Stacking catalog sources in WMAP data
  We stack WMAP 7-year temperature data around extragalactic point sources,
showing that the profiles are consistent with WMAP's beam models, in
disagreement with the findings of Sawangwit & Shanks (2010). These results
require that the source sample's selection is not biased by CMB fluctuations.
We compare profiles from sources in the standard WMAP catalog, the WMAP catalog
selected from a CMB-free combination of data, and the NVSS catalog, and
quantify the agreement with fits to simple parametric beam models. We estimate
the biases in source profiles due to alignments with positive CMB fluctuations,
finding them roughly consistent with those biases found with the WMAP standard
catalog. Addressing those biases, we find source spectral indices significantly
steeper than those used by WMAP, with strong evidence for spectral steepening
above 61 GHz. Such changes modify the power spectrum correction required for
unresolved point sources, and tend to weaken somewhat the evidence for
deviation from a Harrison-Zel'dovich primordial spectrum, but more analysis is
required. Finally, we discuss implications for current CMB experiments.
