Determining the formation epoch of dwarf galaxies using the HST/ACS Ultra Deep Field

Details Determining the formation epoch of dwarf galaxies using the HST/ACS Ultra Deep Field Determining the formation epoch of dwarf galaxies using the HST/ACS Ultra Deep Field

Jul 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004hst..prop10321g&link_type=abstract

HST Proposal ID #10321

Computer Science

Hst Proposal Id #10321 Galaxies

Scientific paper

We will analyze the outer parts of the surface brightness and color profiles of dwarf star-forming galaxies at redshifts between 06} or if this formation was delayed up to z 1-2 by the intense UV-radiation field present at higher redshifts. The depth and high spatial resolution of the UDF are required in order to detect the low-surface-brightness stellar population associated with the galaxy halo and to separate and spatially resolve it from the central, high-surface-brightness component.

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