activity
20122024
most citedCMB-S4 Science Book, First Edition

352 citations · 382 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.CO2024

Non-Gaussian deflections in iterative optimal CMB lensing reconstruction

Omar Darwish, Sebastian Belkner, Louis Legrand +2

The gravitational lensing signal from the Cosmic Microwave Background is highly valuable to constrain the growth of the structures in the Universe in a clean and robust manner over…

astro-ph.CO20241 cited

GANSky -- fast curved sky weak lensing simulations using Generative Adversarial Networks

Supranta S. Boruah, Pier Fiedorowicz, Rafael Garcia +3

Extracting non-Gaussian information from the next generation weak lensing surveys will require fast and accurate full-sky simulations. This is difficult to achieve in practice with…

astro-ph.CO2024

Growth history and quasar bias evolution at z < 3 from Quaia

G. Piccirilli, G. Fabbian, D. Alonso +4

We make use of the Gaia-Unwise quasar catalogue, Quaia, to constrain the growth history out to high redshifts from the clustering of quasars and their cross-correlation with maps o…

astro-ph.CO2024

Planck constraints on Cosmic Birefringence and its cross-correlation with the CMB

G. Zagatti, M. Bortolami, A. Gruppuso +3

Cosmic birefringence is the in-vacuo, frequency independent rotation of the polarization plane of linearly polarized radiation, induced by a parity-violating term in the electromag…

astro-ph.GA20236 cited

A Hierarchy of Normalizing Flows for Modelling the Galaxy-Halo Relationship

Christopher C. Lovell, Sultan Hassan, Daniel Anglés-Alcázar +8

Using a large sample of galaxies taken from the Cosmology and Astrophysics with MachinE Learning Simulations (CAMELS) project, a suite of hydrodynamic simulations varying both cosm…

astro-ph.CO2023

CMB-S4: Forecasting Constraints on Through -distortion Anisotropy

David Zegeye, Federico Bianchini, J. Richard Bond +14

Diffusion damping of the cosmic microwave background (CMB) power spectrum results from imperfect photon-baryon coupling in the pre-recombination plasma. At redshift $5 \times 10^4…