Astronomy and Astrophysics – Astronomy
Scientific paper
Jan 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aas...21531406k&link_type=abstract
American Astronomical Society, AAS Meeting #215, #314.06; Bulletin of the American Astronomical Society, Vol. 42, p.315
Astronomy and Astrophysics
Astronomy
Scientific paper
We present and analyze the rest-UV-through-radio Spectral Energy Distributions (SEDs) of high-redshift galaxies in the Extended Chandra Deep Field-South. Galaxies are separated into sets by their selection method (Lyman break, Lyman alpha emission, blue rest-UV colors) and into bins of photometric redshift. In order to obtain panchromatic SEDs for each set of galaxies, we performed stacking analyses in Spitzer-MIPS (24, 70 micron), sub-mm (870 microns from the Laboca ECDF-S Sub-mm Survey, LESS), and radio (VLA 1.4 GHz and GMRT 610 MHz). We describe our stacking methods, including an optimized treatment of the deblending of multiple galaxy types in the sub-mm imaging. The resulting SEDs are compared with low-redshift templates of galaxies with a variety of star-forming and AGN properties.
Gawiser Eric
Greve Thomas R.
Huynh Minh
Ivison Rob
Kurczynski Peter
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