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SQuIGG﹩\overrightarrow{L}﹩E: Buried Star Formation Cannot Explain the Rapidly Fading CO(2–1) Luminosity in Massive, z ∼ 0.7 Post-starburst Galaxies

  • Authors: David J. Setton, Justin S. Spilker, Rachel Bezanson, Katherine A. Suess, Jenny E. Greene, Andy D. Goulding, Elia Cenci, Vincenzo R. D'Onofrio, Robert Feldmann, Mariska Kriek, Anika Kumar, Yuanze Luo, Desika Narayanan, Margaret E. Verrico, Pengpei Zhu

David J. Setton et al 2025 The Astronomical Journal 170 .

  • Provider: AAS Journals

Caption: Figure 7.

Demonstration of the new SED fitting adopted in this work, as in Figure 6. Here, we highlight J0910+0218, our second most CO-luminous galaxy that is detected in the MIR and in ancillary Herschel imaging. In contrast with J1157+0132 (see Figure 6), both the τBC Tied and τBC Free fits can provide a good match to the full SED, including Herschel. Even in the case where higher τBC allows for a somewhat higher SFR, the total IR luminosity is essentially identical between these models.

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