HDF-N Caltech faint galaxy redshift survey. XIII.

DOI

We introduce a new empirical function for modeling the spectral energy distributions (SEDs) of galaxies. We apply it to a sample of 590 galaxies in the region of the Hubble Deep Field (HDF) with z<1.5 using multicolor photometry with wide wavelength coverage combined with spectroscopic redshifts from our 93% complete R-selected redshift survey there.

Cone search capability for table J/AJ/121/2895/SED (SED parameters for the objects observed)

Cone search capability for table J/AJ/121/2895/redshift (Additions and corrections of redhifts)

Identifier
DOI http://doi.org/10.26093/cds/vizier.51212895
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/AJ/121/2895
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/121/2895
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/AJ/121/2895
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/AJ/121/2895
Provenance
Creator Cohen J.G.
Publisher CDS
Publication Year 2009
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