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We present a subset of the James Clerk Maxwell Telescope Gould Belt Survey's"first-look" results of the southern extent of the Orion A molecular cloud.Employing a two-step structure identification process, we constructedindividual catalogues for large-scale regions of significant emission labeledas "islands" and smaller-scale subregions called "fragments" using the 850$\mu$m continuum maps obtained using the Submillimetre Common-User BolometerArray 2 (SCUBA-2). We highlight the relationship between the concentration andJeans stability for regions of significant emission and present the results ofan investigation into the spatial distribution of Young Stellar Objectsdetected using the Spitzer Space Telescope and the Herschel Space Observatory.We find an apparent evolution in the velocity dispersion from Class 0 to ClassII objects which we derive from comparing our observations to a simple model.

From Clumps to Cores to Protostars: The JCMT Gould Belt Survey's "First-Look" analysis of Southern Orion A using SCUBA-2