activity
20242026
collaborators

12 papers

astro-ph.CO2026

A new measurement of the FRB DM-galaxy cross correlation and a first joint analysis with the kinematic SZ effect

Samuel McCarty, Liam Connor, Kritti Sharma +8

Understanding the distribution of cosmic baryons is crucial for advancing cosmology and galaxy formation. Localized Fast Radio Bursts (FRBs) are a promising new probe of the diffus…

astro-ph.CO2026

Direct shear kSZ correlation: controlling baryons without modeling galaxies

Anoma Ganguly, Emmanuel Schaan, Elisabeth Krause +1

Baryonic feedback redistributes gas within and around dark matter haloes, suppressing the small-scale matter power spectrum at a level that is now the leading systematic for upcomi…

astro-ph.CO2026

Cosmic shear with one component and its application to future radio surveys

Yu-Hsiu Huang, Elisabeth Krause, Tim Eifler +4

We present a new approach to measuring cosmic shear: the one-component kinematic lensing (KL) method. This technique provides a simplified implementation of KL that reduces shape n…

astro-ph.CO2026

Baryons in the Darkest Sites of the Universe

Kritti Sharma, Vikram Ravi, Dhayaa Anbajagane +9

The pristine underdense patches of the Universe, cosmic voids, are powerful cosmological laboratories, uniquely sensitive to dark energy, modified gravity, and neutrino masses, yet…

astro-ph.CO2026

Backlighting the Cosmic Web with Fast Radio Bursts: An Anthology of Dispersion Measure Cross-Correlations with Large-Scale Structure and Baryon Tracers

Kritti Sharma, Elisabeth Krause, Vikram Ravi +11

Fast Radio Bursts (FRBs) probe baryons permeating the cosmic web through their dispersion measures (DMs), which encode the integrated electron density along cosmological sightlines…

astro-ph.CO2026

Informative Priors on Primordial Non-Gaussianity Bias From Galaxy Formation

Anne Moore, Lucia A. Perez, Elisabeth Krause

Constraining primordial non-Gaussianity via its scale-dependent imprint on galaxy clustering requires knowledge of the bias parameter , which is exactly degenerate with $f^{\…