KISS emission-line galaxy candidates. IV Virtual Observatory Resource

Authors
  1. Salzer J.J.
  2. Jangren A.
  3. Gronwall C.
  4. Werk J.K.
  5. Chomiuk L.B.,Caperton K.A.
  6. Melbourne J.
  7. Mckinstry K.
  8. Published by
    CDS
Abstract

Spectroscopic observations for 614 emission-line galaxy (ELG) candidates from the KPNO International Spectroscopic Survey (KISS) have been obtained using the KPNO 2.1m telescope and the WIYN 3.5m telescope. KISS is a wide-field objective-prism survey for extragalactic emission-line objects that has cataloged over 2400 ELG candidates to date. Spectroscopic follow-up observations are being carried out at several telescopes to study the characteristics of the survey objects. We present the following data derived from the KPNO spectra: redshifts, reddening estimates, line equivalent widths, H{alpha} line fluxes, and emission-line ratios. The galaxies have been classified based on their emission-line characteristics.

Keywords
  1. Redshifted
  2. Line intensities
  3. Spectroscopy
  4. Galaxies
Bibliographic source Bibcode
2005AJ....130.2584S
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/130/2584
IVOA Identifier IVOID
ivo://CDS.VizieR/J/AJ/130/2584
Document Object Identifer DOI
doi:10.26093/cds/vizier.51302584

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History

2020-08-16T17:13:23Z
Resource record created
2020-08-16T17:13:23Z
Created
2021-03-29T14:51:10Z
Updated

Contact

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CDS support team
Postal Address
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
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cds-question@unistra.fr