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Article Dans Une Revue Monthly Notices of the Royal Astronomical Society Année : 2020

Constraining the second half of reionization with the Ly β forest

Résumé

We present an analysis of the evolution of the Lyman-series forest into the epoch of reionization using cosmological radiative transfer simulations in a scenario where reionization ends late. We explore models with different mid-points of reionization and gas temperatures. We find that once the simulations have been calibrated to match the mean flux of the observed Lyman-α (Ly α) forest at 4 < z < 6, they also naturally reproduce the distribution of effective optical depths of the Lyman-β (Ly β) forest in this redshift range. We note that the tail of the largest optical depths that is most challenging to match corresponds to the long absorption trough of ULAS J0148+0600, which we have previously shown to be rare in our simulations. We consider the evolution of the Lyman-series forest out to higher redshifts, and show that future observations of the Ly β forest at z > 6 will discriminate between different reionization histories. The evolution of the Ly α and Ly γ forests are less promising as a tool for pushing studies of reionization to higher redshifts due to the stronger saturation and foreground contamination, respectively.

Dates et versions

hal-02459822 , version 1 (29-01-2020)

Identifiants

Citer

Laura C. Keating, Girish Kulkarni, Martin G. Haehnelt, Jonathan Chardin, Laurence Voutquenne-Nazabadioko. Constraining the second half of reionization with the Ly β forest. Monthly Notices of the Royal Astronomical Society, 2020, 497 (1), pp.906-915. ⟨10.1093/mnras/staa1909⟩. ⟨hal-02459822⟩
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