IRAS 20181-2244, with a 60 micron luminosity of 1.4*10^12 Solar
 luminosity and an unreddened absolute visual magnitude of -24.7,
 is the most luminous of the two known narrow line quasars. It
 lies at a redshift of 0.185 and has IRAS fluxes of 10 mJy at 12
 micron to almost 1 Jy at 100 microns. It has been suggested that
 its BLR is totally obscured by a dusty torus. The fact that it
 is the brightest of only two known narrow line quasars makes it
 a highly unusual object worthy of observation.

 We propose to obtain PHOT far-IR photometry, CAM polarimetry and
 SWS line spectra of this object. The PHOT photometry will enable
 us to determine if there is a turnover in the flux at long
 wavelengths and hence determine the dust temperature (assuming
 dust is present). CAM polarimetry will enable us to measure any
 polarisation due to a dusty torus and provide near-IR fluxes. Based
 on optical line data and models we calculate only one line will be
 strong enough to detect: the [OIV] 26 micron line. We therefore
 propose an SWS observation of that line to verify the models and
 calculations. If the line is stronger than predicted and there is
 a second call we will then propose observations of other lines.