The Astrophysical Journal (Jan 2023)

Overview of the DESI Milky Way Survey

  • Andrew P. Cooper,
  • Sergey E. Koposov,
  • Carlos Allende Prieto,
  • Christopher J. Manser,
  • Namitha Kizhuprakkat,
  • Adam D. Myers,
  • Arjun Dey,
  • Boris T. Gänsicke,
  • Ting S. Li,
  • Constance Rockosi,
  • Monica Valluri,
  • Joan Najita,
  • Alis Deason,
  • Anand Raichoor,
  • M.-Y. Wang,
  • Y.-S. Ting,
  • Bokyoung Kim,
  • Andreia Carrillo,
  • Wenting Wang,
  • Leandro Beraldo e Silva,
  • Jiwon Jesse Han,
  • Jiani Ding,
  • Miguel Sánchez-Conde,
  • Jessica N. Aguilar,
  • Steven Ahlen,
  • Stephen Bailey,
  • Vasily Belokurov,
  • David Brooks,
  • Katia Cunha,
  • Kyle Dawson,
  • Axel de la Macorra,
  • Peter Doel,
  • Daniel J. Eisenstein,
  • Parker Fagrelius,
  • Kevin Fanning,
  • Andreu Font-Ribera,
  • Jaime E. Forero-Romero,
  • Enrique Gaztañaga,
  • Satya Gontcho A Gontcho,
  • Julien Guy,
  • Klaus Honscheid,
  • Robert Kehoe,
  • Theodore Kisner,
  • Anthony Kremin,
  • Martin Landriau,
  • Michael E. Levi,
  • Paul Martini,
  • Aaron M. Meisner,
  • Ramon Miquel,
  • John Moustakas,
  • Jundan J. D. Nie,
  • Nathalie Palanque-Delabrouille,
  • Will J. Percival,
  • Claire Poppett,
  • Francisco Prada,
  • Nabeel Rehemtulla,
  • Edward Schlafly,
  • David Schlegel,
  • Michael Schubnell,
  • Ray M. Sharples,
  • Gregory Tarlé,
  • Risa H. Wechsler,
  • David H. Weinberg,
  • Zhimin Zhou,
  • Hu Zou

DOI
https://doi.org/10.3847/1538-4357/acb3c0
Journal volume & issue
Vol. 947, no. 1
p. 37

Abstract

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We describe the Milky Way Survey (MWS) that will be undertaken with the Dark Energy Spectroscopic Instrument (DESI) on the Mayall 4 m telescope at the Kitt Peak National Observatory. Over the next 5 yr DESI MWS will observe approximately seven million stars at Galactic latitudes ∣ b ∣ > 20°, with an inclusive target selection scheme focused on the thick disk and stellar halo. MWS will also include several high-completeness samples of rare stellar types, including white dwarfs, low-mass stars within 100 pc of the Sun, and horizontal branch stars. We summarize the potential of DESI to advance understanding of the Galactic structure and stellar evolution. We introduce the final definitions of the main MWS target classes and estimate the number of stars in each class that will be observed. We describe our pipelines for deriving radial velocities, atmospheric parameters, and chemical abundances. We use ≃500,000 spectra of unique stellar targets from the DESI Survey Validation program (SV) to demonstrate that our pipelines can measure radial velocities to ≃1 km s ^−1 and [Fe/H] accurate to ≃0.2 dex for typical stars in our main sample. We find the stellar parameter distributions from ≈100 deg ^2 of SV observations with ≳90% completeness on our main sample are in good agreement with expectations from mock catalogs and previous surveys.

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