The co-evolution between supermassive black holes and their environment is most directly
traced by the hot atmospheres of dark matter halos. The cooling of the hot atmosphere …

Within the Lambda cold dark matter (ΛCDM) model, measurements from recent cosmic
microwave background (CMB) and weak lensing (WL) surveys have uncovered a∼ 3σ …

Transition Edge Sensors (TESs) are amongst the most sensitive cryogenic detectors and
can be easily optimized for the detection of massive particles or photons ranging from X-rays …

In this work we present PRyMordial: A package dedicated to efficient computations of
observables in the Early Universe with the focus on the cosmological era of Big Bang …

We present new constraints on anisotropic birefringence of the cosmic microwave
background polarization using two seasons of data from the Atacama Cosmology Telescope …

We introduce and validate a delensing framework for the Simons Observatory (SO), which
will be used to improve constraints on inflationary gravitational waves by reducing the …

We present the Aemulus ν simulations: a suite of 150 (1.05 h-1 Gpc) 3 N-body simulations
with a mass resolution of 3.51× 10 10 Ω cb/0.3 h-1 M⊙ in a wνCDM cosmological parameter …

If the physics behind dark energy and/or dark matter violates the parity symmetry assumed in
the standard cosmological paradigm, the linear polarization of the cosmic microwave …

Pulsar-timing arrays (PTAs) are in the near future expected to detect a stochastic
gravitational-wave background (SGWB) produced by a population of inspiralling …

Axion-like particles (ALPs) are a well-motivated dark matter candidate that solves some of
the problems in the clustering of large scale structure in cosmology. ALPs are often …