Table B.4:

Complete results of VLA observations at 6.9 mm and 1.3, 3.5, and 6.2 cm.

Obs. date	Effective	Target sourcea	Continuum fluxb		rmsc	Gaussian size	RAb	Decb
	wavelength		(Peak)	(Integ.)		(arcsec)	(J2000)	(J2000)
	(mm)		(mJy)		(mJy/bm)
20080310	6.93	CoKu Ser G3	<1.2d		0.4	-	18 29 01.8	+00 29 54.5
		182900.88+002931.5	<0.7d		0.2	-	18 29 00.9	+00 29 31.5
		EC 90	<1.0d		0.3	-	18 29 57.7	+01 14 05.7
		VV Ser	<0.7d		0.2	-	18 28 47.9	+00 08 39.8
		EC 97	<0.6d		0.2	-	18 29 58.2	+01 15 21.7
		182850.20+000949.7	<0.6d		0.2	-	18 28 50.2	+00 09 49.6
		EC 82	<0.5d		0.2	-	18 29 56.9	+01 14 46.4
20080311	13.4	CoKu Ser G3	8.66	9.81	0.06		18 29 01.8	+00 29 54.8
		182900.88+002931.5	<0.17d		0.06	-	18 29 00.9	+00 29 31.5
		EC 90	<0.24d		0.08	-	18 29 57.7	+01 14 05.7
		VV Ser	<0.17d		0.06	-	18 28 47.9	+00 08 39.8
		EC 97	<0.15d		0.05	-	18 29 58.2	+01 15 21.7
20080313	13.4	182850.20+000949.7	<0.20d		0.07	-	18 28 50.2	+00 09 49.6
		182909.80+003445.9	<0.23d		0.08	-	18 29 09.8	+00 34 45.8
		EC 82	<0.28d		0.09	-	18 29 56.9	+01 14 46.4
20080314	35.5	EC 82	<0.09d		0.03	-	18 29 56.0	+01 14 49.9
		EC 90	<0.09d		0.03	-	18 29 56.0	+01 14 49.0
		EC 97	<0.09d		0.03	-	18 29 56.0	+01 14 49.0
		CoKu Ser G3	1.11	1.11	0.03		18 29 01.8	+00 29 54.7
		182900.88+002931.5	<0.10d		0.03	-	18 29 05.0	+00 29 44.0
		VV Ser	0.14	0.17	0.03		18 28 47.9	+00 08 40.1
		182850.20+000949.7	<0.08d		0.03	-	18 28 40.0	+00 09 13.0
20080315	61.7	EC 82	<0.09d		0.03	-	18 29 57.0	+01 14 40.0
		EC 90	<0.09d		0.03	-	18 29 57.0	+01 14 40.0
		EC 97	<0.09d		0.03	-	18 29 57.0	+01 14 40.0
		CoKu Ser G3	0.91	1.00	0.04	(unresolved)	18 29 01.9	+00 29 54.9
		182900.88+002931.5	<0.12d		0.04	-	18 29 07.0	+00 32 09.0
		VV Ser	<0.14d		0.05	-	18 29 47.0	+00 09 11.0
		182850.20+000949.7	<0.14d		0.05	-	18 29 47.0	+00 09 11.0

Notes. ^(a) In the case of SSTc2d names, only the coordinates (in J2000) are shown.
^(b) Continuum flux and position are obtained using the AIPS task JMFIT, which fits elliptical Gaussians to the cleaned image. For sources that were detected at 3, both the peak (Peak) and the integrated (Integ.) flux are shown. For sources that were not detected, the coordinates of the phase centre are quoted.
^(c) Calculated from the cleaned image.
^(d) Quoted value is 3 upper limit.