><name>Gavazzi R.</name></creator><creator><name>Piorkowska A.</name></creator><creator><name>Zhu Z.-H.</name></creator><date role="Updated">2019-07-24T11:47:14Z</date><date role="Created">2019-05-28T15:27:08Z</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>redshifted</subject><subject>galaxy-kinematics</subject><subject>surveys</subject><description>In this paper, we assemble a catalog of 118 strong gravitational lensing systems from the Sloan Lens ACS Survey (SLACS), BOSS emission-line lens survey (BELLS), Lens Structure and Dynamics (LSD), and Strong Lensing Legacy Survey (SL2S) and use them to constrain the cosmic equation of state. In particular, we consider two cases of dark energy phenomenology: the XCDM model, where dark energy is modeled by a fluid with constant w equation-of-state parameter, and in the Chevalier-Polarski-Linder (CPL) parameterization, where w is allowed to evolve with redshift, w(z)=w_0_+w_1_(z/1+z). We assume spherically symmetric mass distribution in lensing galaxies, but we relax the rigid assumption of the SIS model in favor of a more general power-law index {gamma}, also allowing it to evolve with redshifts {gamma}(z). Our results for the XCDM cosmology show agreement with values (concerning both w and {gamma} parameters) obtained by other authors. We go further and constrain the CPL parameters jointly with {gamma}(z). The resulting confidence regions for the parameters are much better than those obtained with a similar method in the past. They are also showing a trend of being complementary to the Type Ia supernova data. Our analysis demonstrates that strong gravitational lensing systems can be used to probe cosmological parameters like the cosmic equation of state for dark energy. Moreover, they have a potential to judge whether the cosmic equation of state evolved with time or not.</description><source format="bibcode">2015ApJ...806..185C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/806/185</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/ApJS/219/29">J/ApJS/219/29 : Redshifts in strong lens fields (Momcheva+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/777/97">J/ApJ/777/97 : SL2S galaxy-scale lens sample. III. (Sonnenfeld+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/749/38">J/ApJ/749/38 : CFHTLS-SL2S-ARCS strong lens candidates (More+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/746/85">J/ApJ/746/85 : THe HST Cluster Supernova Survey. V. (Suzuki+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/705/1099">J/ApJ/705/1099 : The Sloan Lens ACS (SLACS) Survey. IX. (Auger+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/690/670">J/ApJ/690/670 : The Sloan lens ACS Survey. VIII. (Treu+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/682/964">J/ApJ/682/964 : Sloan lens ACS survey. V. (Bolton+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/276/1341">J/MNRAS/276/1341 : Spectroscopy of E and S0 galaxies (Jorgensen+, 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/273/1097">J/MNRAS/273/1097 : CCD photometry for E and S0 galaxies (Jorgensen+ 1995)</relatedResource><relatedResource>http://www.sdss3.org/ : SDSS-III home page</relatedResource><relatedResource>http://web.physics.ucsb.edu/~tt/LSD/ : Lens Structure &amp; Dynamics survey</relatedResource><relatedResource>http://www-sl2s.iap.fr/ : CFHTLS-SL2S home page</relatedResource><relatedResource>http://www.slacs.org/ : The Sloan Lens ACS Survey home page</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/806/185</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/806/185</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/806/185</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/806/185</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/806/185</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/806/185</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/ApJ/806/185/table1 (Compilation of strong-lensing systems)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/806/185/table1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/806/185/table1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/806/185/table1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>27.7807111</ra><dec>0.8191581</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/4182 4352 4853 5500 5701 5719 5802 5878 5951 5986 6105 6340 6393 6470 6585 6607 6628 6981 7305 8505 8510 8518 8568 8700 9039 9084 9809 9995 10020 10355 10453 10459 10596 10741 10748 10749 10883 10990 11347 11389 11424 11425 11439 11448 11777 11850 11948 12804 16644 17238 17321 17665 17667 17678 17682 17687 17689 17690 17692 17712 17751 17816 17840 18072 18089 18114 18542 18778 18841 18844 19027 19030 19032 19037 19059 19065 19135 19776 20003 23061 23193 23210 25599 25852 25957 26012 26159 26167 26195 26279 26331 26951 27134 27196 27258 27286 27308 27348 27551 27672 27726 27803 30974 31378 31705 31743 40935 40940 40941 40943 40955 40957 45050</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/806/185?format=ascii</footprint></coverage><tableset><schema><name>default</name><table><name>J/ApJ/806/185/table1</name><description>Compilation of strong-lensing systems</description><column><name>SimbadName</name><description>Simbad column added by the CDS</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="26*">char</dataType></column><column><name>Survey</name><description>Survey ID (1)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">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>Name</name><description>Strong-lensing system ID (JHHMM+DDMM)</description><ucd>meta.id;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="11*">char</dataType></column><column><name>zl</name><description>[0.07/1.1] Lens redshift</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>zs</name><description>[0.19/3.6] Source redshift</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Sigma</name><description>[98/396] Velocity dispersion within the aperture</description><unit>km/s</unit><ucd>phys.veloc.dispersion</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>e_Sigma</name><description>[8/60] Sigma uncertainty</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>thetaE</name><description>[0.3/2.6] Angular Einstein radius</description><unit>arcsec</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>thetaAp</name><description>[0.6/1.5] Aperture radius</description><unit>arcsec</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>thetaEff</name><description>[0.2/4.8] Effective radius</description><unit>arcsec</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Sig0</name><description>[103/391] Aperture-corrected velocity dispersion</description><unit>km/s</unit><ucd>phys.veloc.dispersion</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>e_Sig0</name><description>[8/61] Sig0 uncertainty</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Cat</name><description>Number of cross-matches within 5.0" with SLACS (Cat. J/ApJ/705/1099) and SL2S (Cat. J/ApJ/777/97)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>_RA</name><description>Positions of the systems from SIMBAD or of the lenses (mainly from SL2S) (right ascension part)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Positions of the systems from SIMBAD or of the lenses (mainly from SL2S) (declination part)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column></table></schema></tableset></ri:Resource>