The Astrophysical Journal (Jan 2023)

GTC Follow-up Observations of Very Metal-poor Star Candidates from DESI

  • Carlos Allende Prieto,
  • David S. Aguado,
  • Jonay I. González Hernández,
  • Rafael Rebolo,
  • Joan Najita,
  • Christopher J. Manser,
  • Constance Rockosi,
  • Zachary Slepian,
  • Mar Mezcua,
  • Monica Valluri,
  • Rana Ezzeddine,
  • Sergey E. Koposov,
  • Andrew P. Cooper,
  • Arjun Dey,
  • Boris T. Gänsicke,
  • Ting S. Li,
  • Katia Cunha,
  • Siwei Zou,
  • Jessica Nicole Aguilar,
  • Steven Ahlen,
  • David Brooks,
  • Todd Claybaugh,
  • Shaun Cole,
  • Sarah Eftekharzadeh,
  • Kevin Fanning,
  • Jaime Forero-Romero,
  • Satya Gontcho A Gontcho,
  • Klaus Honscheid,
  • Pascale Jablonka,
  • Robert Kehoe,
  • Theodore Kisner,
  • Martin Landriau,
  • Axel de la Macorra,
  • Aaron Meisner,
  • Ramón Miquel,
  • John Moustakas,
  • Jundan Nie,
  • Claire Poppett,
  • Francisco Prada,
  • Mehdi Rezaie,
  • Graziano Rossi,
  • Eusebio Sánchez,
  • Michael Schubnell,
  • Ray Sharples,
  • Malgorzata Siudek,
  • Verne V. Smith,
  • Gregory Tarlé,
  • Fiorenzo Vincenzo,
  • Benjamin Alan Weaver,
  • Zhimin Zhou,
  • Hu Zou

DOI
https://doi.org/10.3847/1538-4357/acfa96
Journal volume & issue
Vol. 957, no. 2
p. 76

Abstract

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The observations from the Dark Energy Spectroscopic Instrument (DESI) will significantly increase the numbers of known extremely metal-poor stars by a factor of ∼10, improving the sample statistics to study the early chemical evolution of the Milky Way and the nature of the first stars. In this paper we report follow-up observations with high signal-to-noise ratio of nine metal-poor stars identified during the DESI commissioning with the Optical System for Imaging and Low-Resolution Integrated Spectroscopy (OSIRIS) instrument on the 10.4 m Gran Telescopio Canarias. The analysis of the data using a well-vetted methodology confirms the quality of the DESI spectra and the performance of the pipelines developed for the data reduction and analysis of DESI data.

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