\begin{table}%tB.3
\caption{\label{tab: results log CARMA}Complete results of CARMA observations at 1 and 3~mm.}
%\centering
\par
\begin{tabular}{lcccccccc}
\hline
\hline \noalign{\smallskip}
		Obs. date	& Effective	& Target source\tablefootmark{a}	& \multicolumn{2}{c}{Continuum flux\tablefootmark{b}}	& rms\tablefootmark{c}	& Gaussian size		& RA\tablefootmark{b}      	& Dec\tablefootmark{b}	\\
					& wavelength	&				& (P)			& (G)				&			& (arcsec)		& (J2000)		& (J2000)		\\
					& (mm)		&				& \multicolumn{2}{c}{(mJy)}		     		& (mJy/bm)		&			&			&			\\
\hline
			20080518	& 1.33		& GSC 00446-00153		& 43.6		     	& 50.5 	     			& 6.0			& $0.46 \pm 0.32$	& 18 30 06.2		& +00 42 33.6		\\
			20080618	& 3.15		& EC 82				& \multicolumn{2}{c}{${<}2.9$\tablefootmark{d}}			& 1.0			& --			& 18 29 56.8		& +01 14 46.0		\\
					&		& EC 90				& 11.3			& 11.6				& 1.0			& $1.69 \pm 0.97$	& 18 29 57.8		& +01 14 06.9		\\
					&		& 182900.88+002931.5		& 3.4			& 3.9				& 0.6			& (unresolved)		& 18 29 00.9		& +00 29 31.7		\\
					&		& IRAS 18268-0025		& \multicolumn{2}{c}{${<}1.9$\tablefootmark{d}}			& 0.6			& --			& 18 29 28.2		& -00 22 57.1		\\
					&		& CoKu Ser G3			& \multicolumn{2}{c}{${<}1.6$\tablefootmark{d}}			& 0.5			& --			& 18 29 01.8		& +00 29 54.6		\\
					&		& VV Ser			& \multicolumn{2}{c}{${<}1.8$\tablefootmark{d}}		     	& 0.6	     		& --			& 18 28 47.9		& +00 08 40.0 		\\
			20080619	& 3.15		& 182858.08+001724.4		& \multicolumn{2}{c}{${<}1.9$\tablefootmark{d}}			& 0.6			& --			& 18 28 58.1		& +00 17 24.4		\\
					&		& 182850.20+000949.7		& \multicolumn{2}{c}{${<}1.9$\tablefootmark{d}}		     	& 0.6  			& --			& 18 28 50.2		& +00 09 49.7 		\\
					&		& 182944.10+003356.1		& \multicolumn{2}{c}{${<}1.7$\tablefootmark{d}}			& 0.6			& --			& 18 29 44.1		& +00 33 56.1		\\
					&		& 182936.19+004216.7		& \multicolumn{2}{c}{${<}2.7$\tablefootmark{d}}		     	& 0.9	     		& --			& 18 29 36.2		& +00 42 16.7 		\\
			20080620	& 1.33		& EC 82				& \multicolumn{2}{c}{${<}15.7$\tablefootmark{d}}		& 5.2			& --			& 18 29 56.8		& +01 14 46.0		\\
					&		& EC 90				& 91.8			& 91.7				& 10.4			& (unresolved)		& 18 29 57.7		& +01 14 07.0		\\
					&		& 182900.88+002931.5		& \multicolumn{2}{c}{${<}16.4$\tablefootmark{d}}		& 5.5		     	& --			& 18 29 00.9		& +00 29 31.6		\\
					&		& IRAS 18268-0025		& \multicolumn{2}{c}{${<}15.6$\tablefootmark{d}}		& 5.2			& --			& 18 29 28.2		& -00 22 57.1		\\
					&		& CoKu Ser G3			& \multicolumn{2}{c}{${<}17.1$\tablefootmark{d}}		& 5.7			& --			& 18 29 01.8		& +00 29 54.6		\\
					&		& VV Ser 			& \multicolumn{2}{c}{${<}14.8$\tablefootmark{d}}	     	& 4.9 			& --			& 18 29 47.9		& +00 08 40.0  		\\
					&		& 182858.08+001724.4		& \multicolumn{2}{c}{${<}24.6$\tablefootmark{d}}		& 8.2			& --			& 18 28 58.1		& +00 17 24.4		\\
					&		& 182850.20+000949.7		& \multicolumn{2}{c}{${<}98.2$\tablefootmark{d}}	     	& 32.7	     		& --			& 18 28 50.2		& +00 09 49.7 		\\
			20080622	& 3.15		& 182936.19+004216.7		& \multicolumn{2}{c}{${<}5.3$\tablefootmark{d}}			& 1.8			& --			& 18 29 36.2		& +00 42 16.7		\\
					&		& GSC 00446-00153		& 6.8		     	& 8.1	 	       		& 1.0			& $2.71 \pm 1.58$	& 18 30 06.3		& +00 42 34.2 		\\
			20080704	& 1.33		& EC 97				& \multicolumn{2}{c}{${<}23.3$\tablefootmark{d}}		& 7.8			& --			& 18 29 58.2		& +01 15 22.0		\\
					&		& 182850.20+000949.7		& \multicolumn{2}{c}{${<}22.8$\tablefootmark{d}}	     	& 7.6	     		& --			& 18 28 50.2		& +00 09 49.7		\\
					&		& 182944.10+003356.1 		& \multicolumn{2}{c}{${<}15.0$\tablefootmark{d}}		& 5.0			& --			& 18 29 44.1		& +00 35 56.1	     	\\
					&		& 182936.19+004216.7		& \multicolumn{2}{c}{${<}8.7$\tablefootmark{d}}			& 2.9			& --			& 18 29 36.2		& +00 42 16.7		\\
					&		& GSC 00446-00153		& 90.8		     	& 97.6 		     		& 2.8			& $0.67 \pm 0.23$	& 18 30 06.2  		& +00 42 33.6		\\
\hline
\end{tabular}
\tablefoot {\tablefoottext{a}{In the case of SSTc2d names, only the coordinates (in J2000) are shown. } \\
\tablefoottext{b}{Continuum flux and position are from fits in the ($u$,~$v$)~plane. For sources that were detected at~3$\sigma$, both the point-source flux~(P) and the integrated flux for a Gaussian~(G) are shown. For sources that were not detected, the coordinates of the phase centre are quoted.} \\
\tablefoottext{c}{Calculated from the cleaned image.} \\
\tablefoottext{d}{Quoted value is 3$\sigma$ upper limit.}}
\end{table}