Published in

The Mass of Galaxies at Low and High Redshift, p. 324-331

DOI: 10.1007/10899892_78

EDP Sciences, Astronomy & Astrophysics, (512), p. A12, 2010

DOI: 10.1051/0004-6361/200913626

EDP Sciences, Astronomy & Astrophysics, 2(494), p. 443-460, 2008

DOI: 10.1051/0004-6361:200809617

Links

Tools

Export citation

Search in Google Scholar

The great observatories origins deep survey

Journal article published in 2008 by E. Vanzella ORCID, H. Kuntschner, J. Haase, M. Nonino, P. Rosati, A. Grazian, L. A. Moustakas, A. Rettura, P. Popesso, A. Renzini, D. Stern, S. Cristiani, Mark Dickinson, Mauro Giavalisco, C. Cesarsky and other authors.
This paper is made freely available by the publisher.
This paper is made freely available by the publisher.

Full text: Download

Question mark in circle
Preprint: policy unknown
Upload
Question mark in circle
Postprint: policy unknown
Upload
Question mark in circle
Published version: policy unknown
Upload

Abstract

We present the full data set of the VIMOS spectroscopic campaign of the ESO/GOODS program in the CDFS, which complements the FORS2 ESO/GOODS spectroscopic campaign. The GOODS/VIMOS spectroscopic campaign is structured in two separate surveys using two different VIMOS grisms. The VIMOS Low Resolution Blue (LR-Blue) and Medium Resolution (MR) orange grisms have been used to cover different redshift ranges. The LR-Blue campaign is aimed at observing galaxies mainly at 1.8<z<3.5, while the MR campaign mainly aims at galaxies at z<1 and Lyman Break Galaxies (LBGs) at z>3.5. The full GOODS/VIMOS spectroscopic campaign consists of 20 VIMOS masks. This release adds 8 new masks to the previous release (12 masks, Popesso et al. 2009). In total we obtained 5052 spectra, 3634 from the 10 LR-Blue masks and 1418 from the 10 MR masks. A significant fraction of the extracted spectra comes from serendipitously observed sources: ~21% in the LR-Blue and ~16% in the MR masks. We obtained 2242 redshifts in the LR-Blue campaign and 976 in the MR campaign for a total success rate of 62% and 69% respectively, which increases to 66% and 73% if only primary targets are considered. The typical redshift uncertainty is estimated to be ~0.0012 (~255 km/s) for the LR-Blue grism and ~0.00040 (~120 km/s) for the MR grism. By complementing our VIMOS spectroscopic catalog with all existing spectroscopic redshifts publicly available in the CDFS, we compiled a redshift master catalog with 7332 entries, which we used to investigate large scale structures out to z~3.7. We produced stacked spectra of LBGs in a few bins of equivalent width (EW) of the Ly-alpha and found evidence for a lack of bright LBGs with high EW of the Ly-alpha. Finally, we obtained new redshifts for 12 X-ray sources of the CDFS and extended-CDFS. Comment: 22 pages, 20 figures, accepted for publication on Astronomy and Astrophysics, catalogs and data products are available at http://archive.eso.org/cms/eso-data/data-packages/goods-vimos-spectroscopy-data-release-version-2.0/, for ESO-GOODS related material consult http://www.eso.org/sci/activities/projects/goods/