  We present continuum observations of the edge-on spiral galaxy NGC 5775 at
617 MHz with the Giant Metrewave Radio Telescope (GMRT) and at 850 \mu m with
the Submillimetre Common-User Bolometer Array (SCUBA) on the James Clerk
Maxwell Telescope (JCMT). We report the detection of dust at high-latitudes,
extending to about 5 kpc from the disk of the galaxy, and spurs of non-thermal
radio emission. The 617 MHz and 850 \mu m distributions are compared with one
another and we find a strong correlation between metre wavelength radio
emission and sub-mm emission in the disk and at high-latitudes. This suggests
that there may be a more fundamental relationship between cold dust and
synchrotron radiation other than the link via star formation.
