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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 2.

We display the estimated intensities along with their respective errors with boxes at four redshift bins. The red line is an empirical redshift trend of the correlated continuum residual. The shaded green region indicates the redshift range where we anticipate contributions from CO(3–2), while the other bins can contain correlated continuum.

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