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

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