##### AUTHOR ####
Giovanni G. Fazio

##### TITLE ####
Status of the Spitzer Warm Mission SEDS Program  

##### ABSTRACT ####
The Spitzer Extended Deep Survey (SEDS) will provide a unique opportunity to obtain
the first complete census of the assembly of stellar mass and black holes as a function
of cosmic time back to the era of reionization, yielding unique information on galaxy
formation in the early Universe.  The survey will also measure galaxy clustering
over a wide redshift range, which will provide the critical link between galaxies
and their dark matter halos and critical tests of models of early star formation.
SEDS will achieve these goals by tracing the stellar mass growth in mass-selected
samples of galaxies via their broadband spectral energy distributions.  Spitzer Warm
Mission observations of the SEDS program have been initiated.   The status and quality
of the observations will be described as well as plans and timetables to compete
the program.