Halfway to the Peak: Ice Absorption Bands at <i>z</i> ≈ 0.5 with JWST MIRI/MRS

Abstract This paper presents the first combined detections of CO 2 , CO, XCN, and water ices beyond the local Universe. We find gas-phase CO in addition to the solid phase CO. Our source, SSTXFLS J172458.3+591545, is a z = 0.494 star-forming galaxy that also hosts a deeply obscured AGN. The profiles of its ice features are consistent with those of other Galactic and local galaxy sources, and the implied ice mantle composition is similar to that of even more obscured sources. The ice features indicate the presence of a compact nucleus in our Galaxy and allow us to place constraints on its density and temperature ( n &gt; 10 5 cm −3 and T = 20–90 K). We infer the visual extinction towards this nucleus to be A V ≈ 6–7. An observed plot of τ Si versus τ CO2 / τ Si can be viewed as a probe for both the total dustiness of a system as well as the clumpiness of the dust along the line of sight. This paper highlights the potential of using JWST MIRI spectra to study the dust composition and geometric distribution of sources beyond the local Universe.

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Publication Details

Journal
The Astrophysical Journal
Published
2025-05-23
DOI
https://doi.org/10.3847/1538-4357/adc44a
Citations
1
Primary Topic
Astrophysics and Star Formation Studies
Type
article
Field-Weighted Citation Impact
1.15

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article

Halfway to the Peak: Ice Absorption Bands at z ≈ 0.5 with JWST MIRI/MRS

Jed McKinney, Thomas S. -Y. Lai, Jason Young, Miriam Eleazer et al.
1 citations
The Astrophysical Journal
Astrophysics and Star Formation Studies
1.15
article

Halfway to the Peak: Ice Absorption Bands at z ≈ 0.5 with JWST MIRI/MRS

Jed McKinney, Thomas S. -Y. Lai, Jason Young, Miriam Eleazer, H. W. W. Spoon, Sylvain Veilleux, L. Armus, D. Farrah, Lin Yan, Mark Lacy, Alexandra Pope, Anna Sajina
article en
1 citations

Abstract

Abstract This paper presents the first combined detections of CO 2 , CO, XCN, and water ices beyond the local Universe. We find gas-phase CO in addition to the solid phase CO. Our source, SSTXFLS J172458.3+591545, is a z = 0.494 star-forming galaxy that also hosts a deeply obscured AGN. The profiles of its ice features are consistent with those of other Galactic and local galaxy sources, and the implied ice mantle composition is similar to that of even more obscured sources. The ice features indicate the presence of a compact nucleus in our Galaxy and allow us to place constraints on its density and temperature ( n &gt; 10 5 cm −3 and T = 20–90 K). We infer the visual extinction towards this nucleus to be A V ≈ 6–7. An observed plot of τ Si versus τ CO2 / τ Si can be viewed as a probe for both the total dustiness of a system as well as the clumpiness of the dust along the line of sight. This paper highlights the potential of using JWST MIRI spectra to study the dust composition and geometric distribution of sources beyond the local Universe.

The Astrophysical JournalVol. 985(2)
University of Hawaiʻi at Mānoa (US), Tufts University (US), California Institute of Technology (US), Amherst College (US), Cornell University (US), Williams College (US), University of Massachusetts Amherst (US), Joint Space Science Institute (US), University of Maryland, College Park (US), The University of Texas at Austin (US)
Space Telescope Science Institute
Openalex Percentile: Top 19%
Astrophysics and Star Formation Studies
1.15
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