Probing CMB Secondary Anisotropies through Minkowski Functionals
  Secondary contributions to the anisotropy of the Cosmic Microwave Background
(CMB), such as the integrated Sachs-Wolfe (ISW) effect, the thermal
Sunyaev-Zel'dovich effect (tSZ), and the effect of gravitational lensing, have
distinctive non-Gaussian signatures, and full descriptions therefore require
information beyond that contained in their power spectra. In this paper we use
the recently introduced skew-spectra associated with the Minkowski Functionals
(MF) to probe the topology of CMB maps to probe the secondary non-Gaussianity
as a function of beam-smoothing in order to separate various contributions. We
devise estimators for these spectra in the presence of a realistic
observational masks and present expressions for their covariance as a function
of instrumental noise. Specific results are derived for the mixed ISW-lensing
and tSZ-lensing bispectra as well as contamination due to point sources for
noise levels that correspond to the Planck (143 GHz channel) and EPIC (150 GHz
channel) experiments. The cumulative signal to noise ration $S/N$ for one-point
generalized skewness-parameters can reach an order of ${\cal O}(10)$ for Planck
and two orders of magnitude higher for EPIC, i.e. ${\cal O}(10^3)$. We also
find that these three spectra skew-spectra are correlated, having correlation
coefficients $r \sim 0.5-1.0$; higher $l$ modes are more strongly correlated.
Though the values of $S/N$ increase with decreasing noise, the triplets of
skew-spectra that determine the MFs bcome more correlated; the $S/N$ ratios of
lensing-induced skew-spectra are smaller compared to that of a
frequency-cleaned tSZ map.
