Integrated Cosmological Probes: Extended Analysis
  Recent progress in cosmology has relied on combining different cosmological
probes. In earlier work, we implemented an integrated approach to cosmology
where the probes are combined into a common framework at the map level. This
has the advantage of taking full account of the correlations between the
different probes, to provide a stringent test of systematics and of the
validity of the cosmological model. We extend this analysis to include not only
CMB temperature, galaxy clustering, weak lensing from SDSS but also CMB
lensing, weak lensing from the DES SV survey, Type Ia SNe and $H_{0}$
measurements. This yields 12 auto- and cross-power spectra as well as
background probes. Furthermore, we extend the treatment of systematic
uncertainties. For $\Lambda$CDM, we find results that are consistent with our
earlier work. Given our enlarged data set and systematics treatment, this
confirms the robustness of our analysis and results. Furthermore, we find that
our best-fit cosmological model gives a good fit to the data we consider with
no signs of tensions within our analysis. We also find our constraints to be
consistent with those found by WMAP9, SPT and ACT and the KiDS weak lensing
survey. Comparing with the Planck Collaboration results, we see a broad
agreement, but there are indications of a tension from the marginalized
constraints in most pairs of cosmological parameters. Since our analysis
includes CMB temperature Planck data at $10 < \ell < 610$, the tension appears
to arise between the Planck high$-\ell$ and the other measurements.
Furthermore, we find the constraints on the probe calibration parameters to be
in agreement with expectations, showing that the data sets are mutually
consistent. In particular, this yields a confirmation of the amplitude
calibration of the weak lensing measurements from SDSS, DES SV and Planck CMB
lensing from our integrated analysis. [abridged]
