The Mass-radius Relation For Starforming Galaxies At z ˜ 2-3

Details The Mass-radius Relation For Starforming Galaxies At z ˜ 2-3 The Mass-radius Relation For Starforming Galaxies At z ˜ 2-3

Jan 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aas...21733506n&link_type=abstract

American Astronomical Society, AAS Meeting #217, #335.06; Bulletin of the American Astronomical Society, Vol. 43, 2011

Astronomy and Astrophysics

Astronomy

Scientific paper

We present 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 ultimately 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. We discuss the form of the relation between stellar mass and rest-frame optical effective radius, how this relation evolves from z ˜ 3 to z ˜ 1.5, and how it compares to the local starforming galaxy population.

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