HST Galaxy Evolution from Morphology and SEDs

DOI

GEMs is a large-area (800 arcmin 2) two-color (F606W and F850LP) imaging survey with the Advanced Camera for Surveys on the Hubble Space Telescope. Centered on the Chandra Deep Field-South, it covers an area of ~ 28'x28', or about 120 HDF areas, to a depth of MAB(F606W)=28.5(5s) for compact sources. Focusing on the redshift range ~ 0.2<z<1.1, GEMS provides morphologies and structural parameters for nearly 10,000 galaxies where redshift estimates, luminosities, and SEDs exist from COMBO-17.

Identifier
DOI http://doi.org/10.17909/T90010
Source https://dc.g-vo.org/rr/q/lp/custom/mast.stsci/siap/hst.gems
Related Identifier http://archive.stsci.edu/prepds/gems/
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://mast.stsci/siap/hst.gems
Provenance
Creator Rix, et al
Instrument ACS
Publisher Space Telescope Science Institute Archive
Publication Year 2004
OpenAccess true
Contact Archive Branch, STScI <archive(at)stsci.edu>
Representation
Resource Type Other; AstroObjects
Version 1.0
Discipline Astrophysics and Astronomy; Natural Sciences; Observational Astronomy; Physics