\begin{table}%t1
\caption{22.5~GHz fluxes derived from the new VLA observations.}\label{tab:cal}
\small%\centerline
 {
\begin{tabular}{c c c c c c}
\hline\hline
Source & RA & Dec & Source flux & Phase cal & Phase cal flux \\
   & (J2000) & (J2000) & (mJy) & (J2000) & (Jy)  \\
\hline
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 & $0.2683 \pm 0.002$  \\
\hline
\end{tabular}}
\medskip
$^*$ Observations described in Prouton et~al. (\cite{Prou04}).
\end{table}