Prieto, CA;
Cooper, AP;
Dey, A;
Gänsicke, BT;
Koposov, SE;
Li, T;
Manser, C;
... Yèche, C; + view all
(2020)
Preliminary Target Selection for the DESI Milky Way Survey (MWS).
Research Notes of the AAS
, 4
, Article 188. 10.3847/2515-5172/abc1dc.
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Abstract
The DESI Milky Way Survey (MWS) will observe $\ge$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.
Type: | Article |
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Title: | Preliminary Target Selection for the DESI Milky Way Survey (MWS) |
Open access status: | An open access version is available from UCL Discovery |
DOI: | 10.3847/2515-5172/abc1dc |
Publisher version: | http://dx.doi.org/10.3847/2515-5172/abc1dc |
Language: | English |
Additional information: | This version is the author accepted manuscript. For information on re-use, please refer to the publisher’s terms and conditions. |
Keywords: | Astro-ph.GA, astro-ph.GA, astro-ph.SR |
UCL classification: | UCL UCL > Provost and Vice Provost Offices > UCL BEAMS UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Physics and Astronomy |
URI: | https://discovery-pp.ucl.ac.uk/id/eprint/10142292 |
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