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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 1.

The panels depict intensity images generated by galaxies from four distinct redshift bins, stacked onto the CO(2–1) Type 2 map derived from Planck data. The target bin is z = 0.4940–0.5724, but neighboring bins can also transmit redshifted CO(3–2). The beam FWHM for the Type 2 is ﹩15^{\prime} ﹩ (P. A. Ade et al. 2014a).

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