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   PR # 41149
   We propose to observe a narrow-line quasar IRAS 20181-2244. The
   luminosity of the galaxy is comparable to that of QSOs both at
   optical and X-ray region, and its luminosity ratio of X-ray to
   infrared is typical of those of bare AGNs. However its optical
   spectrum is typical of Seyfert 2s. If the AGN is obscured as
   predicted in the unified scheme of AGN, its intrinsic X-ray to
   infrared luminosity ratio becomes unbelievably large. The current
   observation is to test if there is a indded buried AGN in this
   galaxy. This is a crucial test for the unified scheme of AGN; are all
   type 2 AGN indeed obscured type 1s or are there two types of Seyfert
   2s; those with obscured broad line regions (BLRs) and those without
   BLRs ?
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