activity
20072026
most citedA Joint Analysis of BICEP2/Keck Array and Planck Data

985 citations · 8.5k across the 132 of their papers we have counts for

collaborators

133 papers

astro-ph.CO2026

Statistical imprints of wave-like dark matter on multiply-imaged galaxies in strong cluster lenses from JWST

Nino Ephremidze, Daniel Gilman, Cora Dvorkin

Wave-like dark matter (DM) is an elusive dark matter (DM) candidate. The model, often also called fuzzy or ultralight DM, proposes that DM is an extremely light (…

astro-ph.CO2026

Robustness of Neural Networks for CMB Polarization Foreground Removal

Luca Gomez Bachar, Cora Dvorkin, Alberto Daniel Supanitsky

The detection of Cosmic Microwave Background primordial -mode polarization would constitute a ``smoking gun" signal of primordial gravitational waves. However, this measurement…

astro-ph.CO2026

Fast Fourier Transform evaluation of the Fresnel integral for gravitational-wave lensing

Nino Ephremidze, Marc Kamionkowski, Cora Dvorkin

Gravitational waves (GWs) exhibit wave-optics effects when their wavelength is comparable to the scale of the gravitational lens. This may occur in lensing from galactic subhalos i…

astro-ph.CO2025★ 1 cited

Constraining Power of Wavelet vs. Power Spectrum Statistics for CMB Lensing and Weak Lensing with Learned Binning

Kyle Boone, Georgios Valogiannis, Marco Gatti +1

We present forecasts for constraints on the matter density () and the amplitude of matter density fluctuations at 8hMpc () from CMB lensing convergence maps and ga…

cs.AI2025★ 1 cited

The Future of Artificial Intelligence and the Mathematical and Physical Sciences (AI+MPS)

Andrew Ferguson, Marisa LaFleur, Lars Ruthotto +97

This community paper developed out of the NSF Workshop on the Future of Artificial Intelligence (AI) and the Mathematical and Physics Sciences (MPS), which was held in March 2025 w…

astro-ph.CO2025★ 4 cited

Field-level Reconstruction from Foreground-Contaminated 21-cm Maps

Shu-Fan Chen, Kai-Feng Chen, Cora Dvorkin

Current and upcoming 21-cm experiments will soon be able to map 21-cm spatial fluctuations in three dimensions for a wide range of redshifts. However, bright foreground contaminati…