The origin of mid-infrared emission in massive young stellar objects: multi-baseline VLTI observations of W33A

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Table 1:

List of MIDI observations of W33A.
	UT date	Stations	B	PA	Seeing^a
			(m)	( $^\circ$ )	( $^{\prime \prime }$ )
Config. A	2008-06-21	U2-U3	42.03	15.04	0.65
Config. B	2008-04-22	U3-U4	57.95	119.69	1.08
Config. C	2008-04-21	U3-U4	61.08	114.57	0.52
Config. D	2005-09-16	U2-U3	45.58	47.31	1.00

Notes. Executed in the high-sens mode at a spectral resolution of R=30. Configuration D was already presented in de Wit et al. (2007). ^(a) Seeing is the one measured by the DIMM.

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