The MIPSGAL survey covers 278 sq. deg of the inner Galactic Plane at 24 μm (6” resolution) and 70 μm (18” resolution). It is meant to act as a longer wavelength component to the Spitzer-GLIMPSE Survey of the Galactic plane. Its two main science goals are to 1) identify high mass protostars and 2) probe properties of interstellar dust in the inner galaxy. The link to the homepage of the MIPSGAL survey can be found here.
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MIPSGAL_Continuum_Data_Access.pdf
MIPSGAL_Continuum_Data_Access.pdf
Sep 5, 2016 - MIPSGAL Extended Observations: Continuum (2D)
Adobe PDF - 30.4 KB - MD5: c676ad3027d90ff7644ee26265c9f163
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