Table 1: 22.5 GHz fluxes derived from the new VLA observations.
Source RA Dec Source flux Phase cal Phase cal flux
  (J2000) (J2000) (mJy) (J2000) (Jy)
NGC 34* 00 11 06.550 -12 06 26.33 $7.41 \pm 0.14$ 2358-103 $0.5719 \pm 0.005$
IC 1623 01 07 47.49 -17 30 26.3 $21.7 \pm 2.0$ 0050-094 $0.805 \pm 0.007$
CGCG436-30* 01 20 02.722 +14 21 42.94 $8.73 \pm 0.31$ 0121+118 $1.177 \pm 0.007$
IRAS 01364-1042* 01 38 52.870 -10 27 11.70 $3.97 \pm 0.19$ 0141-094 $0.7395 \pm 0.003$
IIIZw 35 01 44 30.53 +17 06 08.5 $9.7 \pm 0.3$ 0121+118 $1.449 \pm 0.011$
UGC 2369 02 54 01.81 +14 58 14.5 $5.3 \pm 0.3$ 0238+166 $2.041 \pm 0.015$
IRAS 03359+1523 03 38 47.12 +15 32 53.5 $4.5 \pm 0.3$ 0325+226 $0.768 \pm 0.006$
NGC 1614 04 34 00.02 -08 34 44.98 $21.0 \pm 1$ 0423-013 $7.480 \pm 0.058$
NGC 2623 08 38 24.08 +25 45 16.40 $18.3 \pm 0.2$ 0830+241 $1.822 \pm 0.013$
IRAS 08572+3915* 09 00 25.390 +39 03 54.40 $3.18 \pm 0.3$ 0927+390 $7.688 \pm 0.15$
UGC 4881 09 15 55.52 +44 19 57.5 $3.5 \pm 0.5$ 0920+446 $2.140 \pm 0.010$
UGC 5101 09 35 51.72 +61 21 11.29 $18.0 \pm 1.0$ 0958+655 $0.972 \pm 0.010$
IRAS 10173+0828 10 20 00.22 +08 13 34.5 $2.9 \pm 0.4$ 1041+061 $1.672 \pm 0.009$
Arp 148 11 03 53.95 +40 50 59.5 $6.1 \pm 0.3$ 1146+399 $1.330 \pm 0.012$
UGC 6436 11 25 45.15 +14 40 29.4 $2.8 \pm 0.5$ 1118+125 $1.238 \pm 0.016$
IRAS 12112+0305 12 13 46.1 +02 48 41.5 $5.7 \pm 0.3$ 1224+035 $0.788 \pm 0.006$
UGC 8387 13 20 35.34 +34 08 22.19 $7.5 \pm 2.0$ 1310+323 $0.963 \pm 0.042$
UGC 8696 13 44 42.11 +55 53 13.15 $14.3 \pm 0.3$ 1419+543 $0.935 \pm 0.023$
IRAS 14348-1447 14 37 38.30 -15 00 24.0 $4.5 \pm 0.5$ 1448-163 $0.376 \pm 0.006$
IZw 107 15 18 06.07 +42 44 45.19 $3.6 \pm 0.3$ 1521+436 $0.195 \pm 0.005$
IRAS 15250+3609 15 26 59.40 +35 58 37.53 $4.2 \pm 0.3$ 1521+436 $0.195 \pm 0.005$
NGC 6286 16 58 31.70 +58 56 14.50 $12.2 \pm 1.5$ 1638+573 $1.259 \pm 0.018$
NGC 7469* 23 03 15.623 +08 52 26.39 $17.50 \pm 0.50$ 2320+052 $0.5661 \pm 0.004$
IC 5298* 23 16 00.690 +25 33 24.20 $3.86 \pm 0.18$ 2321+275 $0.7178 \pm 0.009$
Mrk 331* 23 51 26.802 +20 35 09.87 $9.95 \pm 0.29$ 2358+199 $0.2683 \pm 0.002$

* Observations described in Prouton et al. (2004).


Source LaTeX | All tables | In the text