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The VIMOS Ultra Deep Survey first data release: Spectra and spectroscopic redshifts of 698 objects up to Z_(spec) ~ 6 in CANDELS

Tasca, L. A. M. and Capak, P. and Scoville, N. (2017) The VIMOS Ultra Deep Survey first data release: Spectra and spectroscopic redshifts of 698 objects up to Z_(spec) ~ 6 in CANDELS. Astronomy & Astrophysics, 600 . Art. No. A110. ISSN 0004-6361. https://resolver.caltech.edu/CaltechAUTHORS:20170602-095554506

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Abstract

This paper describes the first data release (DR1) of the VIMOS Ultra Deep Survey (VUDS). The VUDS-DR1 is the release of all low-resolution spectroscopic data obtained in 276.9 arcmin^2 of the CANDELS-COSMOS and CANDELS-ECDFS survey areas, including accurate spectroscopic redshifts zspec and individual spectra obtained with VIMOS on the ESO-VLT. A total of 698 objects have a measured redshift, with 677 galaxies, two type-I AGN, and a small number of 19 contaminating stars. The targets of the spectroscopic survey are selected primarily on the basis of their photometric redshifts to ensure a broad population coverage. About 500 galaxies have z_(spec) > 2, 48 of which have z_(spec) > 4; the highest reliable redshifts reach beyond z_(spec) = 6. This data set approximately doubles the number of galaxies with spectroscopic redshifts at z > 3 in these fields. We discuss the general properties of the VUDS–DR1 sample in terms of the spectroscopic redshift distribution, the distribution of Lyman-α equivalent widths, and physical properties including stellar masses M_⋆ and star formation rates derived from spectral energy distribution fitting with the knowledge of z_(spec). We highlight the properties of the most massive star-forming galaxies, noting the wide range in spectral properties, with Lyman-α in emission or in absorption, and in imaging properties with compact, multi-component, or pair morphologies. We present the catalogue database and data products. All VUDS-DR1 data are publicly available and can be retrieved from a dedicated query-based database. Future VUDS data releases will follow this VUDS-DR1 to give access to the spectra and associated measurement of ~8000 objects in the full ~1 square degree of the VUDS survey.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1051/0004-6361/201527963DOIArticle
https://www.aanda.org/articles/aa/abs/2017/04/aa27963-15/aa27963-15.htmlPublisherArticle
https://arxiv.org/abs/1602.01842arXivDiscussion Paper
ORCID:
AuthorORCID
Capak, P.0000-0003-3578-6843
Scoville, N.0000-0002-0438-3323
Additional Information:© ESO, 2017 Received: 15 December 2015 Accepted: 26 May 2016 This work is supported by funding from the European Research Council Advanced Grant ERC–2010–AdG–268107–EARLY and by INAF Grants PRIN 2010, PRIN 2012 and PICS 2013. A.C., O.C., M.T., and V.S. acknowledge the grant MIUR PRIN 2010–2011. This work is based on data products made available at the CESAM data center, Laboratoire d’Astrophysique de Marseille, France.
Group:Astronomy Department
Funders:
Funding AgencyGrant Number
European Research Council Advanced GrantERC-2010-AdG-268107-EARLY
Istituto Nazionale di Astrofisica (INAF)PRIN 2010
Istituto Nazionale di Astrofisica (INAF)PRIN 2012
Istituto Nazionale di Astrofisica (INAF)PICS 2013
Subject Keywords:galaxies: distances and redshifts – galaxies: high-redshift – cosmology: observations – surveys – catalogs
Record Number:CaltechAUTHORS:20170602-095554506
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20170602-095554506
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:77913
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:02 Jun 2017 18:11
Last Modified:03 Oct 2019 18:03

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