J/AJ/141/14ivo://CDS.VizieR/J/AJ/141/14doi:10.26093/cds/vizier.51410014CDSStraughn A.N.Kuntschner H.Kummel M.Walsh J.R.Cohen S.H.,Gardner J.P.Windhorst R.A.O'Connell R.W.Pirzkal N.Meurer G.,McCarthy P.J.Hathi N.P.Malhotra S.Rhoads J.Balick B.Bond H.E.,Calzetti D.Disney M.J.Dopita M.A.Frogel J.A.Hall D.N.B.,Holtzman J.A.Kimble R.A.Mutchler M.Paresce F.Saha A.Silk J.I.,Trauger J.T.Walker A.R.Whitmore B.C.Young E.T.Xu C.2018-01-30T07:18:24Z2012-08-11T18:30:05ZCDS support team

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

cds-question@unistra.frgalaxiesinfrared-sourcesredshiftedspectroscopyline-intensitiesWe present grism spectra of emission-line galaxies (ELGs) from 0.6 to 1.6um from the Wide Field Camera 3 (WFC3) on the Hubble Space Telescope. These new infrared grism data augment previous optical Advanced Camera for Surveys G800L 0.6-0.95um grism data in GOODS-South from the PEARS program, extending the wavelength coverage well past the G800L red cutoff. The Early Release Science (ERS) grism field was observed at a depth of two orbits per grism, yielding spectra of hundreds of faint objects, a subset of which is presented here. ELGs are studied via the H{alpha}, [OIII], and [OII] emission lines detected in the redshift ranges 0.2~<z~<1.4, 1.2~<z~<2.2, and 2.0~<z~<3.3, respectively, in the G102 (0.8-1.1um; R~=210) and G141 (1.1-1.6um; R~=130) grisms.2011AJ....141...14Shttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/141/14CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toII/261 : GOODS initial results (Giavalisco+, 2004)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/AJ/141/14https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/141/14http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/141/14https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/141/14https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/141/14http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AJ/141/14GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/AJ/141/14/table1 (Global properties of 51 emission-line galaxies (ELG))https://vizier.cds.unistra.fr/viz-bin/conesearch/J/AJ/141/14/table1?https://vizier.iucaa.in/viz-bin/conesearch/J/AJ/141/14/table1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/AJ/141/14/table1?GETtext/xml+votable180.050000true53.04842-27.70953360.0055555555555555566/359351.8535694155097437e-19 2.1741002249411206e-19https://cdsarc.cds.unistra.fr/viz-bin/moc/J/AJ/141/14?format=asciiOpticalInfrareddefaultJ/AJ/141/14/table1Global properties of 51 emission-line galaxies (ELG)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintID[3/583] ID number <[SKK2011] NNN> in Simbadmeta.id;meta.mainintn_ID[ab] Note on source (1)meta.notecharRAJ2000Right ascension in decimal degrees (J2000)degpos.eq.ra;meta.mainDEJ2000Declination in decimal degrees (J2000)degpos.eq.dec;meta.mainF098MHST/WFC3 F098M (Ys) AB magnitudemagphot.mag;em.IR.Jfloatlambda[800/16636] Wavelength of line0.1nmem.wl;spect.lineintFlux? Flux (10^-18^erg/cm^2^/s) (2)zW.m**-2phot.fluxfloatnullablee_Flux? rms uncertainty on FluxzW.m**-2stat.error;phot.fluxintnullableEW? Equivalent width of line (2)0.1nmspect.line.eqWidthintnullableLineLine identification (3)meta.id;spect.lineSFR? Stellar formation rate (2)solMass/yrarith.rate;phys.SFRfloatnullablee_SFR? rms uncertainty on SFRsolMass/yrstat.error;phys.SFRintnullablez? Grism redshift, recalculated redshift based on the line identificationsrc.redshiftfloatnullableFlag? Flag for source of input redshift used for line identification (4)meta.code.errorintnullable