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20192026
most citedThe Quijote simulations

340 citations · 709 across the 22 of their papers we have counts for

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Showing 2026Show all

6 papers · 1 filter

astro-ph.CO2026

Validation of harmonic-space likelihood methods for LiteBIRD B-mode polarisation analysis

G. Galloni, P. Campeti, C. Gimeno-Amo +112

The LiteBIRD satellite mission aims to measure the tensor-to-scalar ratio with unprecedented sensitivity through observations of the cosmic microwave background (CMB) -mode…

astro-ph.CO2026

-sure. Part II. Scattering transforms as robustness test for tensor-to-scalar ratio detection from CMB observations

Claudio Ranucci, Sébastien Pierre, Léo Vacher +7

Galactic foregrounds represent a major contamination to the measurement of primordial -modes from observations of the Cosmic Microwave Background polarisation. Even after the ap…

astro-ph.GA2026

Revealing Galactic dust beneath the cosmic infrared background anisotropies with Wavelet Phase Harmonics

Srijita Sinha, Tuhin Ghosh, Erwan Allys +2

Separating Galactic dust emission from cosmic infrared background (CIB) anisotropies is challenging because both the emission components have similar spectral properties. The prima…

astro-ph.GA2026

Untangling dust emission and cosmic infrared background anisotropies with the scattering transform statistics

Srijita Sinha, Tuhin Ghosh, Erwan Allys +2

The template-fit approach is often used to separate Galactic dust emission from cosmic infrared background (CIB) anisotropies in low column density regions, under the a…

astro-ph.IM2026★ 1 cited

Bayesian imaging inverse problem with scattering transform

Sébastien Pierre, Erwan Allys, Pablo Richard +2

Bayesian imaging inverse problems in astrophysics and cosmology remain challenging, particularly in low-data regimes, due to complex forward operators and the frequent lack of well…

astro-ph.CO2026

Separation of polarized dust emission in Planck observations with Scattering Transforms

Alexandros Tsouros, Elisa Russier, Erwan Allys +3

Polarized dust emission is a major astrophysical foreground contaminant of the cosmic microwave background polarization (CMB), which must be accurately measured to look for the fai…