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We present an assessment of the performance of WISE and the AllWISE datarelease in a section of the Galactic Plane. We lay out an approach toincreasing the reliability of point source photometry extracted from theAllWISE catalog in Galactic Plane regions using parameters provided in thecatalog. We use the resulting catalog to construct a new, revised young stardetection and classification scheme combining WISE and 2MASS near andmid-infrared colors and magnitudes and test it in a section of the Outer MilkyWay. The clustering properties of the candidate Class I and II stars using anearest neighbor density calculation and the two-point correlation functionsuggest that the majority of stars do form in massive star forming regions, andany isolated mode of star formation is at most a small fraction of the totalstar forming output of the Galaxy. We also show that the isolated component maybe very small and could represent the tail end of a single mechanism of starformation in line with models of molecular cloud collapse with supersonicturbulence and not a separate mode all to itself.

astrophysical journal/the astrophysical journal

A Classification Scheme for Young Stellar Objects Using the WIDE-FIELD  INFRARED SURVEY EXPLORER AllWISE Catalog: Revealing Low-Density Star  Formation in the Outer Galaxy