  We cross correlate the large-scale cosmic microwave background (CMB) sky
measured by WMAP with two probes of large-scale structure at z ~ 1. The hard
X-ray background, measured by the HEAO-1 satellite, is positively correlated
with the WMAP data at the 2.5-3.0 sigma level. The number counts of radio
galaxies in the NVSS survey are also correlated at a slightly weaker level
(2.-2.5 sigma). These correlations appear to arise from both hemispheres on the
sky and are resilient to changes in the levels of masking of the Galaxy and
point sources, suggesting that foregrounds are not responsible for the signal.
The implication is that some of the observed CMB fluctuations arise at low
redshifts. The level of the correlations is consistent with that expected for
the cosmological constant (Omega_Lambda = 0.72) concordance model resulting
from the integrated Sachs-Wolfe effect. Thus, we may be observing dark energy's
effect on the growth of structure.
