This paper presents cosmological results based on full-mission Planck observations of
temperature and polarization anisotropies of the cosmic microwave background (CMB) …

We present the current accounting of systematic effect uncertainties for the Low Frequency
Instrument (LFI) that are relevant to the 2015 release of the Planck cosmological results …

This paper presents a study of the integrated Sachs-Wolfe (ISW) effect from the Planck 2015
temperature and polarization data release. This secondary cosmic microwave background …

We present a chrono-cosmography project, aiming at the inference of the four dimensional
formation history of the observed large scale structure from its origin to the present epoch. To …

We study the integrated Sachs-Wolfe (ISW) effect in ghost-free, massive bigravity. We focus
on the infinite-branch bigravity (IBB) model which exhibits viable cosmic expansion histories …

We use the integrated Sachs-Wolfe (ISW) effect, by now detectable at∼ 5 σ within the
context of Λ cold dark matter (Λ CDM) cosmologies, to place strong constraints on dynamical …

CMB photons redshift and blueshift as they move through gravitational potentials Φ while
propagating across the Universe. If the potential is not constant in time, the photons will pick …

We derive updated constraints on the integrated Sachs-Wolfe (ISW) effect through cross-
correlation of the cosmic microwave background with galaxy surveys. We improve with …

Future large-scale structure surveys will measure the locations and shapes of billions of
galaxies. The precision of such catalogues will require meticulous treatment of systematic …

The integrated Sachs-Wolfe (ISW) effect measures the decay of the gravitational potential
due to cosmic acceleration and is thus a direct probe of dark energy. In some of the earlier …