Carlos Allende Prieto
GTC Follow-up Observations of Very Metal-poor Star Candidates from DESI
Allende Prieto, Carlos; Aguado, David S.; González Hernández, Jonay I.; Rebolo, Rafael; Najita, Joan; Manser, Christopher J.; Rockosi, Constance; Slepian, Zachary; Mezcua, Mar; Valluri, Monica; Ezzeddine, Rana; Koposov, Sergey E.; Cooper, Andrew P.; Dey, Arjun; Gänsicke, Boris T.; Li, Ting S.; Cunha, Katia; Zou, Siwei; Aguilar, Jessica Nicole; Ahlen, Steven; Brooks, David; Claybaugh, Todd; Cole, Shaun; Eftekharzadeh, Sarah; Fanning, Kevin; Forero-Romero, Jaime; Gontcho, Satya Gontcho A; Honscheid, Klaus; Jablonka, Pascale; Kehoe, Robert; Kisner, Theodore; Landriau, Martin; de la Macorra, Axel; Meisner, Aaron; Miquel, Ramón; Moustakas, John; Nie, Jundan; Poppett, Claire; Prada, Francisco; Rezaie, Mehdi; Rossi, Graziano; Sánchez, Eusebio; Schubnell, Michael; Sharples, Ray; Siudek, Malgorzata; Smith, Verne V.; Tarlé, Gregory; Vincenzo, Fiorenzo; Weaver, Benjamin Alan; Zhou, Zhimin; Zou, Hu
Authors
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
Professor Shaun Cole shaun.cole@durham.ac.uk
Director of the Institute for Computational Cosmology
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
Professor Ray Sharples r.m.sharples@durham.ac.uk
Professor
Malgorzata Siudek
Verne V. Smith
Gregory Tarlé
Fiorenzo Vincenzo
Benjamin Alan Weaver
Zhimin Zhou
Hu Zou
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 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.
Citation
Allende Prieto, C., Aguado, D. S., González Hernández, J. I., Rebolo, R., Najita, J., Manser, C. J., …Zou, H. (2023). GTC Follow-up Observations of Very Metal-poor Star Candidates from DESI. Astrophysical Journal, 957(2), Article 76. https://doi.org/10.3847/1538-4357/acfa96
Journal Article Type | Article |
---|---|
Acceptance Date | Aug 7, 2023 |
Online Publication Date | Nov 1, 2023 |
Publication Date | Nov 10, 2023 |
Deposit Date | Nov 15, 2023 |
Publicly Available Date | Nov 15, 2023 |
Journal | The Astrophysical Journal |
Print ISSN | 0004-637X |
Publisher | American Astronomical Society |
Peer Reviewed | Peer Reviewed |
Volume | 957 |
Issue | 2 |
Article Number | 76 |
DOI | https://doi.org/10.3847/1538-4357/acfa96 |
Keywords | Spectroscopy, Milky Way formation, Field stars |
Public URL | https://durham-repository.worktribe.com/output/1883948 |
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Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.
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