Far-infrared and submillimeter wavelength surveys have now established the important role
of dusty, star-forming galaxies (DSFGs) in the assembly of stellar mass and the evolution of …

Likelihood-free inference provides a framework for performing rigorous Bayesian inference
using only forward simulations, properly accounting for all physical and observational effects …

Roughly half of the radiation from evolving galaxies in the early Universe reaches us in the
far-infrared and submillimeter wavelength ranges. Recent major advances in observing …

In many cosmological inference problems, the likelihood (the probability of the observed
data as a function of the unknown parameters) is unknown or intractable. This necessitates …

We present new measurements of cosmic infrared background (CIB) anisotropies using
Planck. Combining HFI data with IRAS, the angular auto-and cross-frequency power …

Abstract PRISM (Polarized Radiation Imaging and Spectroscopy Mission) was proposed to
ESA in May 2013 as a large-class mission for investigating within the framework of the ESA …

Panchromatic observations of the best candidate hyperluminous infrared galaxies from the
widest Herschel extragalactic imaging survey have led to the discovery of at least four …

We show how nuisance parameter marginalized posteriors can be inferred directly from
simulations in a likelihood-free setting, without having to jointly infer the higher dimensional …

We apply two Bayesian hierarchical inference schemes to infer shear power spectra, shear
maps and cosmological parameters from the Canada–France–Hawaii Telescope …

Density-estimation likelihood-free inference (DELFI) has recently been proposed as an
efficient method for simulation-based cosmological parameter inference. Compared to the …