The Coordinated Radio and Infrared Survey for High-Mass Star Formation (CORNISH) is an arcsecond-resolution radio continuum survey covering 10°< l < 65° and |b| < 1° at 5 GHz. With an overlapping footprint, it is intended to be the radio counterpart to mid-IR GLIMPSE/MIPSGAL surveys and the near-IR UKIDSS survey of the Galactic plane. One of its main science goals include better characterization of ultra-compact HII regions, massive young stellar objects, and evolved OB stars in the plane of the galaxy. The link to the homepage of the CORNISH survey can be found here.
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CORNISH_Continuum_Data_Access.pdf
CORNISH_Continuum_Data_Access.pdf
Sep 5, 2016 - CORNISH Extended Observations: Continuum (2D)
Adobe PDF - 32.0 KB - MD5: 04f6c7c778e990ea2d6998b50d637d6f
CORNISH_Catalog_Data_Access.pdf
CORNISH_Catalog_Data_Access.pdf
Sep 5, 2016 - CORNISH Catalogs: Source-Based Lists
Adobe PDF - 27.6 KB - MD5: 37731b60d7e6161b44ba78f3d1b4fb9e
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