Data for "The impact of mass-dependent stochasticity at cosmic dawn"
收藏Zenodo2024-08-27 更新2026-05-26 收录
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https://zenodo.org/doi/10.5281/zenodo.13370198
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资源简介:
Data for for the mass-dependent stochasticity model described in Gelli, Mason & Hayward 2024, ApJ
The "LF/" folder contains the UV luminosity functions for the mass-dependent UV scatter model for z = 5-20. The two columns are:
- UV magnitude Muv [mag]
- number density log10_phi [/mag/Mpc^3]
The "SFRD/" folder contains the redshift evolution of the UV luminosity density (obtained by integrating the UVLF down to Muv=-17) and the star formation rate density (derived using [Madau+99](https://iopscience.iop.org/article/10.1086/306975)). The columns are:
- redshift z
- luminosity density log10_rhoUV [erg/s/Hz/Mpc^3]
- star formation rate density log10_SFRD [Msun/yr/Mpc^3]
提供机构:
Zenodo
创建时间:
2024-08-27



