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The three-dimensional structure of Galactic molecular cloud complexes out to 2.5 kpc

<p>Data files for Dharmawardena et al., accepted MNRAS, 2022,&nbsp;<em>The three-dimensional structure of Galactic molecular cloud complexes out to 2.5 kpc.</em></p> <p>In this works we map the Interstellar Dust Extinction and Density in 3D using&nbsp;<em>Dustribution</em> code:&nbsp;Dharmawardena et al., 2022, Astronomy &amp; Astrophysics, Volume 658, id.A166, 30 pp.&nbsp;<a href="https://www.aanda.org/articles/aa/full_html/2022/02/aa41298-21/aa41298-21.html">https://www.aanda.org/articles/aa/full_html/2022/02/aa41298-21/aa41298-21.html</a></p> <p>The <em>Dustribution</em> code can be accessed from&nbsp;<a href="https://github.com/Thavisha/Dustribution">https://github.com/Thavisha/Dustribution</a></p> <p>The latest results from Dustribution can be interactively viewed and downloaded from <a href="https://www2.mpia-hd.mpg.de/homes/tmueller/projects/ThavishaDustDensity/index.html">https://www2.mpia-hd.mpg.de/homes/tmueller/projects/ThavishaDustDensity/index.html</a></p> <p>Data available here:</p> <p>- Trained gpy functions for all&nbsp; sixteen mapped regions which can be used to predict on any selected spherical or cartesian grid.&nbsp;&nbsp;</p> <p>-predicted cubes of 3D dust extinction and corresponding lbd boundary grids</p> <p>- predicted cubes of dust densities on cartesian grids and corresponding xyz boundary grids.&nbsp;</p> <p>- <em>astrodendro</em> derived dendrograms for all sixteen molecular cloud regions.</p> <p>- Tables of <em>astrodendro</em> produced parameters and calculated error bars for each region&#39;s substructure as described in appendix C of paper.&nbsp;</p> <p>- Tables 1,2,3 in main body of&nbsp;&nbsp;paper in .csv format.&nbsp;</p> <p>- 3D rendering videos of the sixteen mapped regions.</p>