Astrophysics with the laser interferometer space antenna
Abstract The Laser Interferometer Space Antenna (LISA) will be a transformative experiment
for gravitational wave astronomy, and, as such, it will offer unique opportunities to address …
for gravitational wave astronomy, and, as such, it will offer unique opportunities to address …
Large-scale dark matter simulations
We review the field of collisionless numerical simulations for the large-scale structure of the
Universe. We start by providing the main set of equations solved by these simulations and …
Universe. We start by providing the main set of equations solved by these simulations and …
The camels project: Cosmology and astrophysics with machine-learning simulations
The CAMELS Project: Cosmology and Astrophysics with Machine-learning Simulations -
IOPscience This site uses cookies. By continuing to use this site you agree to our use of cookies …
IOPscience This site uses cookies. By continuing to use this site you agree to our use of cookies …
Cosmographic view on the and tensions
Measurements of the H 0 and σ 8 parameters within the standard cosmological model
recently highlighted significant statistical tensions between the cosmic microwave …
recently highlighted significant statistical tensions between the cosmic microwave …
Dark Energy Survey Year 3 results: Curved-sky weak lensing mass map reconstruction
We present reconstructed convergence maps, mass maps, from the Dark Energy Survey
(DES) third year (Y3) weak gravitational lensing data set. The mass maps are weighted …
(DES) third year (Y3) weak gravitational lensing data set. The mass maps are weighted …
Likelihood-free inference with neural compression of DES SV weak lensing map statistics
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 …
data as a function of the unknown parameters) is unknown or intractable. This necessitates …
Dark energy survey year 3 results: Cosmology with peaks using an emulator approach
We constrain the matter density Ωm and the amplitude of density fluctuations σ8 within the
ΛCDM cosmological model with shear peak statistics and angular convergence power …
ΛCDM cosmological model with shear peak statistics and angular convergence power …
Constraining dark matter-dark radiation interactions with CMB, BAO, and Lyman-α
Abstract Several interesting Dark Matter (DM) models invoke a dark sector leading to two
types of relic particles, possibly interacting with each other: non-relativistic DM, and …
types of relic particles, possibly interacting with each other: non-relativistic DM, and …
Learning cosmology and clustering with cosmic graphs
P Villanueva-Domingo… - The Astrophysical …, 2022 - iopscience.iop.org
We train deep-learning models on thousands of galaxy catalogs from the state-of-the-art
hydrodynamic simulations of the Cosmology and Astrophysics with MachinE Learning …
hydrodynamic simulations of the Cosmology and Astrophysics with MachinE Learning …
Cosmic shear cosmology beyond two-point statistics: a combined peak count and correlation function analysis of DES-Y1
J Harnois-Déraps, N Martinet, T Castro… - Monthly Notices of …, 2021 - academic.oup.com
We constrain cosmological parameters from a joint cosmic shear analysis of peak-counts
and the two-point shear correlation functions, as measured from the Dark Energy Survey …
and the two-point shear correlation functions, as measured from the Dark Energy Survey …