Multiwavelength Morphologies of Star-Forming Galaxies at Intermediate Redshifts

Details Multiwavelength Morphologies of Star-Forming Galaxies at Intermediate Redshifts Multiwavelength Morphologies of Star-Forming Galaxies at Intermediate Redshifts

Jan 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aas...21733520b&link_type=abstract

American Astronomical Society, AAS Meeting #217, #335.20; Bulletin of the American Astronomical Society, Vol. 43, 2011

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We present preliminary work providing insight into the formation epoch of the Hubble types. We use HST (ACS and WFC3) multiple wavelengths (FUV, U, B, V, i, z, J, H, K, where available) images to analyze the morphology of a sample of 317 star-forming galaxies. This sample is FUV-selected containing star-forming galaxies at intermediate-redshifts (0.1 < z < 1) in the Great Observatories Origins Deep Survey (GOODS) fields. We investigate quantitative morphologies of galaxies versus their spectral types for the FUV sample using rest-frame optical GALFIT morphological parameters and spectral types obtained from GOODS catalogs.

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