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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.GA2024
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…
astro-ph.GA2023
Bayesian inference of 3D densities of galactic HI and H2
Laurin Söding, Philipp Mertsch, Vo Hong Minh Phan
Due to our vantage point in the disk of the Galaxy, its 3D structure is not directly accessible. However, knowing the spatial distribution, e.g. of atomic and molecular hydrogen ga…