Locating dust and molecules in the inner circumstellar environment of R Sculptoris with MATISSE

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Table A.1

Log of the MATISSE observations of R Scl.

Observing date	VLTI config.	BLR	N/N_*	Seeing	τ₀
2018-12-03 → 05	A0–B2–C1–J2	10–129	9/14	0.94	0.6
2018-12-07 → 08	A0–B2–C1–D0	9–34	6/7	0.94	2.3
2018-12-09	B2–D0–J3–K0	29–137	5/5	0.73	4.1
2018-12-10 → 11	D0–G2–J3–K0	34–104	10/10	0.82	4.0
2018-12-12	A0–D0–G1–J3	25–131	4/4	0.80	4.6
2018-12-13 → 14	A0–G1–J2–J3	39–132	9/9	0.67	5.0
2018-12-15	A0–G1–J2–K0	48–123	2/2	0.53	4.7

Notes: BLR stands for Baseline Length Range expressed in m covered with each VLTI configuration. The ratio N/N_* is the ratio of the used files to the pointings to the star, the seeing in arcseconds, and τ₀ is the coherence time in ms.

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