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Preliminary Target Selection for the DESI Milky Way Survey (MWS)

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. Green open access

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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
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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