J/A+AS/120/323ivo://CDS.VizieR/J/A+AS/120/323CDSGallego J.Zamorano J.Rego M.Alonso O.Vitores A.G.1997-12-09T18:22:46Z1997-12-09T19:22:41ZCDS support team

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

cds-question@unistra.frgalaxiesspectroscopySpectroscopic observations for the full sample of H{alpha} emission-line galaxy candidates (ELGs) from the Universidad Complutense de Madrid objective-prism survey Lists 1 and 2 have been obtained in order to investigate fully the properties of the survey constituents as well as the selection characteristics and completeness limits of the survey itself. The spectroscopic data include redshifts, line fluxes, equivalent widths, emission-line ratios, optical reddening estimates and synthesized color indexes. We find that 74% of the objects in this sample do exhibit emission lines. We compare our observational data with parameters given in the published survey lists in order to assess the usefulness of the latter. The different emission-line galaxies have been classified according to their spectra in several groups. Gray-scale images of the CCD spectra near the main emission lines, spatial profiles at the continuum and the line for [OIII]{lambda}5007 and H{alpha} lines, as well as plots of the coadded spectra of selected galaxies are presented, and a number of peculiar objects are described.1996A&AS..120..323Ghttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+AS/120/323CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/ApJS/95/387 : Survey of emission-line galaxies (Zamorano+ 1994)J/ApJS/95/387 : Universidad Complutense de Madrid list 1 (Zamorano+ 1994)J/ApJS/105/343 : Universidad Complutense de Madrid list 2 (Zamorano+ 1996)J/ApJS/122/415 : UCM list 3 (Alonso+, 1999)J/A+AS/118/7 : Photometry & morphology of UCM galaxies (Vitores+, 1996)J/AJ/105/427 : IRAS fluxes of UCM galaxies (Rego+ 1993)J/A+AS/141/409 : Photometry of UCM galaxies. I. (Perez-Gonzalez+, 2000)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+AS/120/323https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+AS/120/323http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+AS/120/323https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+AS/120/323https://vizier.iucaa.in/viz-bin/votable?-source=J/A+AS/120/323http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+AS/120/323GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapOpticaldefaultJ/A+AS/120/323/table4Summary of emission-line intensities[NII]bc? Reddening-corrected [NII](6584A) line flux (1)%spect.line.intensity;arith.ratiointHeIc? Reddening-corrected HeI line flux (1)%spect.line.intensity;arith.ratioint[SII]b? line flux of [SII]{lambda}6731 line flux (1)%spect.line.intensity;arith.ratiointrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintUCMUCM name (Zamorano et al., 1994ApJS...95..387Z)meta.id;meta.maincharm_UCMMultiplicity index on UCMmeta.code.multipchar[OII]? [OII]{lambda}3727 (1)%spect.line.intensity;arith.ratiointHgamma? Hgamma{lambda}4340 line flux (1)%spect.line.intensity;arith.ratiointHbeta? Hbeta{lambda}4861 line flux (1)%spect.line.intensity;arith.ratioint[OIII]a? [OIII]{lambda}4959 line flux (1)%spect.line.intensity;arith.ratioint[OIII]b? [OIII]{lambda}5007 line flux (1)%spect.line.intensity;arith.ratiointHeI? HeI{lambda}5976 line flux (1)%spect.line.intensity;arith.ratioint[OI]? [OI]{lambda}6300 line flux (1)%spect.line.intensity;arith.ratioint[NII]a? [NII]{lambda}6548 line flux (1)%spect.line.intensity;arith.ratiointHalpha? Halpha{lambda}6563 line flux (1)%phot.fluxint[NII]b? [NII]{lambda}6584 line flux (1)%spect.line.intensity;arith.ratioint[SII]a? line flux of [SII]{lambda}6716 line flux (1)%spect.line.intensity;arith.ratioint[OII]c? Reddening-corrected [OII] line flux (1)%spect.line.intensity;arith.ratiointHgammac? Reddening-corrected Hgamma line flux (1)%spect.line.intensity;arith.ratiointHbetac? Reddening-corrected Hbeta line flux (=100)%spect.line.intensity;arith.ratioint[OIII]ac? Reddening-corrected [OIII](4959A) line flux (1)%spect.line.intensity;arith.ratioint[OIII]bc? Reddening-corrected [OIII](5007A) line flux (1)%spect.line.intensity;arith.ratioint[OI]c? Reddening-corrected [OI] line flux (1)%spect.line.intensity;arith.ratioint[NII]ac? Reddening-corrected [NII](6548A) line flux (1)%spect.line.intensity;arith.ratiointHalphac? Reddening-corrected Halpha line flux (1)%spect.line.intensity;arith.ratioint[SII]ac? Reddening-corrected [SII](6716A) line flux (1)%spect.line.intensity;arith.ratioint[SII]bc? Reddening-corrected [SII](6731A) line flux (1)%spect.line.intensity;arith.ratiointJ/A+AS/120/323/table5Summary of spectroscopic datarecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintUCMName in Zamorano+, 1994ApJS...95..387Zmeta.id;meta.maincharm_UCMMultiplicity index on UCMmeta.code.multipcharzHeliocentric redshiftsrc.redshiftfloatSNRSignal-to-noise ratio at the continuum near Halpha (1)stat.snrintEW([OII])? Equivalent width for [OII]{lambda}3727 emission linenmspect.line.eqWidthfloatEW(Hbeta)Equivalent width for Hbeta emission linenmspect.line.eqWidthfloatEW([OIII])Equivalent width for [OIII]{lambda}5007 emission linenmspect.line.eqWidthfloatEW(Halpha)Equivalent width for Halpha emission linenmspect.line.eqWidthfloatFHbetaObserved Hbeta line flux1e-17W.m**-2phot.fluxfloatFHalpha? Observed blend Halpha+[NII] line flux1e-17W.m**-2phot.fluxfloatb-v? b-v synthetic color indexmagphot.color;em.opt.B;em.opt.Vfloatv-r? v-r synthetic color indexmagphot.color;em.opt.V;em.opt.RfloatE(B-V)? B-V color excessmagphot.color.excessfloatu_E(B-V)Uncertainty flag on E(B-V)meta.code.errorcharL(Halpha)? Observed Halpha luminosity1e+08solLumphys.luminosityfloatSpectSpectroscopic classificationsrc.spTypechar