Galaxy Linewidths to z=1 from the DEEP Survey

Details Galaxy Linewidths to z=1 from the DEEP Survey Galaxy Linewidths to z=1 from the DEEP Survey

Nov 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aas...198.9312w&link_type=abstract

American Astronomical Society, 198th AAS Meeting, #93.12; Bulletin of the American Astronomical Society, Vol. 33, p.1180

Astronomy and Astrophysics

Astronomy

Scientific paper

The DEEP Project (Deep Extragalactic Evolutionary Probe) is a survey of faint field galaxies. DEEP has obtained moderate resolution Keck/LRIS spectra for several hundred galaxies at redshifts out to z ~ 1.3, in the Hubble Deep Field and Groth Survey Strip, fields with deep HST imaging. We discuss the use of optical emission linewidths and HST surface photometry to determine the existence and evolution of the linewidth-magnitude relation.

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