Identifying and characterizing the most heavily dust-obscured galaxies at 1 ≤ z ≤ 4
Identifying and characterizing the most heavily dust-obscured galaxies at 1 ≤ z ≤ 4
DOI | Resolve DOI: https://doi.org/10.1093/mnras/stac3455 |
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Author | Search for: 1ORCID identifier: https://orcid.org/0000-0003-3243-9969; Search for: ; Search for: ; Search for: 1; Search for: |
Affiliation |
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Funder | Search for: National Science Foundation; Search for: Canadian Space Agency; Search for: European Southern Observatory |
Format | Text, Article |
Subject | methods: observational; dust; extinction; galaxies: general; galaxies: evolution; techniques: photometric |
Abstract | |
Publication date | 2022-11-29 |
Publisher | Oxford Academic Royal Astronomical Society |
In | |
Language | English |
Peer reviewed | Yes |
Export citation | Export as RIS |
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Record identifier | d1c561ac-d67e-46ae-a9fd-d64363cbbac9 |
Record created | 2023-08-31 |
Record modified | 2023-08-31 |
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