Image Details

Choose export citation format:

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 5.

Top row: transmission–density relation of the whole CLAMATO volume. Bottom row: transmission–density relation of the 4.5 h −1 Mpc sphere centered at COSTCO-I. Left column: relations of underlying matter density vs. δ F after applying the FGPA and redshift-space distortions to the COSTCO matter density field. Middle column: same after applying sight-line sampling and Wiener reconstruction. Right column: Wiener-reconstructed Lyα flux as seen in the real CLAMATO data. The gray lines indicate the FGPA relation τ ∝ (1 + δ)1.6. All data are spatially smoothed with a 4 h −1 Mpc Gaussian kernel.

Other Images in This Article
Copyright and Terms & Conditions

Additional terms of reuse