J/A+AS/120/323 J/A+AS/120/323 Long-slit spectroscopy of UCM galaxies J Gallego J Zamorano M Rego O Alonso A G Vitores Astron. Astrophys. Suppl. Ser. 120 323 1996 1996A&AS..120..323G Galaxies, spectra galaxies: distances and redshifts galaxies: starburst surveys Spectroscopic 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.

UCM UCM name (Zamorano et al., 1994ApJS...95..387Z) --- m_UCM Multiplicity index on UCM --- [OII] [OII]{lambda}3727 number=1 Line fluxes are relative to Hbeta=100 for all emission lines detected. In case of no Hbeta line apparent, the fluxes are given relatives to Halpha=100. % Hgamma Hgamma{lambda}4340 line flux number=1 Line fluxes are relative to Hbeta=100 for all emission lines detected. In case of no Hbeta line apparent, the fluxes are given relatives to Halpha=100. % Hbeta Hbeta{lambda}4861 line flux number=1 Line fluxes are relative to Hbeta=100 for all emission lines detected. In case of no Hbeta line apparent, the fluxes are given relatives to Halpha=100. % [OIII]a [OIII]{lambda}4959 line flux number=1 Line fluxes are relative to Hbeta=100 for all emission lines detected. In case of no Hbeta line apparent, the fluxes are given relatives to Halpha=100. % [OIII]b [OIII]{lambda}5007 line flux number=1 Line fluxes are relative to Hbeta=100 for all emission lines detected. In case of no Hbeta line apparent, the fluxes are given relatives to Halpha=100. % HeI HeI{lambda}5976 line flux number=1 Line fluxes are relative to Hbeta=100 for all emission lines detected. In case of no Hbeta line apparent, the fluxes are given relatives to Halpha=100. % [OI] [OI]{lambda}6300 line flux number=1 Line fluxes are relative to Hbeta=100 for all emission lines detected. In case of no Hbeta line apparent, the fluxes are given relatives to Halpha=100. % [NII]a [NII]{lambda}6548 line flux number=1 Line fluxes are relative to Hbeta=100 for all emission lines detected. In case of no Hbeta line apparent, the fluxes are given relatives to Halpha=100. % Halpha Halpha{lambda}6563 line flux number=1 Line fluxes are relative to Hbeta=100 for all emission lines detected. In case of no Hbeta line apparent, the fluxes are given relatives to Halpha=100. % [NII]b [NII]{lambda}6584 line flux number=1 Line fluxes are relative to Hbeta=100 for all emission lines detected. In case of no Hbeta line apparent, the fluxes are given relatives to Halpha=100. % [SII]a line flux of [SII]{lambda}6716 line flux number=1 Line fluxes are relative to Hbeta=100 for all emission lines detected. In case of no Hbeta line apparent, the fluxes are given relatives to Halpha=100. % [SII]b line flux of [SII]{lambda}6731 line flux number=1 Line fluxes are relative to Hbeta=100 for all emission lines detected. In case of no Hbeta line apparent, the fluxes are given relatives to Halpha=100. % [OII]c Reddening-corrected [OII] line flux number=1 Line fluxes are relative to Hbeta=100 for all emission lines detected. In case of no Hbeta line apparent, the fluxes are given relatives to Halpha=100. % Hgammac Reddening-corrected Hgamma line flux number=1 Line fluxes are relative to Hbeta=100 for all emission lines detected. In case of no Hbeta line apparent, the fluxes are given relatives to Halpha=100. % Hbetac Reddening-corrected Hbeta line flux (=100) % [OIII]ac Reddening-corrected [OIII](4959A) line flux number=1 Line fluxes are relative to Hbeta=100 for all emission lines detected. In case of no Hbeta line apparent, the fluxes are given relatives to Halpha=100. % [OIII]bc Reddening-corrected [OIII](5007A) line flux number=1 Line fluxes are relative to Hbeta=100 for all emission lines detected. In case of no Hbeta line apparent, the fluxes are given relatives to Halpha=100. % HeIc Reddening-corrected HeI line flux number=1 Line fluxes are relative to Hbeta=100 for all emission lines detected. In case of no Hbeta line apparent, the fluxes are given relatives to Halpha=100. % [OI]c Reddening-corrected [OI] line flux number=1 Line fluxes are relative to Hbeta=100 for all emission lines detected. In case of no Hbeta line apparent, the fluxes are given relatives to Halpha=100. % [NII]ac Reddening-corrected [NII](6548A) line flux number=1 Line fluxes are relative to Hbeta=100 for all emission lines detected. In case of no Hbeta line apparent, the fluxes are given relatives to Halpha=100. % Halphac Reddening-corrected Halpha line flux number=1 Line fluxes are relative to Hbeta=100 for all emission lines detected. In case of no Hbeta line apparent, the fluxes are given relatives to Halpha=100. % [NII]bc Reddening-corrected [NII](6584A) line flux number=1 Line fluxes are relative to Hbeta=100 for all emission lines detected. In case of no Hbeta line apparent, the fluxes are given relatives to Halpha=100. % [SII]ac Reddening-corrected [SII](6716A) line flux number=1 Line fluxes are relative to Hbeta=100 for all emission lines detected. In case of no Hbeta line apparent, the fluxes are given relatives to Halpha=100. % [SII]bc Reddening-corrected [SII](6731A) line flux number=1 Line fluxes are relative to Hbeta=100 for all emission lines detected. In case of no Hbeta line apparent, the fluxes are given relatives to Halpha=100. % UCM Name in Zamorano+, 1994ApJS...95..387Z --- m_UCM Multiplicity index on UCM --- z Heliocentric redshift --- SNR Signal-to-noise ratio at the continuum near Halpha number=1 SNR estimated by computing the ratio between the sigma in a 10nm band centered at 6540Angstroem (rest wavelength) and the mean flux in the same range --- EW([OII]) Equivalent width for [OII]{lambda}3727 emission line 0.1nm EW(Hbeta) Equivalent width for Hbeta emission line 0.1nm EW([OIII]) Equivalent width for [OIII]{lambda}5007 emission line 0.1nm EW(Halpha) Equivalent width for Halpha emission line 0.1nm FHbeta Observed Hbeta line flux 10-17W/m2 FHalpha Observed blend Halpha+[NII] line flux 10-17W/m2 b-v b-v synthetic color index mag v-r v-r synthetic color index mag E(B-V) B-V color excess mag u_E(B-V) Uncertainty flag on E(B-V) --- L(Halpha) Observed Halpha luminosity 10+8solLum Spect Spectroscopic classification --- table4.texLaTeX version of table4 table5.texLaTeX version of table5 Patricia Bauer CDS 1996May21Jesus Gallego <jgm@ucolick.org> J_A+AS_120_323.xml