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MAGAZ3NE: Far-IR and Radio Insights into the Nature and Properties of Ultramassive Galaxies at z ≳ 3

  • Authors: Wenjun Chang, Gillian Wilson, Ben Forrest, Ian McConachie, Tracy Webb, Allison Noble, Adam Muzzin, M. C. Cooper, Danilo Marchesini, Gabriela Canalizo, A. J. Battisti, Aurelien Henry, Percy Gomez, Stephanie M. Urbano Stawinski, M.E. Wisz

Wenjun Chang et al 2026 The Astrophysical Journal 1001 .

  • Provider: AAS Journals

Caption: Figure 2.

Ks-band images (left panels) and MOSFIRE 1D and 2D K-band spectra (right panels) for COS-DR3-195616 (upper) and COS-DR1-209435 (lower). The black solid lines show the observed 1D spectra. The gray shading shows the magnitude of the error spectrum. The solid red lines show the best-fit models from FAST++ described in Section 3.3. The green circles are drawn with a 2″ diameter. Red vertical dashed lines indicate the location of prominent emission lines. The y-axis shows flux density in units of 10−18 erg s−1 cm−2 Å−1, plotted from zero with a dash indicating one unit.

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