Distance of Hi-GAL sources

Aims. Distances are key to determining the physical properties of sources. In Galaxy, large (> 10 000) homogeneous samples sources for which distance available, covering whole Galactic range, still missing. Here we present a catalog velocity and sample 100 Hi-GAL compact Methods. We developed fully automatic Python package extract determine distance. To assign source, code uses all available spectroscopic data complemented by morphological analysis. Once is determined, if no stellar or maser parallax known, kinematic calculated ambiguity (for located inside Solar circle) solved with H I self-absorption method from distance–extinction data. Results. Among 150 223 catalog, obtained 124 069 5 σ (and 128 351 3 catalog), where represents noise level each molecular spectrum used line detections made at produce respective catalogs.