Catalog Service: HDF-N Caltech faint galaxy redshift survey. XIII.
Description
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.
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Publisher: CDSivo://CDS[Pub. ID]
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This resource was registered on: 2009 Apr 28 11:24:08ZThis resource description was last updated on: 2021 Oct 21 00:00:00Z
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This is service that does not comply with any IVOA standard but instead provides access to special capabilities specific to this resource.
This is a standard IVOA service that takes as input an ADQL or PQL query and returns tabular data.
This is a standard IVOA service that takes as input a position in the sky and a radius and returns catalog records with positions within that radius.
Cone search capability for table J/AJ/121/2895/SED (SED parameters for the objects observed)
VERB=1
VERB=3
Cone search capability for table J/AJ/121/2895/redshift (Additions and corrections of redhifts)
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