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Dataset from: Gravitational wave sources in our Galactic backyard - Predictions for BHBH, BHNS and NSNS binaries in LISA

Wagg, Tom; Broekgaarden, Floor; de Mink, Selma; Frankel, Neige; van Son, Lieke; Justham, Stephen


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    <dct:title>Dataset from: Gravitational wave sources in our Galactic backyard - Predictions for BHBH, BHNS and NSNS binaries in LISA</dct:title>
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    <dcat:keyword>gravitational waves</dcat:keyword>
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    <dcat:keyword>black hole</dcat:keyword>
    <dcat:keyword>neutron star</dcat:keyword>
    <dcat:keyword>binary star</dcat:keyword>
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    <dct:description>&lt;p&gt;The data from all simulations used in &amp;quot;&lt;em&gt;&lt;strong&gt;Gravitational wave sources in our Galactic backyard: Predictions for BHBH, BHNS and NSNS binaries in LISA&lt;/strong&gt;&lt;/em&gt;&amp;quot;&lt;/p&gt; &lt;p&gt;Contents:&lt;/p&gt; &lt;ul&gt; &lt;li&gt;&lt;strong&gt;detections_and_totals.zip&lt;/strong&gt; &lt;ul&gt; &lt;li&gt;Contains for .npy files that contain tables of the detections and total DCOs in Milky Way. These were calculated with &lt;a href="https://github.com/TomWagg/detecting-DCOs-in-LISA/blob/main/simulation/postprocessing_notebooks/get_detection_rates.ipynb"&gt;this&lt;/a&gt; and &lt;a href="https://github.com/TomWagg/detecting-DCOs-in-LISA/blob/main/simulation/postprocessing_notebooks/get_total_DCOs_in_MW.ipynb"&gt;this&lt;/a&gt; notebook and are included for convenience so you don&amp;#39;t have to re-run these notebooks&lt;/li&gt; &lt;/ul&gt; &lt;/li&gt; &lt;li&gt;&lt;strong&gt;simulations_4yr.zip&lt;/strong&gt; &lt;ul&gt; &lt;li&gt;Contains 60 .h5 files that contain the main simulations for a 4-year LISA mission. Each file contains the results for a single DCO type (BHBH, BHNS or NSNS) and model variation (20 variations) are labeled as &lt;em&gt;{DCO_type}_{variation}_all.h5&lt;/em&gt;&lt;strong&gt;&lt;em&gt;. &lt;/em&gt;&lt;/strong&gt;&lt;/li&gt; &lt;/ul&gt; &lt;/li&gt; &lt;li&gt;&lt;strong&gt;simulations_10yr.zip&lt;/strong&gt; &lt;ul&gt; &lt;li&gt;As simulations_4yr.zip but for a 10-year LISA mission&lt;/li&gt; &lt;/ul&gt; &lt;/li&gt; &lt;li&gt;&lt;strong&gt;simple_mw_simulations.zip&lt;/strong&gt; &lt;ul&gt; &lt;li&gt;As simulations_4yr.zip but using a simple model for the Milky Way (discussed in Appendix D) and only for models A and F (hence only contains 6 .h5 files)&lt;/li&gt; &lt;/ul&gt; &lt;/li&gt; &lt;/ul&gt; &lt;p&gt;For a description of how to use these files to reproduce figures and results see the README.md in the associated GitHub repository: &lt;a href="https://github.com/TomWagg/detecting-DCOs-in-LISA"&gt;https://github.com/TomWagg/detecting-DCOs-in-LISA&lt;/a&gt;&lt;/p&gt; &lt;p&gt;Version 0.0.1 - Changes model E to E&amp;#39; as discussed in paper (now we allow HeHG donors to survive common-envelopes)&lt;/p&gt; &lt;ul&gt; &lt;/ul&gt;</dct:description>
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