학술논문

GTC Follow-up Observations of Very Metal-Poor Star Candidates from DESI
Document Type
Working Paper
Source
Subject
Astrophysics - Solar and Stellar Astrophysics
Astrophysics - Astrophysics of Galaxies
Astrophysics - Instrumentation and Methods for Astrophysics
Language
Abstract
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 high signal-to-noise follow-up observations of 9 metal-poor stars identified during the DESI commissioning with the Optical System for Imaging and low-Intermediate-Resolution Integrated Spectroscopy (OSIRIS) instrument on the 10.4m Gran Telescopio Canarias (GTC). 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.
Comment: 14 pages, 4 figures, accepted for publication in ApJ, data available from https://doi.org/10.5281/zenodo.8363303