J/MNRAS/372/1425ivo://CDS.VizieR/J/MNRAS/372/1425doi:10.26093/cds/vizier.73721425CDSHalkola A.Seitz S.Pannella M.2024-07-03T20:14:26Z2007-10-03T17:36:57ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frgalaxy-clustersgravitational-lensinggalaxy-classification-systemsgalaxy-kinematicsredshiftedWe have derived the mass distribution of galaxy cluster Abell 1689 within 0.3h^-1^_70_Mpc of the cluster centre using its strong lensing (SL) effect on 32 background galaxies, which are mapped in altogether 107 multiple images. The multiple images are based on some from the literature with modifications to both include new and exclude some of the original image systems. The cluster profile is explored further out to ~2.5h^-1^_70_Mpc with weak lensing (WL) shear measurements from the literature. The masses of ~200 cluster galaxies are measured with the Fundamental Plane (FP) in order to model accurately the small-scale mass structure in the cluster. The cluster galaxies are modelled as elliptical truncated isothermal spheres. The scalings of the truncation radii with the velocity dispersions of galaxies are assumed to match those of: (i) field galaxies; and (ii) theoretical expectations for galaxies in dense environments. The dark matter (DM) component of the cluster is described by either non-singular isothermal ellipsoids (NSIE) or elliptical versions of the universal DM profile (elliptical Navarro, Frenk & White, ENFW). To account for substructure in the DM we allow for two DM haloes.2006MNRAS.372.1425Hhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/372/1425CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/372/1425https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/372/1425http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/372/1425https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/372/1425https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/372/1425http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/372/1425GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/MNRAS/372/1425/tableb1 (Galaxy properties from fitting cluster galaxies with a Sersic profile. The parameters of the 80 most massive galaxies are tabulated.)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/372/1425/tableb1?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/372/1425/tableb1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/372/1425/tableb1?GETtext/xml+votable180.050000true197.856375-1.34363610.005555555555555556Cone search capability for table J/MNRAS/372/1425/tablec2 (Images used in this study)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/372/1425/tablec2?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/372/1425/tablec2?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/372/1425/tablec2?GETtext/xml+votable180.050000true197.8608333-1.3324250.0055555555555555566/26189https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/372/1425?format=asciiOpticaldefaultJ/MNRAS/372/1425/tableb1Galaxy properties from fitting cluster galaxies with a Sersic profile. The parameters of the 80 most massive galaxies are tabulated.recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordint[HSP2006]Galaxy sequential numbermeta.recordintRAJ2000Right ascension (J2000)pos.eq.ra;meta.mainDEJ2000Declination (J2000)pos.eq.dec;meta.mainF775WTotal F775W AB magnitude (1)magphot.mag;em.opt.Ifloate_F775Wrms uncertainty on F775Wmagmagstat.errorfloatSerSersic value of the profilestat.fit.paramfloate_Serrms uncertainty on Serstat.errorfloatReCircularized physical half light radiuskpcphys.size.radiusfloate_Rerms uncertainty on Rekpcstat.errorfloat1-b/aGalaxy ellipticitysrc.ellipticityfloate_1-b/arms uncertainty on 1-b/astat.errorfloatPAGalaxy position angledegpos.posAnginte_PArms uncertainty on PAdegstat.errorintsigmaEstimated galaxy velocity dispersion (2)km/sphys.veloc.dispersionintsigmaUUpper value of galaxy velocity dispersion (1{sigma} range)km/sinstr.bandwidthintsigmaLLower value of galaxy velocity dispersion (1{sigma} range)km/sinstr.bandwidthintJ/MNRAS/372/1425/tablec2Images used in this studyrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintArcArc designation ([HSP2006] Arc NN.a in Simbad)meta.id;meta.mainchar[BBC2005]? Broadhurst et al., 2005, Cat. <J/ApJ/621/53> identification numbermeta.idfloatnullableRAJ2000Right ascension (J2000)pos.eq.ra;meta.mainDEJ2000Declination (J2000)pos.eq.dec;meta.mainzp? Photometric redshift, this worksrc.redshift.photfloatnullablee_zp? rms uncertainty on zpstat.errorfloatnullablezbr? Photometric redshift, Broadhurst et al. (2005, Cat. <J/ApJ/621/53>)src.redshift.photfloatnullableE_zbr? Error on zbr (upper limit)stat.error;stat.maxfloatnullablee_zbr? Error on zbr (lower limit)stat.errorfloatnullablezs? Spectroscopic redshift from r_zssrc.redshiftfloatnullabler_zs[def, ] Reference for zs (1)meta.ref;pos.framechar