UV selected sources in the GOODS-S field

DOI

Dust attenuation in galaxies is poorly known, especially at high redshift. And yet the amount of dust attenuation is a key parameter to deduce accurate star formation rates from ultraviolet (UV) rest-frame measurements. The wavelength dependence of the dust attenuation is also of fundamental importance to interpret the observed spectral energy distributions (SEDs) and to derive photometric redshifts or physical properties of galaxies. We want to study dust attenuation at UV wavelengths at high redshift, where the UV is redshifted to the observed visible light wavelength range. In particular, we search for a UV bump and related implications for dust attenuation determinations.

Cone search capability for table J/A+A/545/A141/catalog (Catalogue of UV selected sources in the GOODS-S field)

Identifier
DOI http://doi.org/10.26093/cds/vizier.35450141
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/545/A141
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/545/A141
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/545/A141
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/545/A141
Provenance
Creator Buat V.; Noll S.; Burgarella D.; Giovannoli E.; Charmandaris V.,Pannella M.; Hwang H.S.; Elbaz D.; Dickinson M.; Magdis G.; Reddy N.,Murphy E.J.
Publisher CDS
Publication Year 2012
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; Galactic and extragalactic Astronomy; Natural Sciences; Observational Astronomy; Physics