The wind and the magnetospheric accretion onto the T Tauri star S Coronae Australis at sub-au resolution

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Table 1

Observation log of the VLTI/GRAVITY high-resolution (R ~ 4000) observations of S CrA North and South conducted with the UTs.

UT Date	Tot. Int. S CrA N	Tot. Int. S CrA S	DIT^a	NDIT^b	Proj. baselines	PA^c	Calibrator	UD diameter^d
	[s]	[s]	[s]	#	[m]	[°]		[mas]

2016-07-20	2100	600	60	5	42, 52, 60, 81, 93, 115	53, 38, 130, 100, 45, 76	HD 188787	0.252 ± 0.018
2016-08-16	1200	1200	60	5	47, 56, 59, 87, 102, 130	31, 18, 100, 70, 24, 50	HD 176047	0.309 ± 0.021

Notes.

^(a)

Detector integration time per interferogram.

^(b)

Number of interferograms.

^(c)

Baseline position angle from the shortest to longest baseline.

^(d)

The calibrator uniform-disc (UD) diameter (K band) was taken from Lafrasse et al. (2010).

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