Physical properties of VVDS galaxies Virtual Observatory Resource

Authors
  1. Lamareille F.
  2. Brinchmann J.
  3. Contini T.
  4. Walcher C.J.
  5. Charlot S.,Perez-Montero E.
  6. Zamorani G.
  7. Pozzetti L.
  8. Bolzonella M.
  9. Garilli B.,Paltani S.
  10. Bongiorno A.
  11. Le Fevre O.
  12. Bottini D.
  13. Le Brun V.
  14. Maccagni D.,Scaramella R.
  15. Scodeggio M.
  16. Tresse L.
  17. Vettolani G.
  18. Zanichelli A.,Adami C.
  19. Arnouts S.
  20. Bardelli S.
  21. Cappi A.
  22. Ciliegi P.
  23. Foucaud S.,Franzetti P.
  24. Gavignaud I.
  25. Guzzo L.
  26. Ilbert O.
  27. Iovino A.
  28. McCracken H.J.,Marano B.
  29. Marinoni C.
  30. Mazure A.
  31. Meneux B.
  32. Merighi R.
  33. Pello R.,Pollo A.
  34. Radovich M.
  35. Vergani D.
  36. Zucca E.
  37. Romano A.
  38. Grado A.,Limatola L.
  39. Published by
    CDS
Abstract

We want to derive the mass-metallicity relation of star-forming galaxies up to z~0.9, using data from the VIMOS VLT Deep Survey. The mass-metallicity relation is commonly understood as the relation between the stellar mass and the gas-phase oxygen abundance. Automatic measurement of emission-line fluxes and equivalent widths have been performed on the full spectroscopic sample of the VIMOS VLT Deep Survey. This sample is divided into two sub-samples depending on the apparent magnitude selection: wide (I_AB_<22.5) and deep (I_AB_<24). These two samples span two different ranges of stellar masses. Emission-line galaxies have been separated into star-forming galaxies and active galactic nuclei using emission line ratios. For the star-forming galaxies the emission line ratios have also been used to estimate gas-phase oxygen abundance, using empirical calibrations renormalized in order to give consistent results at low and high redshifts. The stellar masses have been estimated by fitting the whole spectral energy distributions with a set of stellar population synthesis models.

Keywords
  1. surveys
  2. galaxies
  3. spectroscopy
  4. line-intensities
Bibliographic source Bibcode
2009A&A...495...53L
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/495/53
IVOA Identifier IVOID
ivo://CDS.VizieR/J/A+A/495/53
Document Object Identifer DOI
doi:10.26093/cds/vizier.34950053

Access

IVOA Table Access TAP
https://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).
IVOA Cone Search SCS
For use with a cone search client (e.g., TOPCAT).
https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/495/53/catalog?
https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/495/53/catalog?
http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/495/53/catalog?

History

2009-07-29T06:12:29Z
Resource record created
2009-07-29T06:12:29Z
Created
2009-07-29T06:18:59Z
Updated

Contact

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