DESI Emission-line Galaxies: Unveiling the Diversity of [O ii] Profiles and Its Links to Star Formation and Morphology

Abstract We study the [O ii ] profiles of emission-line galaxies (ELGs) from the Early Data Release of the Dark Energy Spectroscopic Instrument (DESI). To this end, we decompose and classify the shape of [O ii ] profiles with the first two eigenspectra derived from principal component analysis. Our results show that DESI ELGs have diverse line profiles, which can be categorized into three main types: (1) narrow lines with a median width of ∼50 km s −1 , (2) broad lines with a median width of ∼80 km s −1 , and (3) two redshift systems with a median velocity separation of ∼150 km s −1 , i.e., double-peak galaxies. To investigate the connections between the line profiles and galaxy properties, we utilize the information from the COSMOS data set and compare the properties of ELGs, including star formation rate (SFR) and galaxy morphology, with the average properties of reference star-forming galaxies with similar stellar mass, sizes, and redshifts. Our findings show that, on average, DESI ELGs have a higher SFR and more asymmetrical/disturbed morphology than the reference galaxies. Moreover, we uncover a relationship between the line profiles, the excess SFR, and the excess asymmetry parameter, showing that DESI ELGs with broader [O ii ] line profiles have more disturbed morphology and higher SFR than the reference star-forming galaxies. Finally, we discuss possible physical mechanisms giving rise to the observed relationship and the implications of our findings on the galaxy clustering measurements, including the halo occupation distribution modeling of DESI ELGs and the observed excess velocity dispersion of the satellite ELGs.

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Publication Details

Journal
The Astrophysical Journal
Published
2024-12-01
DOI
https://doi.org/10.3847/1538-4357/ad8f33
Citations
2
Primary Topic
Galaxies: Formation, Evolution, Phenomena
Type
article
Field-Weighted Citation Impact
0.66

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article

DESI Emission-line Galaxies: Unveiling the Diversity of [O ii] Profiles and Its Links to Star Formation and Morphology

Ting-Wen Lan, A. Lambert, A. Muñoz-Gutiérrez, D. Brooks et al.
2 citations
The Astrophysical Journal
Galaxies: Formation, Evolution, Phenomena
0.66
article

DESI Emission-line Galaxies: Unveiling the Diversity of [O ii] Profiles and Its Links to Star Formation and Morphology

Ting-Wen Lan, A. Lambert, A. Muñoz-Gutiérrez, D. Brooks, Jason Xavier Prochaska, Benjamin Alan Weaver, D. Bianchi, Axel de la Macorra, Martin Landriau, G. Gutierrez, Shaun Cole, M. Schubnell, Jeffrey A. Newman, J. Guy, Eusebio Sanchez, Satya Gontcho A Gontcho, G. Tarlé, J. Aguilar, M. Siudek, Steven P. Ahlen, Aaron Meisner, K. Dawson, R. Miquel, Theodore S. Kisner, John Moustakas, Claire Poppett, K. Honscheid, Hee‐Jong Seo, Hu Zou, Graziano Rossi, J. E. Forero-Romero, P Doel, E. Gaztañaga, T. Claybaugh, F. Prada, R. Kehoe, D. Sprayberry
article en
2 citations

Abstract

Abstract We study the [O ii ] profiles of emission-line galaxies (ELGs) from the Early Data Release of the Dark Energy Spectroscopic Instrument (DESI). To this end, we decompose and classify the shape of [O ii ] profiles with the first two eigenspectra derived from principal component analysis. Our results show that DESI ELGs have diverse line profiles, which can be categorized into three main types: (1) narrow lines with a median width of ∼50 km s −1 , (2) broad lines with a median width of ∼80 km s −1 , and (3) two redshift systems with a median velocity separation of ∼150 km s −1 , i.e., double-peak galaxies. To investigate the connections between the line profiles and galaxy properties, we utilize the information from the COSMOS data set and compare the properties of ELGs, including star formation rate (SFR) and galaxy morphology, with the average properties of reference star-forming galaxies with similar stellar mass, sizes, and redshifts. Our findings show that, on average, DESI ELGs have a higher SFR and more asymmetrical/disturbed morphology than the reference galaxies. Moreover, we uncover a relationship between the line profiles, the excess SFR, and the excess asymmetry parameter, showing that DESI ELGs with broader [O ii ] line profiles have more disturbed morphology and higher SFR than the reference star-forming galaxies. Finally, we discuss possible physical mechanisms giving rise to the observed relationship and the implications of our findings on the galaxy clustering measurements, including the halo occupation distribution modeling of DESI ELGs and the observed excess velocity dispersion of the satellite ELGs.

The Astrophysical JournalVol. 977(2)
National Taiwan University (TW), Campbell Collaboration (NO)
U.S. Department of Energy, Ministry of Education, India, Ministerio de Ciencia e Innovación, National Taiwan University, Narodowa Agencja Wymiany Akademickiej, National Science and Technology Council, Office of Science, High Energy Physics
Openalex Percentile: Top 26%
Galaxies: Formation, Evolution, Phenomena
0.66
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