Grain growth across protoplanetary discs: 10 μm silicate feature versus millimetre slope

D. J. P. Lommen; E. F. van Dishoeck; C. M. Wright; S. T. Maddison; M. Min; D. J. Wilner; D. M. Salter; H. J. van Langevelde; T. L. Bourke; R. F. J. van der Burg; G. A. Blake

doi:10.1051/0004-6361/200913150

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Volume 515 (June 2010)

A&A, 515 (2010) A77

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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 source^a	Continuum flux^b		rms^c	Gaussian size	RA^b	Dec^b
	wavelength		(Peak)	(Integ.)		(arcsec)	(J2000)	(J2000)
	(mm)		(mJy)		(mJy/bm)
20080310	6.93	CoKu Ser G3	<1.2^d		0.4	-	18 29 01.8	+00 29 54.5
		182900.88+002931.5	<0.7^d		0.2	-	18 29 00.9	+00 29 31.5
		EC 90	<1.0^d		0.3	-	18 29 57.7	+01 14 05.7
		VV Ser	<0.7^d		0.2	-	18 28 47.9	+00 08 39.8
		EC 97	<0.6^d		0.2	-	18 29 58.2	+01 15 21.7
		182850.20+000949.7	<0.6^d		0.2	-	18 28 50.2	+00 09 49.6
		EC 82	<0.5^d		0.2	-	18 29 56.9	+01 14 46.4
20080311	13.4	CoKu Ser G3	8.66	9.81	0.06	$1.17 \times 0.91$	18 29 01.8	+00 29 54.8
		182900.88+002931.5	<0.17^d		0.06	-	18 29 00.9	+00 29 31.5
		EC 90	<0.24^d		0.08	-	18 29 57.7	+01 14 05.7
		VV Ser	<0.17^d		0.06	-	18 28 47.9	+00 08 39.8
		EC 97	<0.15^d		0.05	-	18 29 58.2	+01 15 21.7
20080313	13.4	182850.20+000949.7	<0.20^d		0.07	-	18 28 50.2	+00 09 49.6
		182909.80+003445.9	<0.23^d		0.08	-	18 29 09.8	+00 34 45.8
		EC 82	<0.28^d		0.09	-	18 29 56.9	+01 14 46.4
20080314	35.5	EC 82	<0.09^d		0.03	-	18 29 56.0	+01 14 49.9
		EC 90	<0.09^d		0.03	-	18 29 56.0	+01 14 49.0
		EC 97	<0.09^d		0.03	-	18 29 56.0	+01 14 49.0
		CoKu Ser G3	1.11	1.11	0.03	$2.49 \times 2.35$	18 29 01.8	+00 29 54.7
		182900.88+002931.5	<0.10^d		0.03	-	18 29 05.0	+00 29 44.0
		VV Ser	0.14	0.17	0.03	$3.25 \times 2.31$	18 28 47.9	+00 08 40.1
		182850.20+000949.7	<0.08^d		0.03	-	18 28 40.0	+00 09 13.0
20080315	61.7	EC 82	<0.09^d		0.03	-	18 29 57.0	+01 14 40.0
		EC 90	<0.09^d		0.03	-	18 29 57.0	+01 14 40.0
		EC 97	<0.09^d		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	<0.12^d		0.04	-	18 29 07.0	+00 32 09.0
		VV Ser	<0.14^d		0.05	-	18 29 47.0	+00 09 11.0
		182850.20+000949.7	<0.14^d		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 $\sigma$ , 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 $\sigma$ upper limit.

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