Abstract
The DESI Milky Way Survey (MWS) will observe ≥8 million stars between 16 <r <19 mag, supplemented by observations of brighter targets under poor observing conditions. The survey will permit an accurate determination of stellar kinematics and population gradients; characterize diffuse substructure in the thick disk and stellar halo; enable the discovery of extremely metal-poor stars and other rare stellar types; and improve constraints on the Galaxy's 3D dark matter distribution from halo star kinematics. MWS will also enable a detailed characterization of the stellar populations within 100 pc of the Sun, including a complete census of white dwarfs. The target catalog from the preliminary selection described here is public.
| Original language | English |
|---|---|
| Journal | Research Notes of the American Astronomical Society |
| Volume | 4 |
| Issue number | 10 |
| DOIs | |
| Publication status | Published - 23 Oct 2020 |
Keywords / Materials (for Non-textual outputs)
- astro-ph.GA
- astro-ph.SR
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