collaborators

13 papers

math.NA2026

Variational Inference Using a Differentiable Multigrid Linear Solver

Andrés Ramírez, Philipp Haim, David Föger +9

Gradient-based Bayesian inference methods require efficient access to Jacobian and adjoint-Jacobian operators of high-dimensional forward models. While multigrid solvers provide ne…

astro-ph.GA2026

Milky Way Atlas: A radial-velocity-resolved, three-dimensional map of H I within 1.25 kpc

Lewis McCallum, Laurin Söding, Mareike Berkner +9

We present a velocity-resolved three-dimensional map of local atomic hydrogen (HI) within 1.25 kpc of the Sun, tackling the challenge of converting emission from position-position-…

astro-ph.HE2026

Stochastic modelling of cosmic-ray sources for Galactic diffuse emissions

Anton Stall, Philipp Mertsch

Galactic diffuse emissions in gamma rays and neutrinos arise from interactions of cosmic rays with the interstellar medium and probe the cosmic-ray intensity away from the Solar sy…

astro-ph.HE2025

Spectrum and anisotropies of Galactic cosmic rays: a laboratory for magnetic fields

Philipp Mertsch

Much has been learned about Galactic cosmic rays in the past decade: On the observational side, the spectra of cosmic ray nuclei have been directly measured with high precision, re…

astro-ph.GA2025

Local dark matter density from Gaia DR3 K-dwarfs using Gaussian processes

Laurin Söding, Ruben L. Bartel, Philipp Mertsch

The local dark matter density provides constraints on dark matter models and is of importance for experiments hoping to detect dark matter particles in the laboratory. The advent o…

astro-ph.GA2025

Spatially Coherent 3D Distributions of HI and CO in the Milky Way

Laurin Söding, Gordian Edenhofer, Torsten A. Enßlin +6

The spatial distribution of the gaseous components of the Milky Way is of great importance for a number of different fields, for example, Galactic structure, star formation, and co…