Improving CMB non-Gaussianity estimators using tracers of local structure

Abstract

Local non-Gaussianity causes correlations between large scale perturbation modes and the small scale power. The large-scale CMB signal has contributions from the integrated Sachs Wolfe (ISW) effect, which does not correlate with the small scale power. If this ISW contribution can be removed, the sensitivity to local non-Gaussianity is improved. Gravitational lensing and galaxy counts can be used to trace the ISW contribution; in particular we show that the CMB lensing potential is highly correlated with the ISW signal. We construct a nearly-optimal estimator for the local non-Gaussianity parameter $\fnl$ and investigate to what extent we can use this to decrease the variance on ${\fnl}$. We show that the variance can be decreased by up to $20\%$ at Planck sensitivity using galaxy counts. CMB lensing is a good bias-independent ISW tracer for future more sensitive observations, though the fractional decrease in variance is small if good polarization data is also available.

8 pages, 3 figures. Comments welcome

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Cited by in corpus (6)

• The shape of the CMB lensing bispectrum
• The full squeezed CMB bispectrum from inflation
• Non-Gaussianity in Large Scale Structure and Minkowski Functionals
• Long range correlation in cosmic microwave background radiation
• Removing the ISW-lensing bias from the local-form primordial non-Gaussianity estimation
• An improved estimator for non-Gaussianity in cosmic microwave background observations