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A Measurement of CO(3–2) Line Emission from eBOSS Galaxies at z ∼ 0.5 Using Planck Data

  • Authors: Anirban Roy, Nicholas Battaglia, Anthony R. Pullen

Anirban Roy et al 2026 The Astrophysical Journal Letters 1012 .

  • Provider: AAS Journals

Caption: Figure 4.

Various CO(3–2) model predictions are compared with the measured CO(3–2) intensity at z ∼ 0.5. The legend provides descriptions of the SFR models, while annotations within the gray boxes denote the models that convert SFR to CO(3–2) line luminosities. The horizontal bar for a particular line luminosity model is calculated from the variance in intensities for the different SFR models.

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