74 3 1 detected by Miralles et al. (1994ApJS...92..173M) at 2 and 6cm 74 3 2 (F=9.9 and 9.1 mJy, respectively) with VLA (D); also detected by 74 3 3 Hughes & McLeod 1994ApJ...427..857H) at 6cm (S=8.58 mJy) with VLA (C) 76 2 1 also undetected by McCutcheon et al. (1991AJ....101.1435M) at 6cm 76 2 2 with VLA (C). 78 2 1 Detected by Hughes & McLeod (1994ApJ...427..857H) at 6cm (S=15.79mJy) 78 2 2 with VLA (C). 93 S3, S5 2 1 2D gaussian fit did not converge to meaningful sizes; peak fluxes are 93 S3, S5 2 2 correct though. 97 1 1 source is unresolved 99 1 1 source is unresolved; radio peak is 15" from IRAS19095+0942. 104 2 1 detected by Kurtz et al. (1994ApJS...91..659K) at 3.6cm (S=1.5 mJy) 104 2 2 with VLA (B) 110 2 1 detected by Hughes & McLeod (1994ApJ...427..857H) at 6cm (S=2.21 mJy) 110 2 2 with VLA (C). 114 1 1 radio peaks are about 24" from IRAS20049+2721. 119 2 1 detected by Hughes & McLeod (1994ApJ...427..857H) at 6cm (S=0.85 mJy) 119 2 2 with VLA (C) - double int. time compared to us 121 2 1 detected and resolved by McCutcheon et al. (1991AJ....101.1435M) at 121 2 2 6cm (S=29 mJy) with VLA (C). 123 5 1 Detected by Kurtz et al. (1994ApJS...91..659K) at 2cm (S=67.6 mJy) and 123 5 2 3.6cm (S=109.1 mJy) with the VLA (B); also detected by Miralles et al. 123 5 3 (1994ApJS...92..173M) at 2 and 6cm (F=347 and 362 mJy, respectively) 123 5 4 with VLA (D); also detected by Hughes & McLeod (1994ApJ...427..857H) at 123 5 5 6cm (S=446.83 mJy) with VLA (C). 126 3 1 detected by McCutcheon et al. (1991AJ....101.1435M) at 6cm (S=108 mJy) 126 3 2 with VLA (C) - source is very extended (97"x40"), so possibly too 126 3 3 faint for us. 131 1 1 Source is unresolved 133 4 1 Radio source is extended and association is considered positive; 133 4 2 IRAS21078+5209 is 87" away and is not considered to be associated; 133 4 3 also detected by Miralles et al. (1994ApJS...92..173M) at 2 and 6cm 133 4 4 (F=31 and 40 mJy, respectively) with VLA (D). 151 1 1 Source is unresolved