AAS Journals
Published August 22, 2024 | Version v1
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Data for "The impact of mass-dependent stochasticity at cosmic dawn"

Authors/Creators

  • 1. ROR icon University of Copenhagen
  • 2. Cosmic Dawn Center

Description

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]

Files

mass_dependent_stochasticity_LFs.zip

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Additional details

Related works

Is described by
Journal article: arXiv:2405.13108 (arXiv)
Is identical to
Dataset: https://github.com/violagelli/Stochastic_model_UVLF.git (Other)