Lyman-break galaxies from GALEX

DOI

Ultraviolet (UV) galaxies have been selected from the Galaxy Evolution Explorer deep imaging survey. The presence of a far-UV (FUV) drop-out in their spectral energy distributions (SEDs) proved to be a very complete (83.3 per cent) but not very efficient (21.4 per cent) tool for identifying Lyman break galaxies (LBGs) at z~1. In this paper, we explore the physical properties of these galaxies and how they contribute to the total star formation rate (SFR).

Cone search capability for table J/MNRAS/380/986/table1 (*Ultraviolet-selected sample down to within COMBO 17 (C17) field of view with magnitudes estimated from daophot)

Cone search capability for table J/MNRAS/380/986/table3 (The Lyman break galaxies (LBG) sample 0.9<=z<=1.3, as defined in the text, is listed here)

Identifier
DOI http://doi.org/10.26093/cds/vizier.73800986
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/MNRAS/380/986
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/380/986
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/380/986
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/MNRAS/380/986
Provenance
Creator Burgarella D.; Le Floc'h E.; Takeuchi T.T.; Huang J.S.; Buat V.,Rieke G.H.; Tyler K.D.
Publisher CDS
Publication Year 2008
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Cosmology; Galactic and extragalactic Astronomy; Natural Sciences; Observational Astronomy; Physics