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COMPAS v02.27.05 output at representative metallicities

Team COMPAS


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  <identifier identifierType="DOI">10.5281/zenodo.6346444</identifier>
  <creators>
    <creator>
      <creatorName>Team COMPAS</creatorName>
    </creator>
  </creators>
  <titles>
    <title>COMPAS v02.27.05 output at representative metallicities</title>
  </titles>
  <publisher>Zenodo</publisher>
  <publicationYear>2022</publicationYear>
  <dates>
    <date dateType="Issued">2022-03-14</date>
  </dates>
  <language>en</language>
  <resourceType resourceTypeGeneral="Dataset"/>
  <alternateIdentifiers>
    <alternateIdentifier alternateIdentifierType="url">https://zenodo.org/record/6346444</alternateIdentifier>
  </alternateIdentifiers>
  <relatedIdentifiers>
    <relatedIdentifier relatedIdentifierType="DOI" relationType="IsVersionOf">10.5281/zenodo.6346443</relatedIdentifier>
    <relatedIdentifier relatedIdentifierType="URL" relationType="IsPartOf">https://zenodo.org/communities/compas</relatedIdentifier>
  </relatedIdentifiers>
  <version>02.27.05</version>
  <rightsList>
    <rights rightsURI="https://creativecommons.org/licenses/by/4.0/legalcode">Creative Commons Attribution 4.0 International</rights>
    <rights rightsURI="info:eu-repo/semantics/openAccess">Open Access</rights>
  </rightsList>
  <descriptions>
    <description descriptionType="Abstract">&lt;p&gt;This dataset contains the output data of rapid binary population synthesis produced using COMPAS v02.27.05. The details of the initial conditions and setup are described in the &amp;quot;COMPAS_settings_table.pdf&amp;quot; file. We simulate 5 million binaries, at representative metallicities, and store them in HDF5 files, the default format for COMPAS simulations. Each HDF5 file contains the following groups:&lt;/p&gt;

&lt;ul&gt;
	&lt;li&gt;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;lsquo;/BSE_Common_Envelopes&amp;rsquo;&lt;/li&gt;
	&lt;li&gt;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;lsquo;/BSE_Double_Compact_Objects&amp;rsquo;&lt;/li&gt;
	&lt;li&gt;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;lsquo;/BSE_Supernovae&amp;rsquo;&lt;/li&gt;
	&lt;li&gt;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;lsquo;/BSE_System_Parameters&amp;rsquo;&lt;/li&gt;
	&lt;li&gt;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;nbsp;&amp;lsquo;/Run_Details&amp;rsquo;&lt;/li&gt;
&lt;/ul&gt;

&lt;p&gt;For details about the data, such as variable names and attributes, visit the &lt;a href="https://compas.readthedocs.io/en/latest/"&gt;compas.readthedocs.io&lt;/a&gt;.&lt;br&gt;
The metallicities chosen for the simulations are:&lt;/p&gt;

&lt;ol&gt;
	&lt;li&gt;Z=0.0001: the lowest metallicity accounted for in our stellar evolution tracks;&lt;/li&gt;
	&lt;li&gt;Z=0.0002: a proxy metallicity for I Zwicky 18;&lt;/li&gt;
	&lt;li&gt;Z=0.001;&lt;/li&gt;
	&lt;li&gt;Z=0.0021: a proxy metallicity for the Small Magellanic Cloud;&lt;/li&gt;
	&lt;li&gt;Z=0.0047: a proxy metallicity for the Large Magellanic Cloud;&lt;/li&gt;
	&lt;li&gt;Z=0.01;&lt;/li&gt;
	&lt;li&gt;Z=0.0142: a metallicity representative of&amp;nbsp;the Sun;&lt;/li&gt;
	&lt;li&gt;Z=0.02: a super-solar metallicity, aka &amp;quot;old Solar&amp;quot;;&lt;/li&gt;
	&lt;li&gt;Z=0.03: the highest metallicity accounted for in&amp;nbsp;our stellar evolution tracks;&lt;/li&gt;
	&lt;li&gt;U[log&lt;sub&gt;10&lt;/sub&gt;(0.0001), log&lt;sub&gt;10&lt;/sub&gt;(0.03)]: log-uniformly distributed metallicities from the COMPAS metallicities.&lt;/li&gt;
&lt;/ol&gt;

&lt;p&gt;This results in 50 million binaries in total.&lt;/p&gt;

&lt;p&gt;In addition&amp;nbsp;to the Table in the &amp;quot;COMPAS_settings_table.pdf&amp;quot; file, we include a &amp;quot;Run Details&amp;quot; text file, which contains the setup as specified via COMPAS, for a particular batch of the Z=0.02 simulation. This file contains a representative description of the global properties of all the 10 simulations, but some details, e.g. Clock-Time, vary from batch to batch.&lt;/p&gt;

&lt;p&gt;For questions, comments, or suggestions, contact compas-user@googlegroups.com or visit &lt;a href="https://compas.science/"&gt;compas.science/&lt;/a&gt;.&lt;br&gt;
Visit &lt;a href="https://github.com/TeamCOMPAS/COMPAS"&gt;Team COMPAS Github page&lt;/a&gt; to get access to the source code.&lt;br&gt;
Finally, if you use any of these data, we kindly request that, in recognition of this team effort, the paper is cited as:&lt;/p&gt;

&lt;p&gt;Team COMPAS: J. Riley et al., &amp;ldquo;Rapid Stellar and Binary Population Synthesis with COMPAS&amp;rdquo;, &lt;em&gt;The Astrophysical Journal Supplement Series&lt;/em&gt;, vol. 258, no. 2, 2022. &lt;a href="https://iopscience.iop.org/article/10.3847/1538-4365/ac416c/meta"&gt;doi:10.3847/1538-4365/ac416c&lt;/a&gt;.&lt;/p&gt;</description>
  </descriptions>
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