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ZENODO
Dataset . 2024
License: CC BY
Data sources: ZENODO
ZENODO
Dataset . 2024
License: CC BY
Data sources: Datacite
ZENODO
Dataset . 2024
License: CC BY
Data sources: Datacite
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Data for "The impact of mass-dependent stochasticity at cosmic dawn"

Authors: Gelli, Viola; Mason, Charlotte; Hayward, Christopher;

Data for "The impact of mass-dependent stochasticity at cosmic dawn"

Abstract

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]

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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
0
Average
Average
Average