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Halfway to the Peak: Spatially Resolved Star Formation and Kinematics in a z = 0.54 Dusty Galaxy with JWST/MIRI

  • Authors: Jason Young, Alexandra Pope, Anna Sajina, Lin Yan, Thiago S Gonçalves, Miriam Eleazer, Stacey Alberts, Lee Armus, Matteo Bonato, Daniel A. Dale, Duncan Farrah, Carl Ferkinhoff, Christopher C. Hayward, Jed McKinney, Eric J. Murphy, Nicole Nesvadba, Patrick Ogle, Leonid Sajkov, Sylvain Veilleux

Jason Young et al 2023 The Astrophysical Journal Letters 958 .

  • Provider: AAS Journals

Caption: Figure 1.

Top row: collapsed image of all four MRS spectral cubes and HST F160W (rest-frame optical) image, with a 4σ MRS detection contour (full galaxy aperture, black) and five selected regions (colored circles). Bottom: spectra extracted from the full galaxy aperture and the five subregions, and the archival IRS spectrum (top thin spectrum). The IRS slit is close to the size of the entire MRS field of view. Spectra are normalized and offset for visual clarity, and color coded the same as the regions. The vertical shaded bands mark key spectral features.

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