RUBIES: JWST/NIRSpec Resolves Evolutionary Phases of Dusty Star-forming Galaxies at <i>z</i> ∼ 2

Abstract The dearth of high-quality spectroscopy of dusty star-forming galaxies (DSFGs)—the main drivers of the assembly of dust and stellar mass at the peak of activity in the Universe—greatly hinders our ability to interpret their physical processes and evolutionary pathways. We present JWST/NIRSpec observations from RUBIES of four submillimeter-selected, Atacama Large Millimeter/submillimeter Array (ALMA)-detected DSFGs at cosmic noon, z ∼ 2.3–2.7. While photometry uniformly suggests vigorous ongoing star formation for the entire sample in line with canonical DSFGs, the spectra differ: one source has spectroscopic evidence of an evolved stellar population, indicating a recent transition to a post-starburst phase, while the remainder show strong spectroscopic signatures of ongoing starbursts. All four galaxies are infrared luminous (log 10 L IR / L ⊙ &gt; 12.4), massive (log 10 M ⋆ / M ⊙ &gt; 11), and very dust obscured ( A V ∼ 3–4 ABmag). Leveraging detections of multiple Balmer and Paschen lines, we derive an optical attenuation curve consistent with Calzetti overall, yet an optical extinction ratio R V ∼ 2.5, potentially indicating smaller dust grains or differences in star-dust geometry. This case study provides some of the first detailed spectroscopic evidence that the DSFGs encompass a heterogeneous sample spanning a range of star formation properties and evolutionary stages, and illustrates the advantages of synergistic JWST and ALMA analysis of DSFGs.

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Institutions

Publication Details

Journal
The Astrophysical Journal
Published
2025-03-24
DOI
https://doi.org/10.3847/1538-4357/adb8e1
Citations
6
Primary Topic
Galaxies: Formation, Evolution, Phenomena
Type
article
Field-Weighted Citation Impact
6.93

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article

RUBIES: JWST/NIRSpec Resolves Evolutionary Phases of Dusty Star-forming Galaxies at z ∼ 2

Ian McConachie, Jed McKinney, Jenny E. Greene, David J. Setton et al.
6 citations
The Astrophysical Journal
Galaxies: Formation, Evolution, Phenomena
6.93
article

RUBIES: JWST/NIRSpec Resolves Evolutionary Phases of Dusty Star-forming Galaxies at z ∼ 2

Ian McConachie, Jed McKinney, Jenny E. Greene, David J. Setton, Caitlin M. Casey, Leindert Boogaard, Desika Narayanan, Christina C. Williams, Olivia R. Cooper, Joel Leja, Katherine A. Suess, Nikko J. Cleri, Erini Lambrides, B. Gullberg, Victoria Strait, Gabriel Brammer, Raphael E. Hviding, Rashmi Gottumukkala, Michael V. Maseda, Arianna S. Long, Steven Gillman, Sune Toft, Sedona H. Price, Sinclaire M. Manning, Andrea Weibel, K. E. Heintz, Anna de Graaff, Michaela Hirschmann
article en
6 citations

Abstract

Abstract The dearth of high-quality spectroscopy of dusty star-forming galaxies (DSFGs)—the main drivers of the assembly of dust and stellar mass at the peak of activity in the Universe—greatly hinders our ability to interpret their physical processes and evolutionary pathways. We present JWST/NIRSpec observations from RUBIES of four submillimeter-selected, Atacama Large Millimeter/submillimeter Array (ALMA)-detected DSFGs at cosmic noon, z ∼ 2.3–2.7. While photometry uniformly suggests vigorous ongoing star formation for the entire sample in line with canonical DSFGs, the spectra differ: one source has spectroscopic evidence of an evolved stellar population, indicating a recent transition to a post-starburst phase, while the remainder show strong spectroscopic signatures of ongoing starbursts. All four galaxies are infrared luminous (log 10 L IR / L ⊙ &gt; 12.4), massive (log 10 M ⋆ / M ⊙ &gt; 11), and very dust obscured ( A V ∼ 3–4 ABmag). Leveraging detections of multiple Balmer and Paschen lines, we derive an optical attenuation curve consistent with Calzetti overall, yet an optical extinction ratio R V ∼ 2.5, potentially indicating smaller dust grains or differences in star-dust geometry. This case study provides some of the first detailed spectroscopic evidence that the DSFGs encompass a heterogeneous sample spanning a range of star formation properties and evolutionary stages, and illustrates the advantages of synergistic JWST and ALMA analysis of DSFGs.

The Astrophysical JournalVol. 982(2)
University of Copenhagen (DK), DAWN Center for Independent Living (US), Technical University of Denmark (DK)
National Science Foundation, National Aeronautics and Space Administration, Research Corporation for Science Advancement, University of Texas at Austin, Space Telescope Science Institute, National Research Foundation, Danmarks Grundforskningsfond, Deutsches Zentrum für Luft- und Raumfahrt, Bundesministerium für Wirtschaft und Energie, Staatssekretariat für Bildung, Forschung und Innovation
Openalex Percentile: Top 4%
Galaxies: Formation, Evolution, Phenomena
6.93
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