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   62131
   We propose to observe with ASCA two new infrared-loud quasars with warm
   absorbers: IRAS~04392-2713 (z=0.08) and IRAS~F22497+1439 (z=0.135).
   While `Warm' (i.e. partially ionized) absorbers have been studied in
   detail in many low luminosity AGN, only a few cases have even been
   identified at high luminosities. Our systematic search of bright ROSAT
   sources in WGACAT has found a few new cases, of which two are also IRAS
   sources. ASCA spectra of these two quasars will allow us to test for
   the differences in warm absorber ionization state and column density,
   with luminosity and with infrared properties. Being infrared-loud the
   quasars may offer new examples of ``dusty-warm-absorbers'', as are half
   the quasar warm absorbers already known.
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