A Large Sample of Extremely Metal-poor Galaxies at z < 1 Identified from the DESI Early Data
Journal Article
·
· The Astrophysical Journal
more »
- Chinese Academy of Sciences, Beijing (China); University of Chinese Academy of Sciences, Beijing (China); University of Michigan, Ann Arbor MI
- Chinese Academy of Sciences, Beijing (China); University of Chinese Academy of Sciences, Beijing (China)
- University College London (United Kingdom)
- Siena College, Loudonville, NY (United States)
- Institute of Space Sciences, ICE-CSIC, Barcelona (Spain)
- NSF's NOIRLab, Tucson, AZ (United States)
- Chinese Academy of Sciences, Beijing (China)
- University of Portsmouth (United Kingdom)
- Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States)
- Boston University, MA (United States)
- University of Utah, Salt Lake City, UT (United States)
- Universidad Nacional Autónoma de México (Mexico)
- Universidad de los Andes, Bogotá (Colombia)
- The Ohio State University, Columbus, OH (United States)
- Sorbonne Université, Paris (France)
- The Barcelona Institute of Science and Technology (Spain)
- University of California, Berkeley, CA (United States)
- Kansas State University, Manhattan, KS (United States)
- Sejong University, Seoul (Korea, Republic of)
- Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas (CIEMAT), Madrid (Spain)
- Ohio University, Athens, OH (United States)
- University of Michigan, Ann Arbor, MI (United States)
- Tsinghua University, Beijing (China)
Extremely metal-poor galaxies (XMPGs) at relatively low redshift are excellent laboratories for studying galaxy formation and evolution in the early universe. Much effort has been spent on identifying them from large-scale spectroscopic surveys or spectroscopic follow-up observations. Previous work has identified a few hundred XMPGs. In this work, we obtain a large sample of 223 XMPGs at z < 1 from the early data of the Dark Energy Spectroscopic Instrument (DESI). The oxygen abundance is determined using the direct Te method based on the detection of the [O iii]λ4363 line. The sample includes 95 confirmed XMPGs based on the oxygen abundance uncertainty; the remaining 128 galaxies are regarded as XMPG candidates. These XMPGs are only 0.01% of the total DESI observed galaxies. Their coordinates and other properties are provided in the paper. The most XMPGs have an oxygen abundance of ~1/34 Z⊙, a stellar mass of about 1.5 × 107M⊙, and a star formation rate of 0.22 M⊙ yr–1. The two most XMPGs present distinct morphologies suggesting different formation mechanisms. The local environmental investigation shows that XMPGs preferentially reside in relatively low-density regions. Many of them fall below the stellar mass–metallicity relations (MZRs) of normal star-forming galaxies. From a comparison of the MZR with theoretical simulations, it appears that XMPGs are good analogs to high-redshift star-forming galaxies. The nature of these XMPG populations will be further investigated in detail with larger and more complete samples from the ongoing DESI survey.
- Research Organization:
- Univ. of Michigan, Ann Arbor, MI (United States); University of Michigan, Ann Arbor, MI (United States)
- Sponsoring Organization:
- Beijing Municipal Natural Science Foundation; National Key R&D Program of China; National Natural Science Foundation of China; USDOE Office of Science (SC), High Energy Physics (HEP)
- Grant/Contract Number:
- AC02-05CH11231; SC0019193
- Other Award/Contract Number:
- 2022YFA1602902
2023YFA1607800
12120101003
12373010
11890691
1222028
- OSTI ID:
- 2375034
- Alternate ID(s):
- OSTI ID: 3007500
- Journal Information:
- The Astrophysical Journal, Journal Name: The Astrophysical Journal Journal Issue: 2 Vol. 961; ISSN 0004-637X
- Publisher:
- IOP PublishingCopyright Statement
- Country of Publication:
- United States
- Language:
- English
Similar Records
Mass–Metallicity Relation and Fundamental Metallicity Relation of Metal-poor Star-forming Galaxies at 0.6<$Z$<0.9 from the eBOSS Survey
Extremely Metal-Poor Galaxies in DESI DR1: Connections to Galaxies in the Early Universe
Journal Article
·
Wed Dec 05 19:00:00 EST 2018
· The Astrophysical Journal (Online)
·
OSTI ID:1544072
Extremely Metal-Poor Galaxies in DESI DR1: Connections to Galaxies in the Early Universe
Journal Article
·
Thu Mar 05 19:00:00 EST 2026
· No journal information
·
OSTI ID:3023407