IRAC and MIPS imaging of the HDF_S

Details IRAC and MIPS imaging of the HDF_S IRAC and MIPS imaging of the HDF_S

Sep 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004sptz.prop..214f&link_type=abstract

Spitzer Proposal ID #214

Physics

Scientific paper

We will image the WFPC2 field of the Hubble Deep Field South with IRAC,
in four bands (3.5-8 micron). Combined with the ultra-deep VLT
near-infrared imaging, we will determine the spectral energy
distributions of the high redshift galaxies to the restframe K band.
These SED's will be modeled using stellar population synthesis models.

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