Rest-frame Optical Imaging Of z 2-3 Galaxies With HST/WFC3

Details Rest-frame Optical Imaging Of z 2-3 Galaxies With HST/WFC3 Rest-frame Optical Imaging Of z 2-3 Galaxies With HST/WFC3

Jan 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aas...21721105l&link_type=abstract

American Astronomical Society, AAS Meeting #217, #211.05; Bulletin of the American Astronomical Society, Vol. 43, 2011

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I will describe some early results from an ongoing HST/WFC3 rest-frame optical imaging survey of star-forming galaxies in the redshift range 1.5 < z < 3.5. With 42 orbits of F160W imaging distributed amongst 10 survey fields, our survey will cover 65 square arcmin to a depth of 27.9 AB and contain > 300 spectroscopically confirmed galaxies with stellar masses in the range M* = 1e9 - 1e11 solar masses. I will discuss the typical morphological properties of these galaxies, the relation between morphology and the strength of galactic-scale gaseous outflows, and the form of the mass-radius relation in comparison to local galaxy samples.

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