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Observational Evidence for Large-scale Gas Heating in a Galaxy Protocluster at z = 2.30

  • Authors: Chenze Dong, Khee-Gan Lee, Metin Ata, Benjamin Horowitz, Rieko Momose

Chenze Dong et al 2023 The Astrophysical Journal Letters 945 .

  • Provider: AAS Journals

Caption: Figure 3.

Distribution of ﹩{\delta }_{F}^{\mathrm{pc}}﹩ derived from the method in Section 3.2. We include all nine protoclusters in the overlap of CLAMATO and COSTCO volumes. The blue histogram is the distribution of ﹩{\delta }_{F}^{\mathrm{pc}}﹩ in 1140 COSTCO-FGPA mock realizations, the orange line marks the ﹩{\delta }_{F}^{\mathrm{pc}}﹩ of the corresponding protoclusters in the observed CLAMATO, and the gray vertical dashed line represents ﹩{\delta }_{F}^{\mathrm{pc}}=0﹩. We highlight COSTCO-I with bold text (center panel); the mocks for this structure are clearly inconsistent with the CLAMATO measurement.

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