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ZENODO
Dataset . 2022
License: CC BY
Data sources: Datacite
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ZENODO
Dataset . 2022
License: CC BY
Data sources: Datacite
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ZENODO
Dataset . 2022
License: CC BY
Data sources: ZENODO
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ZENODO
Dataset . 2022
License: CC BY
Data sources: Datacite
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ZENODO
Dataset . 2022
License: CC BY
Data sources: ZENODO
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Claim

Supporting information for "An Atlas of Convection in Main-Sequence Stars"

Research datakeyboard_double_arrow_right Dataset 16 Mar 2022Publisher:ZenodoFunded by:NSF | Kavli Institute for Theor...
Authors: Adam S Jermyn; Evan H Anders; Daniel Lecoanet; Matteo Cantiello;

doi: 10.5281/zenodo.6363521 , 10.5281/zenodo.6533097 , 10.5281/zenodo.6363522

Supporting information for "An Atlas of Convection in Main-Sequence Stars"

Abstract

The contents of 'code.zip' are the plotting and analysis scripts used in generating the plots in this work. The contents of 'atlas_Z_MW_time_2022_05_06_13_40_06_sha_94d5.zip' are the history files for the MESA runs which the plotting scripts analyze. Each file is in its own directory, labelled by the mass of the star in solar units.

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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!
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