114   04497+1410   1030   o1 Ori; extended at 60 mum; binary with hot WD 
                           companion (Ake & Johnson 1988) 
 347   07245+4605   0013   Y Lyn, extended according to Young et al. (1993)
 845   14121-5155   2410   Source extended at 12 and 25 mum, strongly 
                           variable according to GSC; indices not typical for 
                           a stellar source, although no background galaxy is 
                           seen on ESO Schmidt plates 
 903   15492+4837   0110   ST Her, extended according to Young et al. (1993) 
 919   16156-5030   5521   Also listed as a planetary nebula (PK 332-0.2);
                           high background at 12 and 25 mum
1150   19354+5005   0000   R Cyg, extended according to Young et al. (1993)  
1165   19486+3247   2100   chi Cyg, very bright IRAS source, extended according
                           to Young et al. (1993) and Bujarrabal & Alcolea 
                           (1991), but with possible cirrus contamination
1196   20120-4433   0003   RZ Sgr (Li-rich), extended according to Young et al.
                           (1993); associated with an optical nebula 
                           (Whitelock 1994)
1294   22196-4612   2200   pi1 Gru, very bright IRAS source. Feast (1953) 
                           notices that there is a G0V companion having the 
                           same radial velocity 2.7" away; Sahai (1992)
                           discovered a bipolar mass outflow from CO 
                           observations; source extended at 60 mum according to
                           Young et al. (1993)
1314   22512+6100   0220   Possibly extended at 60 mum (FWHM = 2.5')