activity
20232026
most citedCMB-S4: Iterative Internal Delensing and Constraints

40 citations · 41 across the 14 of their papers we have counts for

collaborators

15 papers

astro-ph.IM2026

Optimization of multi-resolution observation strategies for cosmic microwave background experiments

Sara M. Simon, Jacques Delabrouille, Julien Carron +4

Cosmic microwave background (CMB) observations are increasingly performed by using a combination of both small aperture telescopes (SATs) and large aperture telescopes (LATs) to ex…

astro-ph.CO2026

Cross-correlation of SPT-3G D1 CMB lensing and DES Y3 galaxy lensing

A. Ouellette, Y. Omori, E. Anderes +92

Measurements of the weak lensing of galaxies and of the cosmic microwave background (CMB) provide direct probes of the cosmic matter density field, but the two observables are sens…

astro-ph.CO2026

SPT-3G D1: Maps of the millimeter-wave sky from 2019 and 2020 observations of the SPT-3G Main field

W. Quan, E. Camphuis, C. Daley +92

Maps of the sky in millimeter wavelengths contain rich information on cosmology through anisotropies of the cosmic microwave background (CMB). Creating multifrequency sky maps of a…

astro-ph.CO2026

Fast partial-sky spherical harmonic transforms

Julien Carron, Martin Reinecke

We discuss in some details a novel algorithm for performing partial-sky spherical harmonic transforms (SHT), building on the Fourier-sphere method of Reinecke et al (2023) handling…

astro-ph.CO2025

An iterative CMB lensing estimator minimizing instrumental noise bias

Louis Legrand, Blake Sherwin, Anthony Challinor +2

Noise maps from CMB experiments are generally statistically anisotropic, due to scanning strategies, atmospheric conditions, or instrumental effects. Any mis-modeling of this compl…

astro-ph.CO2025★ 1 cited

Characterizing CMB noise anisotropies from CMB delensing

Louis Legrand, Julien Carron

Un-doing the effect of gravitational lensing on the Cosmic Microwave Background (`de-lensing') is essential in shaping constraints on weak signals limited by lensing effects on the…

astro-ph.CO2025

On likelihood-based analysis of the gravitationally (de)lensed CMB

Julien Carron

By reducing variance induced by gravitational lensing, likelihood-based de-lensing techniques have true potential to extract significantly more information from deep and high-resol…

astro-ph.CO2025

CMB-S4: Foreground-Cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves

Federico Bianchini, Dominic Beck, W. L. Kimmy Wu +6

We compare multiple foreground-cleaning pipelines for estimating the tensor-to-scalar ratio, , using simulated maps of the planned CMB-S4 experiment within the context of the So…

astro-ph.CO2025

Detecting rotation from lensing in the CMB

Julien Carron, Enea di Dio, Ruth Durrer

An excellent estimate of the lensing signal is expected from the availability of deep and high-resolution polarization data in the near future. This is most important to allow for…

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.IM2024

: GPU Accelerated Spherical Harmonic Transforms on Arbitrary Pixelizations

Sebastian Belkner, Adriaan J. Duivenvoorden, Julien Carron +2

We present , a general-purpose Python package that wraps a highly efficient CUDA implementation of the nonuniform spin- spherical harmonic transform. The metho…

astro-ph.CO2024

Detectable signals of post-Born lensing curl B-modes

Mathew Robertson, Giulio Fabbian, Julien Carron +1

Curl lensing, also known as lensing field-rotation or shear B-modes, is a distinct post-Born observable caused by two lensing deflections at different redshifts (lens-lens coupling…

astro-ph.CO2024

Spherical bispectrum expansion and quadratic estimators

Julien Carron, Antony Lewis

We describe a general expansion of spherical (full-sky) bispectra into a set of orthogonal modes. For squeezed shapes, the basis separates physically-distinct signals and is domina…

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.CO2023★ 40 cited

CMB-S4: Iterative Internal Delensing and Constraints

Sebastian Belkner, Julien Carron, Louis Legrand +3

The tightest constraints on the tensor-to-scalar ratio can only be obtained after removing a substantial fraction of the lensing -mode sample variance. The planned CMB-S4 ex…