POLAR-I: linking the 21-cm signal from the epoch of reionization to galaxy 
formation

Ma, Qing-Bo; Ghara, Raghunath; Ciardi, Benedetta; Iliev, Ilian T.; Koopmans, Léon V. E.; Mellema, Garrelt; Mondal, Rajesh; Zaroubi, Saleem

doi:10.1093/mnras/stad1203

アイテム詳細

登録内容を編集ファイル形式で保存

一時保存へ追加

タグ情報を表示リリース履歴を表示詳細要約

公開

学術論文

POLAR-I: linking the 21-cm signal from the epoch of reionization to galaxy formation

MPS-Authors

/persons/resource/persons18445

Ciardi, Benedetta
Computational Structure Formation, MPI for Astrophysics, Max Planck Society;

External Resource

There are no locators available

Fulltext (restricted access)

There are currently no full texts shared for your IP range.

フルテキスト (公開)

公開されているフルテキストはありません

付随資料 (公開)

There is no public supplementary material available

引用

Ma, Q.-B., Ghara, R., Ciardi, B., Iliev, I. T., Koopmans, L. V. E., Mellema, G., Mondal, R., & Zaroubi, S. (2023). POLAR-I: linking the 21-cm signal from the epoch of reionization to galaxy formation. Monthly Notices of the Royal Astronomical Society, 522(3), 3284-3297. doi:10.1093/mnras/stad1203.

引用: https://hdl.handle.net/21.11116/0000-000D-DF35-D

要旨

To self-consistently model galactic properties, reionization of the intergalactic medium, and the associated 21-cm signal, we have developed the algorithm polar by integrating the one-dimensional radiative transfer code grizzly with the semi-analytical galaxy formation code L-Galaxies 2020. Our proof-of-concept results are consistent with observations of the star formation rate history, UV luminosity function, and the CMB Thomson scattering optical depth. We then investigate how different galaxy formation models affect UV luminosity functions and 21-cm power spectra, and find that while the former are most sensitive to the parameters describing the merger of haloes, the latter have a stronger dependence on the supernovae feedback parameters, and both are affected by the escape fraction model.