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Dataset for: "Modeling the Hα Emission Surrounding Spica using the Lyman Continuum from a Gravity-darkened Central Star"

<p><strong>Summary:&nbsp;</strong>This deposit supplements the manuscript, &quot;<em>Modeling the H&alpha;&nbsp;Emission Surrounding Spica using the Lyman&nbsp;Continuum from a Gravity-darkened Central Star</em>&quot;, accepted to the Astrophysical Journal. The tar.gz archive file contains&nbsp;an example Cloudy script and associated data. The complete listing of the files included in this archive file are given here:&nbsp;&nbsp;</p> <p>&nbsp; &nbsp; ReadMe&nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; Documentation file<br> &nbsp; &nbsp; example_cloudy_input_file.txt &nbsp; &nbsp; &nbsp; &nbsp;Cloudy script<br> &nbsp; &nbsp; spica_i=100_V5_solar.ascii &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;Spica input stellar spectral energy distribution<br> &nbsp; &nbsp; spica_i=110_V5_solar.ascii &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;Spica input stellar spectral energy distribution<br> &nbsp; &nbsp; spica_i=116_V5_solar.ascii &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;Spica input stellar spectral energy distribution<br> &nbsp; &nbsp; spica_i=120_V5_solar.ascii &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;Spica input stellar spectral energy distribution<br> &nbsp; &nbsp; spica_i=130_V5_solar.ascii &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;Spica input stellar spectral energy distribution<br> &nbsp; &nbsp; spica_i=140_V5_solar.ascii &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;Spica input stellar spectral energy distribution<br> &nbsp; &nbsp; spica_i=150_V5_solar.ascii &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;Spica input stellar spectral energy distribution<br> &nbsp; &nbsp; spica_i=160_V5_solar.ascii &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;Spica input stellar spectral energy distribution<br> &nbsp; &nbsp; spica_i=170_V5_solar.ascii &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;Spica input stellar spectral energy distribution<br> &nbsp; &nbsp; spica_i=180_V5_solar.ascii &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;Spica input stellar spectral energy distribution<br> &nbsp; &nbsp; spica_i=90_V5_solar.ascii&nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; Spica input stellar spectral energy distribution<br> &nbsp;</p> <p><strong>System requirements:</strong> The input script and SED files correspond to Cloudy code&nbsp;version 17.02:<br> &nbsp; &nbsp; &nbsp; &nbsp; Codebase: <a href="https://trac.nublado.org/">https://trac.nublado.org/</a><br> &nbsp; &nbsp; &nbsp; &nbsp; Primary documentation: Ferland et al. (<a href="https://ui.adsabs.harvard.edu/abs/2017RMxAA..53..385F/abstract">2017RMxAA..53..385F</a>; arXiv:<a href="https://arxiv.org/abs/1705.10877">1705.10877</a>)<br> &nbsp;</p> <p>Additional documentation provided in the ReadMe file.</p>

ShareScore

44/100

Overall dataset sharing score

Score breakdown

These five areas show where the dataset supports — or may limit — practical reuse.

Stewardship
4
Harmonization
8
Access
16
Reuse readiness
8
Engagement
8