J/A+A/578/A30ivo://CDS.VizieR/J/A+A/578/A30doi:10.26093/cds/vizier.35780030CDSSanchez-portal M.Pintos-Castro I.Perez-Martinez R.Cepa J.,Perez Garcia A.M.Dominguez-Sanchez H.Bongiovanni A.Serra A.L.,Alfaro E.Altieri B.Aragon-Salamanca A.Balkowski C.Biviano A.,Bremer M.Castander F.Castaneda H.Castro-Rodriguez N.,Chies-santos A.L.Coia D.Diaferio A.Duc P.A.Ederoclite A.Geach J.,Gonzalez-Serrano I.Haines C.P.Mcbreen B.Metcalfe L.Oteo I.,Perez-Fournon I.Poggianti B.Polednikova J.Ramon-Perez M.,Rodriguez-Espinosa J.M.Santos J.S.Smail I.Smith G.P.Temporin S.,Valtchanov I.2017-10-03T05:12:39Z2015-09-25T08:17:27ZCDS support team

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

cds-question@unistra.frgalaxy-clustersactive-galactic-nucleivisible-astronomyh-alpha-photometryspectroscopyThe cores of clusters at 0<~z<~1 are dominated by quiescent early-type galaxies, whereas the field is dominated by star-forming late-type galaxies. Clusters grow through the accretion of galaxies and groups from the surrounding field, which implies that galaxy properties, notably the star formation ability, are altered as they fall into overdense regions. The critical issues for understanding this evolution are how the truncation of star formation is connected to the morphological transformation and what physical mechanism is responsible for these changes. The GaLAxy Cluster Evolution Survey (GLACE) is conducting a thorough study of the variations in galaxy properties (star formation, AGN activity, and morphology) as a function of environment in a representative and well-studied sample of clusters. To address these questions, the GLACE survey is making a deep panoramic survey of emission line galaxies (ELG), mapping a set of optical lines ([OII], [OIII], H{beta} and H{alpha}/[NII] when possible) in several galaxy clusters at z~0.40, 0.63, and 0.86. Using the tunable filters (TF) of the OSIRIS instrument at the 10.4m GTC telescope, the GLACE survey applies the technique of TF tomography: for each line, a set of images are taken through the OSIRIS TF, each image tuned at a different wavelength (equally spaced), to cover a rest frame velocity range of several thousand km/s centred on the mean cluster redshift, and scanned for the full TF field of view of an 8arcmin diameter. Here we present the first results of the GLACE project, targeting the H{alpha}/[NII] lines in the intermediate-redshift cluster ZwCl0024.0+1652 at z=0.395. Two pointings have been performed that cover ~2*r_vir_.2015A&A...578A..30Shttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/578/A30CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/578/A30https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/578/A30http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/578/A30https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/578/A30https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/578/A30http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/578/A30GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/578/A30/table5 (Catalogue of unique ELGs of Cl0024)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/578/A30/table5?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/578/A30/table5?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/578/A30/table5?GETtext/xml+votable180.050000true6.642791717.101250.0055555555555555566/19846https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/578/A30?format=asciiOpticaldefaultJ/A+A/578/A30/table5Catalogue of unique ELGs of Cl0024SimbadNameSimbad column added by the CDSmeta.idcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIDName, NNNN_C or NNNN_0 (1)meta.id;meta.maincharRAJ2000Right ascension (J2000)pos.eq.ra;meta.mainDEJ2000Declination (J2000)pos.eq.dec;meta.mainz[0.37/0.43] Redshiftsrc.redshiftfloatFHa[4/114] H{alpha} flux (10^-17^erg/cm^2^/s)1e-20W.m**-2phot.flux;em.line.Halphainte_FHa[1/30] rms uncertainty on FHa1e-20W.m**-2stat.errorintF[NII][1/66]? [NII] flux (10^-17^erg/cm^2^/s)1e-20W.m**-2phot.fluxintnullablee_F[NII][1/38]? rms uncertainty on F[NII]1e-20W.m**-2stat.errorintnullableEWHa[6/426] H{alpha} equivalent width0.1nmspect.line.eqWidth;em.line.HalphafloatEWHaN[11/438]? H{alpha}+[NII] equivalent width0.1nmspect.line.eqWidth;em.line.HalphafloatnullableClassGalaxy type: "SF" (star-forming), "BLAGN" (Broad-line), or "NLAGN" (narrow-line)src.classchar