Spectral Energy Distributions of the High-Redshift 4C Sources: Testing Unification

Details Spectral Energy Distributions of the High-Redshift 4C Sources: Testing Unification Spectral Energy Distributions of the High-Redshift 4C Sources: Testing Unification

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008sptz.prop50040f&link_type=abstract

Spitzer Proposal ID #50040

Physics

Scientific paper

We propose IRAC and IRS peakup photometry of high-redshift (z>1.5) radio galaxies and quasars. This is a followup to previous proposals in cycle 4. It will add IRAC and 16-micron data for galaxies having only MIPS observations. The galaxy spectral energy distributions will enable us to determine the stellar luminosity and mass and will help separate AGN from starburst emission.

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