We present a new three-dimensional map of dust reddening, based on Gaia parallaxes and
stellar photometry from Pan-STARRS 1 and 2MASS. This map covers the sky north of a decl …

Gaia stellar measurements are currently revolutionizing our knowledge of the evolutionary
history of the Milky Way. 3D maps of the interstellar dust provide complementary information …

We present a new 3D map of interstellar dust reddening, covering three quarters of the sky
(declinations of δ≳− 30°) out to a distance of several kiloparsecs. The map is based on high …

Abstract The Galactic Archaeology with HERMES (GALAH) survey is a large high-resolution
spectroscopic survey using the newly commissioned High Efficiency and Resolution Multi …

Context. Three-dimensional (3D) maps of the extinction density in the Milky Way can be built
through the inversion of large catalogues of distance-extinction pairs for individual target …

We present a three-dimensional map of interstellar dust reddening, covering three-quarters
of the sky out to a distance of several kiloparsecs, based on Pan-STARRS 1 (PS1) and …

Context. Gaia data and stellar surveys open the way to the construction of detailed 3D maps
of the Galactic interstellar (IS) dust based on the synthesis of star distances and extinctions …

Inferences about the spatial density or phase-space structure of stellar populations in the
Milky Way require a precise determination of the effective survey volume. The volume …

The spatial structure of stellar populations with different chemical abundances in the Milky
Way (MW) contains a wealth of information on Galactic evolution over cosmic time. We use …

We leverage the 1 pc spatial resolution of the Leike et al. three-dimensional (3D) dust map
to characterize the 3D structure of nearby molecular clouds (d≲ 400 pc). We start by" …