The EDGES team publishes the first full public description of its 21-cm global-signal analysis pipeline, an open-source end-to-end software package, and the raw data from prior observations.
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Conditioning f_coll on tidal eigenvalues from small-box simulations allows low-resolution large-volume reionization runs to recover HI power spectra to within 2-5% on scales k less than 0.5 h/Mpc.
Lumina runs a 500 cMpc radiation-hydrodynamic simulation combining IllustrisTNG galaxy formation with six-bin M1 radiation transport to predict late stellar-driven HI reionization ending around z=4.75 and AGN-driven HeII reionization nearly complete by z=3.
citing papers explorer
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The EDGES Analysis Pipeline: Description and Validation
The EDGES team publishes the first full public description of its 21-cm global-signal analysis pipeline, an open-source end-to-end software package, and the raw data from prior observations.
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Conditioning halos on the tidal environment for fast and accurate HI power spectra during reionization
Conditioning f_coll on tidal eigenvalues from small-box simulations allows low-resolution large-volume reionization runs to recover HI power spectra to within 2-5% on scales k less than 0.5 h/Mpc.
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Introducing the Lumina project: large-volume radiation-hydrodynamic simulations of the epochs of hydrogen and helium reionization
Lumina runs a 500 cMpc radiation-hydrodynamic simulation combining IllustrisTNG galaxy formation with six-bin M1 radiation transport to predict late stellar-driven HI reionization ending around z=4.75 and AGN-driven HeII reionization nearly complete by z=3.