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View article: Local dark matter density from <i>Gaia</i> DR3 K-dwarfs using Gaussian processes
Local dark matter density from <i>Gaia</i> DR3 K-dwarfs using Gaussian processes Open
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 of extensive survey data calls for more complex physical mod…
View article: Spatially coherent 3D distributions of HI and CO in the Milky Way
Spatially coherent 3D distributions of HI and CO in the Milky Way Open
Context. 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 cosmic rays. However, obtaining distance information…
View article: Spatially Coherent 3D Distributions of HI and CO in the Milky Way
Spatially Coherent 3D Distributions of HI and CO in the Milky Way Open
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 cosmic rays. However, obtaining distance information to gaseo…
View article: The influence of the 3D Galactic gas structure on cosmic-ray transport and $γ$-ray emission
The influence of the 3D Galactic gas structure on cosmic-ray transport and $γ$-ray emission Open
Cosmic rays (CRs) play a major role in the dynamics of the interstellar medium (ISM). Their interactions and transport ionize, heat, and push the ISM thereby coupling different regions of it. The spatial distribution of CRs depends on the …
View article: Bayesian inference of 3D densities of galactic HI and H2
Bayesian inference of 3D densities of galactic HI and H2 Open
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 gas is of great importance for interpreting and modelling cos…
View article: Bayesian inference of 3D densities of galactic HI and H2
Bayesian inference of 3D densities of galactic HI and H2 Open
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 gas is of great importance for interpreting and modelling cos…
View article: Evolving ultralight scalars into non-linearity with Lagrangian perturbation theory
Evolving ultralight scalars into non-linearity with Lagrangian perturbation theory Open
Many models of high energy physics suggest that the cosmological dark sector consists of not just one, but a spectrum of ultralight scalar particles with logarithmically distributed masses. To study the potential signatures of low concentr…