collaborators

5 papers

stat.CO2026

GraphGP: Scalable Gaussian Processes with Vecchia's Approximation

Benjamin Dodge, Philipp Frank, Susan E. Clark

Gaussian processes are a powerful tool for modeling continuous fields, but their naive computational cost and memory requirement often limit t…

astro-ph.GA2026

Imprints of the Neutral Interstellar Medium on Polarized Synchrotron Emission and Faraday Rotation

Minjie Lei, S. E. Clark, Mehrnoosh Tahani +5

The interstellar medium (ISM) is a complex, multiphase medium, where disentangling the distribution of gas and magnetic field structure across different phases remains a considerab…

astro-ph.GA2026

Phase-dependent magnetic coherence in the turbulent interstellar medium

Iryna S. Butsky, Caleb Redshaw, Minjie Lei +2

Magnetic fields permeate the multiphase interstellar medium (ISM), yet their phase-dependent structure remains poorly constrained by observations. Dust polarization and \ion{H}{1}…

astro-ph.GA2026

The radial component of the local Galactic magnetic field in 3D

Lewis McCallum, Philipp Frank, Sebastian Hutschenreuter +9

We present a distance-resolved reconstruction of the local line-of-sight Galactic magnetic field, , by combining a 3D electron density () map derived from dust map-i…

astro-ph.GA2025

A three-dimensional model for the reversal in the local large-scale interstellar magnetic field

Rebecca A. Booth, Anna Ordog, Jo-Anne Brown +8

We probe the three-dimensional geometry of the large-scale Galactic magnetic field within 1 kpc of the Sun using the Dominion Radio Astrophysical Observatory (DRAO) Global Magneto-…